BibTeX 用文献リストをつくってみた。Tさんの使い方を参考にして書式は note に直打ちすることにした。sort できないって warning 吐くけど気にしない。あと Abstract にアブストを、Keywords に実験名などキーワードを書く。Keywords 書いておくと BibDesk で探しやすくなる。BibTeX 使い始めたとこなのでこれからどうなるかは分からない。
dvipdfmx の hyperref が必要。自分の環境では \usepackage[dvipdfmx]{graphicx,hyperref,psfrag,color}
久しぶりに BibDesk 起動してアップデートしたら、なんかいい感じになってる気がする。Local Files というフィールドが出来てて、ローカルファイルを登録できて、すぐ飛べる！ これなら論文を適当な場所に置いても困らない！ Dropbox に PDF を置いて、BibDesk に登録すれば Mendeley 要らず。
BibTeX 用文献リストをつくってみた。Tさんの使い方を参考にして書式は note に直打ちすることにした。sort できないって warning 吐くけど気にしない。あと Abstract にアブストを、Keywords に実験名などキーワードを書く。Keywords 書いておくと BibDesk で探しやすくなる。BibTeX 使い始めたとこなのでこれからどうなるかは分からない。
dvipdfmx の hyperref が必要。自分の環境では \usepackage[dvipdfmx]{graphicx,hyperref,psfrag,color}
久しぶりに BibDesk 起動してアップデートしたら、なんかいい感じになってる気がする。Local Files というフィールドが出来てて、ローカルファイルを登録できて、すぐ飛べる！ これなら論文を適当な場所に置いても困らない！ Dropbox に PDF を置いて、BibDesk に登録すれば Mendeley 要らず。
| %% This BibTeX bibliography file was created using BibDesk. | |
| %% http://bibdesk.sourceforge.net/ | |
| %% Created for OKA Naoya at 2016-11-22 15:56:10 +0900 | |
| %% Saved with string encoding Unicode (UTF-8) | |
| @article{1921SPAW.......966K, | |
| Adsnote = {Provided by the SAO/NASA Astrophysics Data System}, | |
| Adsurl = {http://adsabs.harvard.edu/abs/1921SPAW.......966K}, | |
| Author = {{Kaluza}, T.}, | |
| Date-Added = {2016-11-22 06:55:17 +0000}, | |
| Date-Modified = {2016-11-22 06:55:17 +0000}, | |
| Journal = {Sitzungsberichte der K{\"o}niglich Preu{\ss}ischen Akademie der Wissenschaften (Berlin), Seite p.~966-972}, | |
| Pages = {966-972}, | |
| Title = {{Zum Unit{\"a}tsproblem der Physik}}, | |
| Year = 1921} | |
| @article{Klein1926, | |
| Abstract = {Auf den folgenden Seiten m{\"o}chte ich auf einen einfachen Zusammenhang hinweisen zwischen der von Kaluza vorgeschlagenen Theorie f{\"u}r den Zusammenhang zwischen Elektromagnetismus und Gravitation einerseits und der von de Broglie und Schr{\"o}dinger angegebenen Methode zur Behandlung der Quantenprobleme andererseits. Die Theorie von Kaluza geht darauf hinaus, die zehn Einsteinschen Gravitationspotentiale gik und die vier elektromagnetischen Potentiale ϕi in Zusammenhang zu bringen mit den Koeffizienten $\gamma$ik eines Linienelementes von einem Riemannschen Raum, der au{\ss}er den vier gew{\"o}hnlichen Dimensionen noch eine f{\"u}nfte Dimension enth{\"a}lt. Die Bewegungsgleichungen der elektrischen Teilchen nehmen hierbei auch in elektromagnetischen Feldern die Gestalt von Gleichungen geod{\"a}tischer Linien an. Wenn dieselben als Strahlengleichungen gedeutet werden, indem die Materie als eine Art Wellenausbreitung betrachtet wird, kommt man fast von selbst zu einer partiellen Differentialgleichung zweiter Ordnung, die als eine Verallgemeinerung der gew{\"o}hnlichen Wellengleichung angesehen werden kann. Werden nun solche L{\"o}sungen dieser Gleichung betrachtet, bei denen die f{\"u}nfte Dimension rein harmonisch auftritt mit einer bestimmten mit der Planckschen Konstante zusammenh{\"a}ngenden Periode, so kommt man eben zu den obenerw{\"a}hnten quantentheoretischen Methoden.}, | |
| Author = {Klein, Oskar}, | |
| Date-Added = {2016-11-22 06:48:36 +0000}, | |
| Date-Modified = {2016-11-22 06:48:36 +0000}, | |
| Doi = {10.1007/BF01397481}, | |
| Issn = {0044-3328}, | |
| Journal = {Zeitschrift f{\"u}r Physik}, | |
| Number = {12}, | |
| Pages = {895--906}, | |
| Title = {Quantentheorie und f{\"u}nfdimensionale Relativit{\"a}tstheorie}, | |
| Url = {http://dx.doi.org/10.1007/BF01397481}, | |
| Volume = {37}, | |
| Year = {1926}, | |
| Bdsk-Url-1 = {http://dx.doi.org/10.1007/BF01397481}} | |
| @article{PhysRevD.92.092003, | |
| Author = {Pendlebury, J. M. and Afach, S. and Ayres, N. J. and Baker, C. A. and Ban, G. and Bison, G. and Bodek, K. and Burghoff, M. and Geltenbort, P. and Green, K. and Griffith, W. C. and van der Grinten, M. and Gruji\ifmmode \acute{c}\else \'{c}\fi{}, Z. D. and Harris, P. G. and H\'elaine, V. and Iaydjiev, P. and Ivanov, S. N. and Kasprzak, M. and Kermaidic, Y. and Kirch, K. and Koch, H.-C. and Komposch, S. and Kozela, A. and Krempel, J. and Lauss, B. and Lefort, T. and Lemi\`ere, Y. and May, D. J. R. and Musgrave, M. and Naviliat-Cuncic, O. and Piegsa, F. M. and Pignol, G. and Prashanth, P. N. and Qu\'em\'ener, G. and Rawlik, M. and Rebreyend, D. and Richardson, J. D. and Ries, D. and Roccia, S. and Rozpedzik, D. and Schnabel, A. and Schmidt-Wellenburg, P. and Severijns, N. and Shiers, D. and Thorne, J. A. and Weis, A. and Winston, O. J. and Wursten, E. and Zejma, J. and Zsigmond, G.}, | |
| Date-Added = {2016-11-09 00:57:50 +0000}, | |
| Date-Modified = {2016-11-09 00:57:50 +0000}, | |
| Doi = {10.1103/PhysRevD.92.092003}, | |
| Issue = {9}, | |
| Journal = {Phys. Rev. D}, | |
| Month = {Nov}, | |
| Numpages = {22}, | |
| Pages = {092003}, | |
| Publisher = {American Physical Society}, | |
| Title = {Revised experimental upper limit on the electric dipole moment of the neutron}, | |
| Url = {http://link.aps.org/doi/10.1103/PhysRevD.92.092003}, | |
| Volume = {92}, | |
| Year = {2015}, | |
| Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.92.092003}, | |
| Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.92.092003}} | |
| @article{PhysRevLett.83.3370, | |
| Author = {Randall, Lisa and Sundrum, Raman}, | |
| Date-Added = {2016-11-08 07:46:45 +0000}, | |
| Date-Modified = {2016-11-08 07:46:45 +0000}, | |
| Doi = {10.1103/PhysRevLett.83.3370}, | |
| Issue = {17}, | |
| Journal = {Phys. Rev. Lett.}, | |
| Month = {Oct}, | |
| Numpages = {0}, | |
| Pages = {3370--3373}, | |
| Publisher = {American Physical Society}, | |
| Title = {Large Mass Hierarchy from a Small Extra Dimension}, | |
| Url = {http://link.aps.org/doi/10.1103/PhysRevLett.83.3370}, | |
| Volume = {83}, | |
| Year = {1999}, | |
| Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevLett.83.3370}, | |
| Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevLett.83.3370}} | |
| @article{PhysRevD.66.053010, | |
| Author = {Fogli, G. L. and Lisi, E. and Marrone, A. and Montanino, D. and Palazzo, A.}, | |
| Date-Added = {2016-11-02 01:39:12 +0000}, | |
| Date-Modified = {2016-11-02 01:39:12 +0000}, | |
| Doi = {10.1103/PhysRevD.66.053010}, | |
| Issue = {5}, | |
| Journal = {Phys. Rev. D}, | |
| Month = {Sep}, | |
| Numpages = {22}, | |
| Pages = {053010}, | |
| Publisher = {American Physical Society}, | |
| Title = {Getting the most from the statistical analysis of solar neutrino oscillations}, | |
| Url = {http://link.aps.org/doi/10.1103/PhysRevD.66.053010}, | |
| Volume = {66}, | |
| Year = {2002}, | |
| Bdsk-File-1 = {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}, | |
| Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.66.053010}, | |
| Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.66.053010}} | |
| @article{PhysRevD.58.055006, | |
| Author = {Kim, Jihn E.}, | |
| Date-Added = {2016-10-24 14:19:58 +0000}, | |
| Date-Modified = {2016-10-24 14:19:58 +0000}, | |
| Doi = {10.1103/PhysRevD.58.055006}, | |
| Issue = {5}, | |
| Journal = {Phys. Rev. D}, | |
| Month = {Jul}, | |
| Numpages = {4}, | |
| Pages = {055006}, | |
| Publisher = {American Physical Society}, | |
| Title = {Constraints on very light axions from cavity experiments}, | |
| Url = {http://link.aps.org/doi/10.1103/PhysRevD.58.055006}, | |
| Volume = {58}, | |
| Year = {1998}, | |
| Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.58.055006}, | |
| Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.58.055006}} | |
| @article{Bertone2005279, | |
| Abstract = {In this review article, we discuss the current status of particle dark matter, including experimental evidence and theoretical motivations. We discuss a wide array of candidates for particle dark matter, but focus on neutralinos in models of supersymmetry and Kaluza--Klein dark matter in models of universal extra dimensions. We devote much of our attention to direct and indirect detection techniques, the constraints placed by these experiments and the reach of future experimental efforts. }, | |
| Author = {Gianfranco Bertone and Dan Hooper and Joseph Silk}, | |
