费米LAT对30至200 GeV光子线的搜索及其暗物质意义
高能天体物理现象
2012-05-15 v1 宇宙学与河外天体物理
高能物理 - 实验
高能物理 - 唯象学
摘要
暗物质粒子湮灭或衰变可以产生单色γ射线，易于与天体物理源区分。本文利用费米大面积望远镜11个月的数据（20-300 GeV），基于γ射线线分析的要求进行选择，并积分了大部分天区，给出了30 GeV至200 GeV的γ射线线极限。我们获得了0.6-4.5×10^{-9} cm^{-2} s^{-1}范围内的γ射线线通量上限，并给出了相应的暗物质湮灭截面和衰变寿命极限。简要讨论了理论意义。
引用
@article{arxiv.1001.4836,
title = {Fermi LAT Search for Photon Lines from 30 to 200 GeV and Dark Matter Implications},
author = {The Fermi LAT Collaboration and A. A. Abdo and M. Ackermann and M. Ajello and W. B. Atwood and L. Baldini and J. Ballet and G. Barbiellini and D. Bastieri and K. Bechtol and R. Bellazzini and B. Berenji and E. D. Bloom and E. Bonamente and A. W. Borgland and A. Bouvier and J. Bregeon and A. Brez and M. Brigida and P. Bruel and T. H. Burnett and S. Buson and G. A. Caliandro and R. A. Cameron and P. A. Caraveo and S. Carrigan and J. M. Casandjian and C. Cecchi and O. C. Elik and A. Chekhtman and J. Chiang and S. Ciprini and R. Claus and J. Cohen-Tanugi and J. Conrad and C. D. Dermer and A. de Angelis and F. de Palma and S. W. Digel and E. do Couto e Silva and P. S. Drell and A. Drlica-Wagner and R. Dubois and D. Dumora and Y. Edmonds and R. Essig and C. Farnier and C. Favuzzi and S. J. Fegan and W. B. Focke and P. Fortin and M. Frailis and Y. Fukazawa and S. Funk and P. Fusco and F. Gargano and D. Gasparrini and N. Gehrels and S. Germani and N. Giglietto and F. Giordano and T. Glanzman and G. Godfrey and I. A. Grenier and J. E. Grove and L. Guillemot and S. Guiriec and M. Gustafsson and D. Hadasch and A. K. Harding and D. Horan and R. E. Hughes and M. S. Jackson and G. J . ohannesson and A. S. Johnson and R. P. Johnson and W. N. Johnson and T. Kamae and H. Katagiri and J. Kataoka and N. Kawai and M. Kerr and J. Kno . dlseder and M. Kuss and J. Lande and L. Latronico and M. Llena Garde and F. Longo and F. Loparco and B. Lott and M. N. Lovellette and P. Lubrano and A. Makeev and M. N. Mazziotta and J. E. McEnery and C. Meurer and P. F. Michelson and W. Mitthumsiri and T. Mizuno and A. A. Moiseev and C. Monte and M. E. Monzani and A. Morselli and I. V. Moskalenko and S. Murgia and P. L. Nolan and J. P. Norris and E. Nuss and T. Ohsugi and N. Omodei and E. Orlando and J. F. Ormes and M. Ozaki and D. Paneque and J. H. Panetta and D. Parent and V. Pelassa and M. Pepe and M. Pesce-Rollins and F. Piron and S. Rainó and R. Rando and M. Razzano and A. Reimer and O. Reimer and T. Reposeur and J. Ripken and S. Ritz and A. Y. Rodriguez and M. Roth and H. F. -W. Sadrozinski and A. Sander and P. M. Saz Parkinson and J. D. Scargle and T. L. Schalk and A. Sellerholm and C. Sgró and E. J. Siskind and D. A. Smith and P. D. Smith and G. Spandre and P. Spinelli and J. -L. Starck and M. S. Strickman and D. J. Suson and H. Tajima and H. Takahashi and T. Tanaka and J. B. Thayer and J. G. Thayer and L. Tibaldo and D. F. Torres and Y. Uchiyama and T. L. Usher and V. Vasileiou and N. Vilchez and V. Vitale and A. P. Waite and P. Wang and B. L. Winer and K. S. Wood and T. Ylinen and M. Ziegler},
journal= {arXiv preprint arXiv:1001.4836},
year = {2012}
}
备注
6 pages, 1 figure. Accepted for publication by The Physical Review Letters