| Date-Added = {2016-10-23 14:27:20 +0000}, | |
| Date-Modified = {2016-10-23 14:27:20 +0000}, | |
| Doi = {http://dx.doi.org/10.1016/j.physrep.2004.08.031}, | |
| Issn = {0370-1573}, | |
| Journal = {Physics Reports}, | |
| Number = {5--6}, | |
| Pages = {279 - 390}, | |
| Title = {Particle dark matter: evidence, candidates and constraints}, | |
| Url = {http://www.sciencedirect.com/science/article/pii/S0370157304003515}, | |
| Volume = {405}, | |
| Year = {2005}, | |
| Bdsk-Url-1 = {http://www.sciencedirect.com/science/article/pii/S0370157304003515}, | |
| Bdsk-Url-2 = {http://dx.doi.org/10.1016/j.physrep.2004.08.031}} | |
| @inproceedings{Ponton:2012bi, | |
| Archiveprefix = {arXiv}, | |
| Author = {Ponton, Eduardo}, | |
| Booktitle = {{The Dark Secrets of the Terascale: Proceedings, TASI 2011, Boulder, Colorado, USA, Jun 6 - Jul 11, 2011}}, | |
| Date-Added = {2016-10-23 14:23:33 +0000}, | |
| Date-Modified = {2016-10-23 14:23:33 +0000}, | |
| Doi = {10.1142/9789814390163_0007}, | |
| Eprint = {1207.3827}, | |
| Pages = {283-374}, | |
| Primaryclass = {hep-ph}, | |
| Slaccitation = {%%CITATION = ARXIV:1207.3827;%%}, | |
| Title = {{TASI 2011: Four Lectures on TeV Scale Extra Dimensions}}, | |
| Url = {https://inspirehep.net/record/1122856/files/arXiv:1207.3827.pdf}, | |
| Year = {2013}, | |
| Bdsk-Url-1 = {https://inspirehep.net/record/1122856/files/arXiv:1207.3827.pdf}, | |
| Bdsk-Url-2 = {http://dx.doi.org/10.1142/9789814390163_0007}} | |
| @article{PhysRevD.65.087701, | |
| Author = {Horvat, R. and Kr\ifmmode \check{c}\else \v{c}\fi{}mar, M. and Laki\ifmmode \acute{c}\else \'{c}\fi{}, B.}, | |
| Date-Added = {2016-10-22 15:31:22 +0000}, | |
| Date-Modified = {2016-10-22 15:31:22 +0000}, | |
| Doi = {10.1103/PhysRevD.65.087701}, | |
| Issue = {8}, | |
| Journal = {Phys. Rev. D}, | |
| Month = {Mar}, | |
| Numpages = {4}, | |
| Pages = {087701}, | |
| Publisher = {American Physical Society}, | |
| Title = {Recent searches for solar axions and large extra dimensions}, | |
| Url = {http://link.aps.org/doi/10.1103/PhysRevD.65.087701}, | |
| Volume = {65}, | |
| Year = {2002}, | |
| Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.65.087701}, | |
| Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.65.087701}} | |
| @article{Lakic:2008zza, | |
| Author = {Lakic, Biljana and Horvat, Raul and Krcmar, Milica}, | |
| Booktitle = {{Axions: Theory, cosmology, and experimental searches. Proceedings, 1st Joint ILIAS-CERN-CAST axion training, Geneva, Switzerland, November 30-December 2, 2005}}, | |
| Date-Added = {2016-10-22 15:27:51 +0000}, | |
| Date-Modified = {2016-10-22 15:27:51 +0000}, | |
| Doi = {10.1007/978-3-540-73518-2_4}, | |
| Journal = {Lect. Notes Phys.}, | |
| Note = {[,73(2008)]}, | |
| Pages = {73-82}, | |
| Slaccitation = {%%CITATION = LNPHA,741,73;%%}, | |
| Title = {{Axions and large extra dimensions}}, | |
| Volume = {741}, | |
| Year = {2008}, | |
| Bdsk-Url-1 = {http://dx.doi.org/10.1007/978-3-540-73518-2_4}} | |
| @article{doi:10.1142/S0217751X10050421, | |
| Author = {NAMATAME, HARUKA}, | |
| Date-Added = {2016-10-22 14:18:37 +0000}, | |
| Date-Modified = {2016-10-22 14:18:37 +0000}, | |
| Doi = {10.1142/S0217751X10050421}, | |
| Eprint = {http://www.worldscientific.com/doi/pdf/10.1142/S0217751X10050421}, | |
| Journal = {International Journal of Modern Physics A}, | |
| Number = {23}, | |
| Pages = {4511-4523}, | |
| Title = {A PROBLEM IN VIRTUAL GRAVITON EXCHANGES IN FLAT LARGE EXTRA DIMENSIONS}, | |
| Url = {http://www.worldscientific.com/doi/abs/10.1142/S0217751X10050421}, | |
| Volume = {25}, | |
| Year = {2010}, | |
| Bdsk-Url-1 = {http://www.worldscientific.com/doi/abs/10.1142/S0217751X10050421}, | |
| Bdsk-Url-2 = {http://dx.doi.org/10.1142/S0217751X10050421}} | |
| @phdthesis{500000915711, | |
| Author = {内田, 裕義 and Uchida, Hiroyoshi}, | |
| Date-Added = {2016-10-19 06:13:59 +0000}, | |
| Date-Modified = {2016-10-19 06:13:59 +0000}, | |
| School = {名古屋大学}, | |
| Title = {Search for WIMP-129Xe inelastic scattering in the XMASS large low background liquid Xe detector}, | |
| Url = {http://ci.nii.ac.jp/naid/500000915711}, | |
| Year = {2014}, | |
| Bdsk-Url-1 = {http://ci.nii.ac.jp/naid/500000915711}} | |
| @article{PhysRevLett.112.131301, | |
| Author = {Sikivie, P. and Sullivan, N. and Tanner, D. B.}, | |
| Date-Added = {2016-10-12 21:30:09 +0000}, | |
| Date-Modified = {2016-10-12 21:30:09 +0000}, | |
| Doi = {10.1103/PhysRevLett.112.131301}, | |
| Issue = {13}, | |
| Journal = {Phys. Rev. Lett.}, | |
| Month = {Mar}, | |
| Numpages = {5}, | |
| Pages = {131301}, | |
| Publisher = {American Physical Society}, | |
| Title = {Proposal for Axion Dark Matter Detection Using an $LC$ Circuit}, | |
| Url = {http://link.aps.org/doi/10.1103/PhysRevLett.112.131301}, | |
| Volume = {112}, | |
| Year = {2014}, | |
| Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevLett.112.131301}, | |
| Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevLett.112.131301}} | |
| @article{PhysRevD.82.043007, | |
| Author = {Brax, Philippe and Zioutas, Konstantin}, | |
| Date-Added = {2016-10-12 19:13:00 +0000}, | |
| Date-Modified = {2016-10-12 19:13:00 +0000}, | |
| Doi = {10.1103/PhysRevD.82.043007}, | |
| Issue = {4}, | |
| Journal = {Phys. Rev. D}, | |
| Month = {Aug}, | |
| Numpages = {9}, | |
| Pages = {043007}, | |
| Publisher = {American Physical Society}, | |
| Title = {Solar chameleons}, | |
| Url = {http://link.aps.org/doi/10.1103/PhysRevD.82.043007}, | |
| Volume = {82}, | |
| Year = {2010}, | |
| Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.82.043007}, | |
| Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.82.043007}} | |
| @article{Derbin2011, | |
| Abstract = {Axions of energy 14.4 keV that originated from the M1 transition in 57Fe nuclei in the Sun were sought by using the resonance-absorption reaction A+57Fe {\textrightarrow} 57Fe* {\textrightarrow} 57Fe+$\gamma$ (14.4 keV). Asectioned Si(Li) detector arranged in a low-background facility was used to record photons from this reaction. This resulted in setting a new limit on the axion couplings to nucleons, |−1.19g AN 0 + g AN 3 | ≤ 3.0{\texttimes}10−6. Within the hadronic-axion model, the respective constraint on the axion mass is m A ≤ 145 eV (at a 95{\%} C.L.).}, | |
| Author = {Derbin, A. V. and Muratova, V. N. and Semenov, D. A. and Unzhakov, E. V.}, | |
| Date-Added = {2016-10-12 17:15:39 +0000}, | |
| Date-Modified = {2016-10-12 17:15:39 +0000}, | |
| Doi = {10.1134/S1063778811040041}, | |
| Issn = {1562-692X}, | |
| Journal = {Physics of Atomic Nuclei}, | |
| Number = {4}, | |
| Pages = {596--602}, | |
| Title = {New limit on the mass of 14.4-keV solar axions emitted in an M1 transition in 57Fe nuclei}, | |
| Url = {http://dx.doi.org/10.1134/S1063778811040041}, | |
| Volume = {74}, | |
| Year = {2011}, | |
| Bdsk-Url-1 = {http://dx.doi.org/10.1134/S1063778811040041}} | |
| @article{PhysRevD.94.042004, | |
| Author = {Yuzurihara, Hirotaka and Hayama, Kazuhiro and Mano, Shuhei and Verkindt, Didier and Kanda, Nobuyuki}, | |
| Date-Added = {2016-10-12 15:42:22 +0000}, | |
| Date-Modified = {2016-10-12 15:42:22 +0000}, | |
| Doi = {10.1103/PhysRevD.94.042004}, | |
| Issue = {4}, | |
| Journal = {Phys. Rev. D}, | |
| Month = {Aug}, | |
| Numpages = {7}, | |
| Pages = {042004}, | |
| Publisher = {American Physical Society}, | |
| Title = {Unveiling linearly and nonlinearly correlated signals between gravitational wave detectors and environmental monitors}, | |
| Url = {http://link.aps.org/doi/10.1103/PhysRevD.94.042004}, | |
| Volume = {94}, | |
| Year = {2016}, | |
| Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.94.042004}, | |
| Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.94.042004}} | |
| @article{PhysRevLett.75.3222, | |
| Author = {Moriyama, Shigetaka}, | |
| Date-Added = {2016-10-11 21:12:45 +0000}, | |
| Date-Modified = {2016-10-11 21:12:45 +0000}, | |
| Doi = {10.1103/PhysRevLett.75.3222}, | |
| Issue = {18}, | |
| Journal = {Phys. Rev. Lett.}, | |
| Month = {Oct}, | |
| Numpages = {0}, | |
| Pages = {3222--3225}, | |
| Publisher = {American Physical Society}, | |
| Title = {Proposal to Search for a Monochromatic Component of Solar Axions Using ${}^{57}$Fe}, | |
| Url = {http://link.aps.org/doi/10.1103/PhysRevLett.75.3222}, | |
| Volume = {75}, | |
| Year = {1995}, | |
| Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevLett.75.3222}, | |
| Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevLett.75.3222}} | |
| @article{PhysRevLett.113.201301, | |
| Author = {Sikivie, P.}, | |
| Date-Added = {2016-10-11 21:11:42 +0000}, | |
| Date-Modified = {2016-10-11 21:11:42 +0000}, | |
| Doi = {10.1103/PhysRevLett.113.201301}, | |
| Issue = {20}, | |
| Journal = {Phys. Rev. Lett.}, | |
| Month = {Nov}, | |
| Numpages = {5}, | |
| Pages = {201301}, | |
| Publisher = {American Physical Society}, | |
| Title = {Axion Dark Matter Detection Using Atomic Transitions}, | |
| Url = {http://link.aps.org/doi/10.1103/PhysRevLett.113.201301}, | |
| Volume = {113}, | |
| Year = {2014}, | |
| Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevLett.113.201301}, | |
| Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevLett.113.201301}} | |
| @article{ZIOUTAS198894, | |
| Abstract = {The coupling of axion to electron in atomic and molecular M1 or O− transitions is proposed to be used for the axion production by using a powerful maser/laser device. For their detection a resonance cavity tuned on the same frequency might well improve drastically the overall sensitivity.}, | |
| Author = {K. Zioutas and Y. Semertzidis}, | |
| Date-Added = {2016-10-11 21:11:03 +0000}, | |
| Date-Modified = {2016-10-11 21:11:03 +0000}, | |
| Doi = {http://dx.doi.org/10.1016/0375-9601(88)90245-9}, | |
| Issn = {0375-9601}, | |
| Journal = {Physics Letters A}, | |
| Number = {2}, | |
| Pages = {94 - 97}, | |
| Title = {A new detector scheme for axions}, | |
| Url = {http://www.sciencedirect.com/science/article/pii/0375960188902459}, | |
| Volume = {130}, | |
| Year = {1988}, | |
| Bdsk-Url-1 = {http://www.sciencedirect.com/science/article/pii/0375960188902459}, | |
| Bdsk-Url-2 = {http://dx.doi.org/10.1016/0375-9601(88)90245-9}} | |
| @article{PhysRevD.82.065006, | |
| Author = {Derevianko, A. and Dzuba, V. A. and Flambaum, V. V. and Pospelov, M.}, | |
| Date-Added = {2016-10-06 12:51:59 +0000}, | |
| Date-Modified = {2016-10-06 12:51:59 +0000}, | |
| Doi = {10.1103/PhysRevD.82.065006}, | |
| Issue = {6}, | |
| Journal = {Phys. Rev. D}, | |
| Month = {Sep}, | |
| Numpages = {8}, | |
| Pages = {065006}, | |
| Publisher = {American Physical Society}, | |
| Title = {Axio-electric effect}, | |
| Url = {http://link.aps.org/doi/10.1103/PhysRevD.82.065006}, | |
| Volume = {82}, | |
| Year = {2010}, | |
| Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.82.065006}, | |
| Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.82.065006}} | |
| @article{Morgan:2005xn, | |
| Author = {Morgan, B. and Spooner, N. J. C. and Armel-Funkhouser, M. S. and Snowden-Ifft, D. P. and Hoffmann, D. H. H. and Zioutas, K. and Jacoby, J.}, | |
| Date-Added = {2016-10-06 01:53:44 +0000}, | |
| Date-Modified = {2016-10-06 01:53:44 +0000}, | |
| Doi = {10.1016/j.astropartphys.2005.01.002}, | |
| Journal = {Astropart. Phys.}, | |
| Pages = {287-302}, | |
| Slaccitation = {%%CITATION = APHYE,23,287;%%}, | |
| Title = {{Searches for solar Kaluza--Klein axions with gas TPCs}}, | |
| Volume = {23}, | |
| Year = {2005}, | |
| Bdsk-Url-1 = {http://dx.doi.org/10.1016/j.astropartphys.2005.01.002}} | |
| @article{Abe:2015eos, | |
| Archiveprefix = {arXiv}, | |
| Author = {Abe, K. and others}, | |
| Collaboration = {XMASS}, | |
| Date-Added = {2016-10-05 08:45:50 +0000}, | |
| Date-Modified = {2016-10-05 08:45:50 +0000}, | |
| Doi = {10.1016/j.physletb.2016.05.081}, | |
| Eprint = {1511.04807}, | |
| Journal = {Phys. Lett.}, | |
| Pages = {272-276}, | |
| Primaryclass = {astro-ph.CO}, | |
| Slaccitation = {%%CITATION = ARXIV:1511.04807;%%}, | |
| Title = {{Direct dark matter search by annual modulation in XMASS-I}}, | |
| Volume = {B759}, | |
| Year = {2016}, | |
| Bdsk-Url-1 = {http://dx.doi.org/10.1016/j.physletb.2016.05.081}} | |
| @article{Takiya2016192, | |
| Abstract = {Abstract We report the measurement of the emission time profile of scintillation from gamma-ray induced events in the XMASS-I 832 kg liquid xenon scintillation detector. Decay time constant was derived from a comparison of scintillation photon timing distributions between the observed data and simulated samples in order to take into account optical processes such as absorption and scattering in liquid xenon. Calibration data of radioactive sources, 55Fe, 241Am, and 57Co were used to obtain the decay time constant. Assuming two decay components, τ1 and τ2, the decay time constant τ2 increased from 27.9 ns to 37.0 ns as the gamma-ray energy increased from 5.9 keV to 122 keV. The accuracy of the measurement was better than 1.5 ns at all energy levels. A fast decay component with τ 1 ∼ 2 ns was necessary to reproduce data. Energy dependencies of τ2 and the fraction of the fast decay component were studied as a function of the kinetic energy of electrons induced by gamma-rays. The obtained data almost reproduced previously reported results and extended them to the lower energy region relevant to direct dark matter searches. }, | |
| Author = {H. Takiya and K. Abe and K. Hiraide and K. Ichimura and Y. Kishimoto and K. Kobayashi and M. Kobayashi and S. Moriyama and M. Nakahata and T. Norita and H. Ogawa and H. Sekiya and O. Takachio and A. Takeda and S. Tasaka and M. Yamashita and B.S. Yang and N.Y. Kim and Y.D. Kim and Y. Itow and R. Kegasa and K. Kobayashi and K. Masuda and K. Fushimi and K. Martens and Y. Suzuki and R. Fujita and K. Hosokawa and K. Miuchi and N. Oka and Y. Onishi and Y. Takeuchi and Y.H. Kim and J.S. Lee and K.B. Lee and M.K. Lee and Y. Fukuda and K. Nishijima and S. Nakamura}, | |
| Date-Added = {2016-10-05 08:43:24 +0000}, | |
| Date-Modified = {2016-10-05 08:43:24 +0000}, | |
| Doi = {http://dx.doi.org/10.1016/j.nima.2016.08.014}, | |
| Issn = {0168-9002}, | |
| Journal = {Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment}, | |
| Keywords = {Scintillator}, | |
| Pages = {192 - 196}, | |
| Title = {A measurement of the time profile of scintillation induced by low energy gamma-rays in liquid xenon with the XMASS-I detector}, | |
| Url = {http://www.sciencedirect.com/science/article/pii/S0168900216308324}, | |
| Volume = {834}, | |
| Year = {2016}, | |
| Bdsk-Url-1 = {http://www.sciencedirect.com/science/article/pii/S0168900216308324}, | |
| Bdsk-Url-2 = {http://dx.doi.org/10.1016/j.nima.2016.08.014}} | |
| @article{1748-0221-11-02-C02034, | |
| Abstract = {XMASS-I, the first phase of the XMASS implementation, is dedicated to direct dark matter detection using 832 kg of liquid xenon as target material. To understand the detector response to nuclear recoils, we performed a neutron calibration using a 252 Cf source. In this presentation, we discuss the calibration setup and result. In particular we present the obtained scintillation decay time and scintillation efficiency. The MC reproducibility is also shown.}, | |
| Author = {K. Ichimura}, | |
| Date-Added = {2016-10-05 08:42:03 +0000}, | |
| Date-Modified = {2016-10-05 08:42:03 +0000}, | |
| Journal = {Journal of Instrumentation}, | |
| Number = {02}, | |
| Pages = {C02034}, | |
| Title = {XMASS detector calibration using a neutron source}, | |
| Url = {http://stacks.iop.org/1748-0221/11/i=02/a=C02034}, | |
| Volume = {11}, | |
| Year = {2016}, | |
| Bdsk-Url-1 = {http://stacks.iop.org/1748-0221/11/i=02/a=C02034}} | |
| @article{1742-6596-664-8-082018, | |
| Abstract = {The XMASS experiment aims to detect dark matter, pp and 7Be solar neutrinos, and neutrinoless double beta decay using highly purified liquid xenon located underground in the Kamioka Observatory in Japan. Construction of the detector was completed in September 2010 and data-taking started in December 2010. This paper discusses the design of the XMASS data acquisition system and its capabilities.}, | |
| Author = {Katsuki Hiraide}, | |
| Date-Added = {2016-10-05 08:40:01 +0000}, | |
| Date-Modified = {2016-10-05 08:40:01 +0000}, | |
| Journal = {Journal of Physics: Conference Series}, | |
| Number = {8}, | |
| Pages = {082018}, | |
| Title = {The data acquisition system of the XMASS experiment}, | |
| Url = {http://stacks.iop.org/1742-6596/664/i=8/a=082018}, | |
| Volume = {664}, | |
| Year = {2015}, | |
| Bdsk-Url-1 = {http://stacks.iop.org/1742-6596/664/i=8/a=082018}} | |
| @article{Abe201664, | |
| Abstract = {Abstract Double electron capture is a rare nuclear decay process in which two orbital electrons are captured simultaneously in the same nucleus. Measurement of its two-neutrino mode would provide a new reference for the calculation of nuclear matrix elements whereas observation of its neutrinoless mode would demonstrate lepton number violation. A search for two-neutrino double electron capture on 124Xe is performed using 165.9 days of data collected with the XMASS-I liquid xenon detector. No significant excess above background was observed and we set a lower limit on the half-life as 4.7 × 10 21 years at 90% confidence level. The obtained limit has ruled out parts of some theoretical expectations. We obtain a lower limit on the 126Xe two-neutrino double electron capture half-life of 4.3 × 10 21 years at 90% confidence level as well. }, | |
| Author = {K. Abe and K. Hiraide and K. Ichimura and Y. Kishimoto and K. Kobayashi and M. Kobayashi and S. Moriyama and K. Nakagawa and M. Nakahata and T. Norita and H. Ogawa and H. Sekiya and O. Takachio and A. Takeda and M. Yamashita and B.S. Yang and N.Y. Kim and Y.D. Kim and S. Tasaka and J. Liu and K. Martens and Y. Suzuki and R. Fujita and K. Hosokawa and K. Miuchi and N. Oka and Y. Onishi and Y. Takeuchi and Y.H. Kim and J.S. Lee and K.B. Lee and M.K. Lee and Y. Fukuda and Y. Itow and R. Kegasa and K. Kobayashi and K. Masuda and H. Takiya and H. Uchida and K. Nishijima and K. Fujii and I. Murayama and S. Nakamura}, | |
| Date-Added = {2016-10-05 08:39:26 +0000}, | |
| Date-Modified = {2016-10-05 08:39:26 +0000}, | |
| Doi = {http://dx.doi.org/10.1016/j.physletb.2016.05.039}, | |
| Issn = {0370-2693}, | |
| Journal = {Physics Letters B}, | |
| Keywords = {Liquid xenon}, | |
| Pages = {64 - 68}, | |
| Title = {Search for two-neutrino double electron capture on 124Xe with the XMASS-I detector}, | |
| Url = {http://www.sciencedirect.com/science/article/pii/S0370269316301861}, | |
| Volume = {759}, | |
| Year = {2016}, | |
| Bdsk-Url-1 = {http://www.sciencedirect.com/science/article/pii/S0370269316301861}, | |
| Bdsk-Url-2 = {http://dx.doi.org/10.1016/j.physletb.2016.05.039}} | |
| @article{Abe2009290, | |
| Abstract = {A high performance distillation system to remove krypton from xenon was constructed, and a purity level of Kr/Xe = ∼3 × 10−12 was achieved. This development is crucial in facilitating high-sensitivity low-background experiments such as the search for dark matter in the universe. }, | |
| Author = {K. Abe and J. Hosaka and T. Iida and M. Ikeda and K. Kobayashi and Y. Koshio and A. Minamino and M. Miura and S. Moriyama and M. Nakahata and Y. Nakajima and T. Namba and H. Ogawa and H. Sekiya and M. Shiozawa and Y. Suzuki and A. Takeda and Y. Takeuchi and K. Ueshima and M. Yamashita and K. Kaneyuki and Y. Ebizuka and J. Kikuchi and A. Ota and S. Suzuki and T. Takahashi and H. Hagiwara and T. Kamei and K. Miyamoto and T. Nagase and S. Nakamura and Y. Ozaki and T. Sato and Y. Fukuda and T. Sato and K. Nishijima and M. Sakurai and T. Maruyama and D. Motoki and Y. Itow and H. Ohsumi and S. Tasaka and S.B. Kim and Y.D. Kim and J.I. Lee and S.H. Moon and Y. Urakawa and M. Uchino and Y. Kamioka}, | |
| Date-Added = {2016-10-05 08:38:00 +0000}, | |
| Date-Modified = {2016-10-05 08:38:00 +0000}, | |
| Doi = {http://dx.doi.org/10.1016/j.astropartphys.2009.02.006}, | |
| Issn = {0927-6505}, | |
| Journal = {Astroparticle Physics}, | |
| Keywords = {Dark matter}, | |
| Number = {4}, | |
| Pages = {290 - 296}, | |
| Title = {Distillation of liquid xenon to remove krypton}, | |
| Url = {http://www.sciencedirect.com/science/article/pii/S092765050900036X}, | |
| Volume = {31}, | |
| Year = {2009}, | |
| Bdsk-Url-1 = {http://www.sciencedirect.com/science/article/pii/S092765050900036X}, | |
| Bdsk-Url-2 = {http://dx.doi.org/10.1016/j.astropartphys.2009.02.006}} | |
| @article{Abe201371978, | |
| Abstract = {A search for light dark matter using low-threshold data from the single phase liquid xenon scintillation detector XMASS, has been conducted. Using the entire 835 kg inner volume as target, the analysis threshold can be lowered to 0.3 keVee (electron-equivalent) to search for light dark matter. With low-threshold data corresponding to a 5591.4 kg day exposure of the detector and without discriminating between nuclear-recoil and electronic events, \{XMASS\} excludes part of the parameter space favored by other experiments. }, | |
| Author = {K. Abe and K. Hieda and K. Hiraide and S. Hirano and Y. Kishimoto and K. Kobayashi and S. Moriyama and K. Nakagawa and M. Nakahata and H. Ogawa and N. Oka and H. Sekiya and A. Shinozaki and Y. Suzuki and A. Takeda and O. Takachio and K. Ueshima and D. Umemoto and M. Yamashita and B.S. Yang and S. Tasaka and J. Liu and K. Martens and K. Hosokawa and K. Miuchi and A. Murata and Y. Onishi and Y. Otsuka and Y. Takeuchi and Y.H. Kim and K.B. Lee and M.K. Lee and J.S. Lee and Y. Fukuda and Y. Itow and K. Masuda and Y. Nishitani and H. Takiya and H. Uchida and N.Y. Kim and Y.D. Kim and F. Kusaba and D. Motoki and K. Nishijima and K. Fujii and I. Murayama and S. Nakamura}, | |
| Date-Added = {2016-10-05 08:36:36 +0000}, | |
| Date-Modified = {2016-10-05 08:38:38 +0000}, | |
| Doi = {http://dx.doi.org/10.1016/j.physletb.2013.01.001}, | |
| Issn = {0370-2693}, | |
| Journal = {Physics Letters B}, | |
| Keywords = {Xenon}, | |
| Number = {1--3}, | |
| Pages = {78 - 82}, | |
| Title = {Light \{WIMP\} search in \{XMASS\}}, | |
| Url = {http://www.sciencedirect.com/science/article/pii/S0370269313000117}, | |
| Volume = {719}, | |
| Year = {2013}, | |
| Bdsk-Url-1 = {http://www.sciencedirect.com/science/article/pii/S0370269313000117}, | |
| Bdsk-Url-2 = {http://dx.doi.org/10.1016/j.physletb.2013.01.001}} | |
| @article{Abe201371678, | |
| Abstract = {Abstract The \{XMASS\} project aims to detect dark matter, pp and 7Be solar neutrinos, and neutrinoless double beta decay using ultra pure liquid xenon. The first phase of the \{XMASS\} experiment searches for dark matter. In this paper, we describe the \{XMASS\} detector in detail, including its configuration, data acquisition equipment and calibration system. }, | |
| Author = {K. Abe and K. Hieda and K. Hiraide and S. Hirano and Y. Kishimoto and K. Kobayashi and S. Moriyama and K. Nakagawa and M. Nakahata and H. Nishiie and H. Ogawa and N. Oka and H. Sekiya and A. Shinozaki and Y. Suzuki and A. Takeda and O. Takachio and K. Ueshima and D. Umemoto and M. Yamashita and B.S. Yang and S. Tasaka and J. Liu and K. Martens and K. Hosokawa and K. Miuchi and A. Murata and Y. Onishi and Y. Otsuka and Y. Takeuchi and Y.H. Kim and K.B. Lee and M.K. Lee and J.S. Lee and Y. Fukuda and Y. Itow and Y. Nishitani and K. Masuda and H. Takiya and H. Uchida and N.Y. Kim and Y.D. Kim and F. Kusaba and D. Motoki and K. Nishijima and K. Fujii and I. Murayama and S. Nakamura}, | |
| Date-Added = {2016-10-05 08:35:46 +0000}, | |
| Date-Modified = {2016-10-05 08:47:48 +0000}, | |
| Doi = {http://dx.doi.org/10.1016/j.nima.2013.03.059}, | |
| Issn = {0168-9002}, | |
| Journal = {Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment}, | |
| Keywords = {Revision 5}, | |
| Pages = {78 - 85}, | |
| Title = {XMASS detector}, | |
| Url = {http://www.sciencedirect.com/science/article/pii/S0168900213003690}, | |
| Volume = {716}, | |
| Year = {2013}, | |
| Bdsk-Url-1 = {http://www.sciencedirect.com/science/article/pii/S0168900213003690}, | |
| Bdsk-Url-2 = {http://dx.doi.org/10.1016/j.nima.2013.03.059}} | |
| @article{Uchida:2014cnn, | |
| Archiveprefix = {arXiv}, | |
| Author = {Uchida, H. and others}, | |
| Collaboration = {XMASS-I}, | |
| Date-Added = {2016-10-05 08:35:16 +0000}, | |
| Date-Modified = {2016-10-05 08:35:16 +0000}, | |
| Doi = {10.1093/ptep/ptu064}, | |
| Eprint = {1401.4737}, | |
| Journal = {PTEP}, | |
| Number = {6}, | |
| Pages = {063C01}, | |
| Primaryclass = {astro-ph.CO}, | |
| Slaccitation = {%%CITATION = ARXIV:1401.4737;%%}, | |
| Title = {{Search for inelastic WIMP nucleus scattering on $^{129}Xe$ in data from the XMASS-I experiment}}, | |
| Volume = {2014}, | |
| Year = {2014}, | |
| Bdsk-Url-1 = {http://dx.doi.org/10.1093/ptep/ptu064}} | |
| @article{PhysRevLett.113.121301, | |
| Author = {Abe, K. and Hieda, K. and Hiraide, K. and Hirano, S. and Kishimoto, Y. and Ichimura, K. and Kobayashi, K. and Moriyama, S. and Nakagawa, K. and Nakahata, M. and Ogawa, H. and Oka, N. and Sekiya, H. and Shinozaki, A. and Suzuki, Y. and Takeda, A. and Takachio, O. and Umemoto, D. and Yamashita, M. and Yang, B. S. and Tasaka, S. and Liu, J. and Martens, K. and Hosokawa, K. and Miuchi, K. and Murata, A. and Onishi, Y. and Otsuka, Y. and Takeuchi, Y. and Kim, Y. H. and Lee, K. B. and Lee, M. K. and Lee, J. S. and Fukuda, Y. and Itow, Y. and Masuda, K. and Takiya, H. and Uchida, H. and Kim, N. Y. and Kim, Y. D. and Kusaba, F. and Nishijima, K. and Fujii, K. and Murayama, I. and Nakamura, S.}, | |
| Collaboration = {XMASS Collaboration}, | |
| Date-Added = {2016-10-05 08:34:21 +0000}, | |
| Date-Modified = {2016-10-05 08:34:21 +0000}, | |
| Doi = {10.1103/PhysRevLett.113.121301}, | |
| Issue = {12}, | |
| Journal = {Phys. Rev. Lett.}, | |
| Month = {Sep}, | |
| Numpages = {5}, | |
| Pages = {121301}, | |
| Publisher = {American Physical Society}, | |
| Title = {Search for Bosonic Superweakly Interacting Massive Dark Matter Particles with the XMASS-I Detector}, | |
| Url = {http://link.aps.org/doi/10.1103/PhysRevLett.113.121301}, | |
| Volume = {113}, | |
| Year = {2014}, | |
| Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevLett.113.121301}, | |
| Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevLett.113.121301}} | |
| @article{Hosokawa:2015qna, | |
| Author = {Hosokawa, K.}, | |
| Booktitle = {{Proceedings, 13th International Conference on Topics in Astroparticle and Underground Physics (TAUP 2013): Asilomar, California, September 8-13, 2013}}, | |
| Collaboration = {XMASS}, | |
| Date-Added = {2016-10-05 08:33:58 +0000}, | |
| Date-Modified = {2016-10-05 08:33:58 +0000}, | |
| Doi = {10.1016/j.phpro.2014.12.086}, | |
| Journal = {Phys. Procedia}, | |
| Pages = {714-718}, | |
| Slaccitation = {%%CITATION = INSPIRE-1357762;%%}, | |
| Title = {{Design of Low-energy Calibration Sources for Liquid Xenon Dark Matter Detectors}}, | |
| Volume = {61}, | |
| Year = {2015}, | |
| Bdsk-Url-1 = {http://dx.doi.org/10.1016/j.phpro.2014.12.086}} | |
| @article{1748-0221-11-02-C02053, | |
| Abstract = {XMASS is a single phase liquid xenon (LXe) detector, designed for a program of physics targets. As a first step in the program, the XMASS-I detector started operation with 832 kg of LXe in the sensitive volume from Sep. 2010. GEANT4 tools are used for the detector simulation to understand the detector response and background. In the simulation detailed structure and processes are required to reproduce background such as detector surface events and Cherenkov events. We present details of the geometry and processes used in the XMASS simulation in this paper.}, | |
| Author = {K. Abe}, | |
| Date-Added = {2016-10-05 08:33:29 +0000}, | |
| Date-Modified = {2016-10-05 08:33:29 +0000}, | |
| Journal = {Journal of Instrumentation}, | |
| Number = {02}, | |
| Pages = {C02053}, | |
| Title = {XMASS MC simulation}, | |
| Url = {http://stacks.iop.org/1748-0221/11/i=02/a=C02053}, | |
| Volume = {11}, | |
| Year = {2016}, | |
| Bdsk-Url-1 = {http://stacks.iop.org/1748-0221/11/i=02/a=C02053}} | |
| @article{Kim2015499, | |
| Abstract = {Abstract \{XMASS\} is a multipurpose liquid-xenon detector that currently aims to directly detect dark matter. In this paper, we describe the fabrication and characterization of reference sources used for the energy calibration and position reconstruction of the present \{XMASS\} detector. Several gamma-ray sources were produced in the form of a sealed needle-source. A thin-wall tube with a diameter of approximately 0.2 mm was sealed at both ends, with the 241Am or 57Co source material contained inside. The active region of the source was observed to be 1--2 mm long, close to the tip of the needle. These sources were tested in the \{XMASS\} detector, and the results were compared with Monte-Carlo simulations. }, | |
| Author = {N.Y. Kim and K. Abe and K. Hieda and K. Hiraide and S. Hirano and Y. Kishimoto and K. Kobayashi and S. Moriyama and K. Nakagawa and M. Nakahata and H. Nishiie and H. Ogawa and N. Oka and H. Sekiya and A. Shinozaki and Y. Suzuki and A. Takeda and O. Takachio and K. Ueshima and D. Umemoto and M. Yamashita and B.S. Yang and S. Tasaka and J. Liu and K. Martens and K. Hosokawa and K. Miuchi and A. Murata and Y. Onishi and Y. Otsuka and Y. Takeuchi and Y.H. Kim and K.B. Lee and M.K. Lee and J.S. Lee and Y. Fukuda and Y. Itow and Y. Nishitani and K. Masuda and H. Takiya and H. Uchida and Y.D. Kim and F. Kusaba and D. Motoki and K. Nishijima and K. Fujii and I. Murayama and S. Nakamura}, | |
| Date-Added = {2016-10-05 08:32:52 +0000}, | |
| Date-Modified = {2016-10-05 08:32:52 +0000}, | |
| Doi = {http://dx.doi.org/10.1016/j.nima.2014.11.012}, | |
| Issn = {0168-9002}, | |
| Journal = {Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment}, | |
| Keywords = {Micro-size radioactive source}, | |
| Note = {Symposium on Radiation Measurements and Applications 2014 (SORMA XV)}, | |
| Pages = {499 - 503}, | |
| Title = {Micro-source development for \{XMASS\} experiment}, | |
| Url = {http://www.sciencedirect.com/science/article/pii/S0168900214012765}, | |
| Volume = {784}, | |
| Year = {2015}, | |
| Bdsk-Url-1 = {http://www.sciencedirect.com/science/article/pii/S0168900214012765}, | |
| Bdsk-Url-2 = {http://dx.doi.org/10.1016/j.nima.2014.11.012}} | |
| @article{XMASS:2016cmy, | |
| Archiveprefix = {arXiv}, | |
| Author = {Abe, K. and others}, | |
| Collaboration = {XMASS}, | |
| Date-Added = {2016-10-05 08:30:15 +0000}, | |
| Date-Modified = {2016-10-05 08:30:15 +0000}, | |
| Eprint = {1604.01218}, | |
| Primaryclass = {physics.ins-det}, | |
| Slaccitation = {%%CITATION = ARXIV:1604.01218;%%}, | |
| Title = {{Detectability of galactic supernova neutrinos coherently scattered on xenon nuclei in XMASS}}, | |
| Year = {2016}} | |
| @article{DiLella2003145, | |
| Abstract = {Several unexpected astrophysical observations can be explained by gravitationally captured massive axions or axion-like particles, which are produced inside the Sun or other stars and are accumulated over cosmic times. Their radiative decay in solar outer space would give rise to a `self-irradiation' of the whole star, providing the time-independent component of the corona heating source (we do not address here the flaring Sun). In analogy with the Sun-irradiated Earth atmosphere, the temperature and density gradient in the corona--chromosphere transition region is suggestive for an omnipresent irradiation of the Sun, which is the strongest evidence for the generic axion-like scenario. The same mechanism is compatible with phenomena like the solar wind, the X-rays from the dark-side of the Moon, the X-ray background radiation, the diffuse X-ray excesses (below ∼1 keV), the non-cooling of oldest stars, etc. A temperature of ∼106 K is observed in various places, while the radiative decay of a population of such elusive particles mimics a hot gas, which fits unexpected astrophysical X-ray observations. Furthermore, the recently reconstructed quiet solar X-ray spectrum during solar minimum supports this work, since it covers the expected energy range, and it is consistent with the result of a simulation based on Kaluza--Klein axions above ∼1 keV. The derived axion luminosity (La≈0.16L⊙) fits the cosmic energy density spectrum and is compatible within 2σ with the recent \{SNO\} result, showing the important interplay between any exotic energy loss mechanism and neutrino production. At lower energies, using also a \{ROSAT\} observation, only ∼3% of the X-ray intensity is explained. Data from orbiting X-ray telescopes provide upper limits for particle decay rates 1 a.u. from the Sun, and suggest new types of searches on Earth or in space. In particular, X-ray observatories, with an unrivalled equivalent fiducial volume of ∼103 m3 for the 0.1--10 keV range, can search for the radiative decay of new particles even from existing data. This work introduces the elongation angle of the X-ray telescope relative to the Sun as a relevant new parameter. }, | |
| Author = {L DiLella and K Zioutas}, | |
| Date-Added = {2016-10-05 08:20:39 +0000}, | |
| Date-Modified = {2016-10-05 08:20:39 +0000}, | |
| Doi = {http://dx.doi.org/10.1016/S0927-6505(02)00186-X}, | |
| Issn = {0927-6505}, | |
| Journal = {Astroparticle Physics}, | |
| Number = {1}, | |
| Pages = {145 - 170}, | |
| Title = {Observational evidence for gravitationally trapped massive axion(-like) particles}, | |
| Url = {http://www.sciencedirect.com/science/article/pii/S092765050200186X}, | |
| Volume = {19}, | |
| Year = {2003}, | |
| Bdsk-Url-1 = {http://www.sciencedirect.com/science/article/pii/S092765050200186X}, | |
| Bdsk-Url-2 = {http://dx.doi.org/10.1016/S0927-6505(02)00186-X}} | |
| @article{0004-637X-607-1-575, | |
| Abstract = {We have studied published data from the Yohkoh solar X-ray mission with the purpose of searching for signals from radiative decays of new, as yet undiscovered massive neutral particles. This search is based on the prediction that solar axions of the Kaluza-Klein type should result in the emission of X-rays from the Sun direction beyond the limb with a characteristic radial distribution. These X-rays should be observed more easily during periods of quiet Sun. An additional signature is the observed emission of hard X-rays by the Solar Maximum Mission ( SMM ), the Near Earth Asteroid Rendezvous ( NEAR ), and RHESSI . The recent observation made by RHESSI of a continuous emission from the nonflaring Sun of X-rays in the 3 to ~15 keV range fits the generic axion scenario. This work also suggests new analyses of existing data in order to exclude instrumental effects; it provides the rationale for targeted observations with present and upcoming (solar) X-ray telescopes, which can provide the final answer to the nature of the signals considered here. Such measurements become more promising during the forthcoming solar cycle minimum with an increased number of quiet-Sun periods.}, | |
| Author = {K. Zioutas and K. Dennerl and L. DiLella and D. H. H. Hoffmann and J. Jacoby and Th. Papaevangelou}, | |
| Date-Added = {2016-10-05 08:19:59 +0000}, | |
| Date-Modified = {2016-10-05 08:19:59 +0000}, | |
| Journal = {The Astrophysical Journal}, | |
| Number = {1}, | |
| Pages = {575}, | |
| Title = {Quiet-Sun X-Rays as Signature for New Particles}, | |
| Url = {http://stacks.iop.org/0004-637X/607/i=1/a=575}, | |
| Volume = {607}, | |
| Year = {2004}, | |
| Bdsk-Url-1 = {http://stacks.iop.org/0004-637X/607/i=1/a=575}} | |
| @phdthesis{500000130987, | |
| Author = {小川, 泉}, | |
| Date-Added = {2016-10-03 09:31:43 +0000}, | |
| Date-Modified = {2016-10-03 09:31:43 +0000}, | |
| School = {京都大学}, | |
| Title = {Development of an experimental system for dark matter axion search with Rydberg atoms}, | |
| Url = {http://ci.nii.ac.jp/naid/500000130987}, | |
| Year = {1996}, | |
| Bdsk-Url-1 = {http://ci.nii.ac.jp/naid/500000130987}} | |
| @article{Inada:2016jzh, | |
| Archiveprefix = {arXiv}, | |
| Author = {Inada, T. and others}, | |
| Date-Added = {2016-10-02 02:31:22 +0000}, | |
| Date-Modified = {2016-10-02 02:31:22 +0000}, | |
| Eprint = {1609.05425}, | |
| Primaryclass = {hep-ex}, | |
| Slaccitation = {%%CITATION = ARXIV:1609.05425;%%}, | |
| Title = {{Search for Two-Photon Interaction with Axionlike Particles Using High-Repetition Pulsed Magnets and Synchrotron X Rays}}, | |
| Year = {2016}} | |
| @article{110007504107, | |
| Author = {Akimoto, Yuki and Minowa, Makoto}, | |
| Date-Added = {2016-10-01 01:20:17 +0000}, | |
| Date-Modified = {2016-10-01 01:20:17 +0000}, | |
| Issn = {00290181}, | |
| Journal = {Butsuri}, | |
| Month = {jan}, | |
| Number = {1}, | |
| Pages = {25-29}, | |
| Publisher = {The Physical Society of Japan (JPS)}, | |
| Title = {Search for Solar Axions(Current Topics)}, | |
| Url = {http://ci.nii.ac.jp/naid/110007504107/en/}, | |
| Volume = {65}, | |
| Year = {2010}, | |
| Bdsk-Url-1 = {http://ci.nii.ac.jp/naid/110007504107/en/}} | |
| @article{Inoue200893, | |
| Abstract = {A search for solar axions has been performed using an axion helioscope which is equipped with a 2.3-m long 4 T superconducting magnet, a gas container to hold dispersion-matching gas, PIN-photodiode X-ray detectors, and a telescope mount mechanism to track the sun. A mass region around m a = 1 eV was newly explored. From the absence of any evidence, analysis sets a limit on axion--photon coupling constant to be g a γ γ < 5.6 -- 13.4 × 10 −10 GeV −1 for the axion mass of 0.84 < m a < 1.00 eV at 95% confidence level. It is the first result to search for the axion in the g a γ γ -- m a parameter region of the preferred axion models with a magnetic helioscope. }, | |
| Author = {Y. Inoue and Y. Akimoto and R. Ohta and T. Mizumoto and A. Yamamoto and M. Minowa}, | |
| Date-Added = {2016-10-01 01:19:31 +0000}, | |
| Date-Modified = {2016-10-01 01:19:31 +0000}, | |
| Doi = {http://dx.doi.org/10.1016/j.physletb.2008.08.020}, | |
| Issn = {0370-2693}, | |
| Journal = {Physics Letters B}, | |
| Keywords = {Superconducting magnet}, | |
| Number = {2}, | |
| Pages = {93 - 97}, | |
| Title = {Search for solar axions with mass around 1 eV using coherent conversion of axions into photons}, | |
| Url = {http://www.sciencedirect.com/science/article/pii/S0370269308010137}, | |
| Volume = {668}, | |
| Year = {2008}, | |
| Bdsk-Url-1 = {http://www.sciencedirect.com/science/article/pii/S0370269308010137}, | |
| Bdsk-Url-2 = {http://dx.doi.org/10.1016/j.physletb.2008.08.020}} | |
| @phdthesis{500000210402, | |
| Author = {田澤, 志郎}, | |
| Date-Added = {2016-10-01 01:18:55 +0000}, | |
| Date-Modified = {2016-10-01 01:18:55 +0000}, | |
| School = {東北大学}, | |
| Title = {大きな余剰次元理論におけるアクシオンへの宇宙論的制限}, | |
| Url = {http://ci.nii.ac.jp/naid/500000210402}, | |
| Year = {2001}, | |
| Bdsk-Url-1 = {http://ci.nii.ac.jp/naid/500000210402}} | |
| @article{PhysRevLett.38.1440, | |
| Author = {Peccei, R. D. and Quinn, Helen R.}, | |
| Date-Added = {2016-09-30 04:14:58 +0000}, | |
| Date-Modified = {2016-09-30 04:14:58 +0000}, | |
| Doi = {10.1103/PhysRevLett.38.1440}, | |
| Issue = {25}, | |
| Journal = {Phys. Rev. Lett.}, | |
| Month = {Jun}, | |
| Numpages = {0}, | |
| Pages = {1440--1443}, | |
| Publisher = {American Physical Society}, | |
| Title = {$\mathrm{CP}$ Conservation in the Presence of Pseudoparticles}, | |
| Url = {http://link.aps.org/doi/10.1103/PhysRevLett.38.1440}, | |
| Volume = {38}, | |
| Year = {1977}, | |
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| Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevLett.38.1440}, | |
| Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevLett.38.1440}} | |
| @article{PhysRevD.59.086004, | |
| Author = {Arkani-Hamed, Nima and Dimopoulos, Savas and Dvali, Gia}, | |
| Date-Added = {2016-09-13 10:47:54 +0000}, | |
| Date-Modified = {2016-09-13 11:00:32 +0000}, | |
| Doi = {10.1103/PhysRevD.59.086004}, | |
| Issue = {8}, | |
| Journal = {Phys. Rev. D}, | |
| Keywords = {Extra Dimensions, KK axion}, | |
| Month = {Mar}, | |
| Numpages = {21}, | |
| Pages = {086004}, | |
| Project = {Doctor Thesis}, | |
| Publisher = {American Physical Society}, | |
| Title = {Phenomenology, astrophysics, and cosmology of theories with submillimeter dimensions and TeV scale quantum gravity}, | |
| Url = {http://link.aps.org/doi/10.1103/PhysRevD.59.086004}, | |
| Volume = {59}, | |
| Year = {1999}, | |
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| Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.59.086004}, | |
| Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.59.086004}} | |
| @article{Antoniadis1998257, | |
| Abstract = {Recently, a new framework for solving the hierarchy problem has been proposed which does not rely on low energy supersymmetry or technicolor. The gravitational and gauge interactions unite at the electroweak scale, and the observed weakness of gravity at long distances is due the existence of large new spatial dimensions. In this letter, we show that this framework can be embedded in string theory. These models have a perturbative description in the context of type I string theory. The gravitational sector consists of closed strings propagating in the higher-dimensional bulk, while ordinary matter consists of open strings living on D3-branes. This scenario raises the exciting possibility that the \{LHC\} and \{NLC\} will experimentally study ordinary aspects of string physics such as the production of narrow Regge-excitations of all standard model particles, as well more exotic phenomena involving strong gravity such as the production of black holes. The new dimensions can be probed by events with large missing energy carried off by gravitons escaping into the bulk. We finally discuss some important issues of model building, such as proton stability, gauge coupling unification and supersymmetry breaking. }, | |
| Author = {Ignatios Antoniadis and Nima Arkani-Hamed and Savas Dimopoulos and Gia Dvali}, | |
| Date-Added = {2016-09-13 10:44:53 +0000}, | |
| Date-Modified = {2016-09-13 11:00:15 +0000}, | |
| Journal = {Physics Letters B}, | |
| Keywords = {Extra Dimensions}, | |
| Number = {3--4}, | |
| Pages = {257 - 263}, | |
| Project = {Doctor Thesis}, | |
| Title = {New dimensions at a millimeter to a fermi and superstrings at a TeV}, | |
| Url = {http://www.sciencedirect.com/science/article/pii/S0370269398008600}, | |
| Volume = {436}, | |
| Year = {1998}, | |
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| Bdsk-Url-1 = {http://www.sciencedirect.com/science/article/pii/S0370269398008600}} | |
| @article{ArkaniHamed1998263, | |
| Abstract = {We propose a new framework for solving the hierarchy problem which does not rely on either supersymmetry or technicolor. In this framework, the gravitational and gauge interactions become united at the weak scale, which we take as the only fundamental short distance scale in nature. The observed weakness of gravity on distances ≳ 1 mm is due to the existence of n≥2 new compact spatial dimensions large compared to the weak scale. The Planck scale MPl∼GN−1/2 is not a fundamental scale; its enormity is simply a consequence of the large size of the new dimensions. While gravitons can freely propagate in the new dimensions, at sub-weak energies the Standard Model (SM) fields must be localized to a 4-dimensional manifold of weak scale ``thickness'' in the extra dimensions. This picture leads to a number of striking signals for accelerator and laboratory experiments. For the case of n=2 new dimensions, planned sub-millimeter measurements of gravity may observe the transition from 1/r2→1/r4 Newtonian gravitation. For any number of new dimensions, the \{LHC\} and \{NLC\} could observe strong quantum gravitational interactions. Furthermore, \{SM\} particles can be kicked off our 4 dimensional manifold into the new dimensions, carrying away energy, and leading to an abrupt decrease in events with high transverse momentum pT≳ TeV. For certain compact manifolds, such particles will keep circling in the extra dimensions, periodically returning, colliding with and depositing energy to our four dimensional vacuum with frequencies of ∼1012 Hz or larger. As a concrete illustration, we construct a model with \{SM\} fields localized on the 4-dimensional throat of a vortex in 6 dimensions, with a Pati-Salam gauge symmetry SU(4)×SU(2)×SU(2) in the bulk. | |
| }, | |
| Author = {Antoniadis, Ignatios and Arkani-Hamed, Nima and Dimopoulos, Savas and Dvali, Gia}, | |
| Date-Added = {2016-09-13 10:41:16 +0000}, | |
| Date-Modified = {2016-09-13 11:00:02 +0000}, | |
| Doi = {http://dx.doi.org/10.1016/S0370-2693(98)00466-3}, | |
| Issn = {0370-2693}, | |
| Journal = {Physics Letters B}, | |
| Keywords = {Extra Dimensions}, | |
| Number = {3--4}, | |
| Pages = {263 - 272}, | |
| Project = {Doctor Thesis}, | |
| Title = {The hierarchy problem and new dimensions at a millimeter}, | |
| Url = {http://www.sciencedirect.com/science/article/pii/S0370269398004663}, | |
| Volume = {429}, | |
| Year = {1998}, | |
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| @incollection{Bando2001, | |
| Author = {坂東, 昌子 and 中野, 博章}, | |
| Booktitle = {現代物理最前線}, | |
| Date-Added = {2016-09-13 08:53:11 +0000}, | |
| Date-Modified = {2016-09-13 10:58:52 +0000}, | |
| Editor = {大槻義彦}, | |
| Keywords = {Extra Dimensions}, | |
| Month = {10}, | |
| Pages = {3-72}, | |
| Project = {Doctor Thesis}, | |
| Publisher = {共立出版株式会社}, | |
| Series = {現代物理最前線}, | |
| Title = {四次元を超える時空と素粒子―隠された次元}, | |
| Url = {http://www.kyoritsu-pub.co.jp/bookdetail/9784320033900}, | |
| Volume = {5}, | |
| Year = {2001}, | |
| Bdsk-Url-1 = {http://www.kyoritsu-pub.co.jp/bookdetail/9784320033900}} | |
| @article{PhysRevD.62.105023, | |
| Author = {Dienes, Keith R. and Dudas, Emilian and Gherghetta, Tony}, | |
| Date-Added = {2016-09-13 06:39:07 +0000}, | |
| Date-Modified = {2016-09-13 06:39:31 +0000}, | |
| Doi = {10.1103/PhysRevD.62.105023}, | |
| Issue = {10}, | |
| Journal = {Phys. Rev. D}, | |
| Month = {Oct}, | |
| Numpages = {22}, | |
| Pages = {105023}, | |
| Project = {Doctor Thesis}, | |
| Publisher = {American Physical Society}, | |
| Title = {Invisible axions and large-radius compactifications}, | |
| Url = {http://link.aps.org/doi/10.1103/PhysRevD.62.105023}, | |
| Volume = {62}, | |
| Year = {2000}, | |
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| Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.62.105023}, | |
| Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.62.105023}} | |
| @article{PhysRevD.62.125011, | |
| Author = {Di Lella, L. and Pilaftsis, A. and Raffelt, G. and Zioutas, K.}, | |
| Date-Added = {2016-09-13 06:35:07 +0000}, | |
| Date-Modified = {2016-09-13 06:36:09 +0000}, | |
| Doi = {10.1103/PhysRevD.62.125011}, | |
| Issue = {12}, | |
| Journal = {Phys. Rev. D}, | |
| Keywords = {KK axion, Extra Dimensions}, | |
| Month = {Nov}, | |
| Numpages = {8}, | |
| Pages = {125011}, | |
| Project = {Doctor Thesis}, | |
| Publisher = {American Physical Society}, | |
| Title = {Search for solar Kaluza-Klein axions in theories of low-scale quantum gravity}, | |
| Url = {http://link.aps.org/doi/10.1103/PhysRevD.62.125011}, | |
| Volume = {62}, | |
| Year = {2000}, | |
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| Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.62.125011}, | |
| Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.62.125011}} | |
| @article{PhysRevD.61.084005, | |
| Annote = {2016/09/13 追加。 | |
| }, | |
| Author = {Chang, Sanghyeon and Tazawa, Shiro and Yamaguchi, Masahiro}, | |
| Date-Added = {2016-09-13 04:36:53 +0000}, | |
| Date-Modified = {2016-09-13 04:53:42 +0000}, | |
| Doi = {10.1103/PhysRevD.61.084005}, | |
| Issue = {8}, | |
| Journal = {Phys. Rev. D}, | |
| Keywords = {KK axion, Extra Dimensions}, | |
| Month = {Mar}, | |
| Numpages = {11}, | |
| Pages = {084005}, | |
| Project = {Doctor Thesis}, | |
| Publisher = {American Physical Society}, | |
| Title = {Axion model in extra dimensions with TeV scale gravity}, | |
| Url = {http://link.aps.org/doi/10.1103/PhysRevD.61.084005}, | |
| Volume = {61}, | |
| Year = {2000}, | |
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| Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.61.084005}, | |
| Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.61.084005}} | |
| @mastersthesis{Oka-Master, | |
| Abstract = {My master thesis.}, | |
| Author = {岡直哉}, | |
| Date-Added = {2014-12-14 01:19:26 +0000}, | |
| Date-Modified = {2016-09-13 10:51:33 +0000}, | |
| Keywords = {XMASS}, | |
| Note = {\texttt{\href{http://www-sk.icrr.u-tokyo.ac.jp/xmass/publist/master-oka.pdf}{http://www-sk.icrr.u-tokyo.ac.jp/xmass/publist/master-oka.pdf}}}, | |
| Project = {Master Thesis, My Work}, | |
| Read = {1}, | |
| School = {東京大学大学院理学系研究科物理学専攻}, | |
| Title = {{XMASS}実験における検出器材料由来バックグラウンドの研究}, | |
| Url = {http://www-sk.icrr.u-tokyo.ac.jp/xmass/publist/master-oka.pdf}, | |
| Year = {2014}, | |
| Bdsk-Url-1 = {http://www-sk.icrr.u-tokyo.ac.jp/xmass/publist/master-oka.pdf}} | |
| @misc{Oka-Master-teuchi, | |
| Note = {岡直哉, 東京大学大学院理学系研究科修士論文(2014).\\ \texttt{\href{http://www-sk.icrr.u-tokyo.ac.jp/xmass/publist/master-oka.pdf}{http://www-sk.icrr.u-tokyo.ac.jp/xmass/publist/master-oka.pdf}}}} | |
| @misc{CRESST2012, | |
| Abstract = {730 kg day のexposureで67 event残り、BGで説明できなかった。(4-sigama) "these backgrounds are not sufficient to explain all the observed events."}, | |
| Keywords = {CRESST}, | |
| Note = {Angloher, G. \textit{et al}., Results from 730 kg days of the CRESST-II Dark Matter search. \textit{Eur. Phys. J.} C \textbf{72} (2012) 1971.\\ \texttt{\href{http://dx.doi.org/10.1140/epjc/s10052-012-1971-8}{DOI:10.1140/epjc/s10052-012-1971-8}}}} | |
| @misc{CoGeNT2013, | |
| Abstract = {これより前に報告された低エネルギーのevent excessと、annual modulationの、BGを検証したけど説明できなかった。surface event contaminationも評価した。"showed a 2:8 significance modulation of the monthly event rate in the low-energy region that is compatible with the dark matter signature described in [6]."}, | |
| Keywords = {CoGeNT}, | |
| Note = {Aalseth, C. E. \textit{et al}. (CoGeNT Collaboration), CoGeNT: A search for low-mass dark matter using p-type point contact germanium detectors. \textit{Phys. Rev.} D \textbf{88} (2013) 012002.\\ \texttt{\href{http://dx.doi.org/10.1103/PhysRevD.88.012002}{DOI:10.1103/PhysRevD.88.012002}}}} | |
| @misc{YKishimoto2014, | |
| Keywords = {XMASS}, | |
| Note = {岸本康宏, 大型実験装置による暗黒物質直接探索, 新学術「地下素核研究」第一回研究会(2014) \texttt{\href{http://www.lowbg.org/ugnd/WS/index.html}{http://www.lowbg.org/ugnd/WS/index.html}}.\\ \texttt{\href{http://www.lowbg.org/ugnd/WS/Data/Prog/31_Kishimoto_XMASS.pdf}{http://www.lowbg.org/ugnd/WS/Data/Prog/31\_Kishimoto\_XMASS.pdf}}}} | |
| @misc{SuperCDMS2014, | |
| Abstract = {Super CDMSの最初の結果。2013年のCDMS II Siの領域を棄却している。}, | |
| Keywords = {CDMS}, | |
| Note = {Agnese, R. \textit{et al}. (CDMS Collaboration), Search for Low-Mass WIMPs with SuperCDMS, \textit{arXiv:}1402.7137 [hep-ex].// \texttt{\href{http://arxiv.org/abs/1402.7137}{arXiv:1402.7137}}}} | |
| @misc{CDMS-Si2013, | |
| Abstract = {3 event残り、BGで説明できなかった。}, | |
| Keywords = {CDMS}, | |
| Note = {Agnese, R. \textit{et al}. (CDMS Collaboration), Silicon Detector Dark Matter Results from the Final Exposure of CDMS II, \textit{arXiv:}1304.4279 [hep-ex] .\\ \texttt{\href{http://arxiv.org/abs/1304.4279}{arXiv:1304.4279}}}} | |
| @misc{LUX2014, | |
| Abstract = {First result from LUX and world best limit.}, | |
| Keywords = {LUX}, | |
| Note = {Akerib, D.S. \textit{et al}. (LUX Collaboration), First Results from the LUX Dark Matter Experiment at the Sanford Underground Research Facility. \textit{Phys. Rev. Lett.} \textbf{112} (2014) 091303.\\ \texttt{\href{http://dx.doi.org/10.1103/PhysRevLett.112.091303}{DOI:10.1103/PhysRevLett.112.091303}}}} | |
| @misc{DAMIC2012, | |
| Abstract = {First result from DAMIC 0.5g}, | |
| Keywords = {DAMIC}, | |
| Note = {Barreto, J. \textit{et al}., Direct search for low mass dark matter particles with CCDs. \textit{Phys. Lett. B} \textbf{711} (2012) 264-269.\\ \texttt{\href{http://dx.doi.org/10.1016/j.physletb.2012.04.006}{DOI:10.1016/j.physletb.2012.04.006}}}} | |
| @misc{DAMIC2014, | |
| Abstract = {Explanation of Detector of DAMIC in SNOLAB}, | |
| Keywords = {DAMIC}, | |
| Note = {Chavarria, A. E. \textit{et al}., DAMIC at SNOLAB. \textit{arXiv:}1407.0347 [physics.ins-det].\\ \texttt{\href{http://arxiv.org/abs/1407.0347}{arXiv:1407.0347}}}} | |
| @misc{CDMSlite2014, | |
| Abstract = {arXiv上ではCDMSliteとなっている。DAMIC3 GeV以上ではDAMICよりもかなりいいlimit.}, | |
| Keywords = {CDMS}, | |
| Note = {Agnese, R. \textit{et al}. (SuperCDMS collaboration), Search for Low-Mass Weakly Interacting Massive Particles Using Voltage-Assisted Calorimetric Ionization Detection in the SuperCDMS Experiment. \textit{Phys. Rev. Lett.} \textbf{112} (2014) 041302.\\ \texttt{\href{http://dx.doi.org/10.1103/PhysRevLett.112.041302}{DOI:10.1103/PhysRevLett.112.041302}}}} | |
| @misc{Magnusson1957, | |
| Abstract = {Np XrayとAm gamma rayの強度の研究。古いのでもっと新しいのがあれば知りたい。あった-> http://dx.doi.org/10.1016/j.apradiso.2009.11.032}, | |
| Date-Modified = {2016-09-13 10:53:11 +0000}, | |
| Keywords = {Radioactivity}, | |
| Note = {Magnusson, L. B. , Intensities of X-Rays and $\gamma$ Rays in Am$^{241}$ Alpha Decay. \textit{Phys. Rev.} \textbf{107} (1957) 161.\\ \texttt{\href{http://dx.doi.org/10.1103/PhysRev.107.161}{DOI:10.1103/PhysRev.107.161}}}, | |
| Project = {SOI-DM}} | |
| @misc{Yang&Hamilton, | |
| Abstract = {X線の勉強に読んだ。}, | |
| Date-Modified = {2016-09-13 10:52:55 +0000}, | |
| Keywords = {Xray}, | |
| Note = {Yang, F. and Hamilton, J. H., Modern Atomic and Nuclear Physics. (Revised Edition) \textit{World Scientific} (2010).\\ \texttt{\href{http://dx.doi.org/10.1142/7099}{DOI:10.1142/7099}}}, | |
| Project = {SOI-DM}} | |
| @misc{XRPIX-NIMA, | |
| Abstract = {XRPIXのNIM A}, | |
| Date-Modified = {2016-09-13 10:52:43 +0000}, | |
| Keywords = {Xray, SOI}, | |
| Note = {Matsumura, H, et al., Investigation of charge-collection efficiency of Kyoto׳s X-ray astronomical SOI pixel sensors, XRPIX. \textit{Nucl. Inst. and Meth. A} \textbf{765} (2014) 183-186.\\ \texttt{\href{http://dx.doi.org/10.1016/j.nima.2014.05.025}{DOI:10.1016/j.nima.2014.05.025}}}, | |
| Project = {SOI-DM}} | |
| @article{PhysRevLett.112.041302, | |
| Author = {Agnese, R. and Anderson, A. J. and Asai, M. and Balakishiyeva, D. and Basu Thakur, R. and Bauer, D. A. and Billard, J. and Borgland, A. and Bowles, M. A. and Brandt, D. and Brink, P. L. and Bunker, R. and Cabrera, B. and Caldwell, D. O. and Cerdeno, D. G. and Chagani, H. and Cooley, J. and Cornell, B. and Crewdson, C. H. and Cushman, P. and Daal, M. and Di Stefano, P. C. F. and Doughty, T. and Esteban, L. and Fallows, S. and Figueroa-Feliciano, E. and Godfrey, G. L. and Golwala, S. R. and Hall, J. and Harris, H. R. and Hertel, S. A. and Hofer, T. and Holmgren, D. and Hsu, L. and Huber, M. E. and Jastram, A. and Kamaev, O. and Kara, B. and Kelsey, M. H. and Kennedy, A. and Kiveni, M. and Koch, K. and Loer, B. and Lopez Asamar, E. and Mahapatra, R. and Mandic, V. and Martinez, C. and McCarthy, K. A. and Mirabolfathi, N. and Moffatt, R. A. and Moore, D. C. and Nadeau, P. and Nelson, R. H. and Page, K. and Partridge, R. and Pepin, M. and Phipps, A. and Prasad, K. and Pyle, M. and Qiu, H. and Rau, W. and Redl, P. and Reisetter, A. and Ricci, Y. and Saab, T. and Sadoulet, B. and Sander, J. and Schneck, K. and Schnee, R. W. and Scorza, S. and Serfass, B. and Shank, B. and Speller, D. and Villano, A. N. and Welliver, B. and Wright, D. H. and Yellin, S. and Yen, J. J. and Young, B. A. and Zhang, J.}, | |
| Collaboration = {(SuperCDMS collaboration)}, | |
| Date-Modified = {2016-09-13 04:57:38 +0000}, | |
| Doi = {10.1103/PhysRevLett.112.041302}, | |
| Issue = {4}, | |
| Journal = {Phys. Rev. Lett.}, | |
| Keywords = {CDMS, Light WIMPs}, | |
| Month = {Jan}, | |
| Numpages = {6}, | |
| Pages = {041302}, | |
| Publisher = {American Physical Society}, | |
| Title = {Search for Low-Mass Weakly Interacting Massive Particles Using Voltage-Assisted Calorimetric Ionization Detection in the SuperCDMS Experiment}, | |
| Url = {http://link.aps.org/doi/10.1103/PhysRevLett.112.041302}, | |
| Volume = {112}, | |
| Year = {2014}, | |
| Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevLett.112.041302}, | |
| Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevLett.112.041302}} |