Limits on sub-GeV dark matter from the PROSPECT reactor antineutrino experiment
Limits on sub-GeV dark matter from the PROSPECT reactor antineutrino experiment
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PROSPECT 反应堆反中微子实验对亚 GeV 暗物质的限制
DOI：
10.1103/physrevd.104.012009
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发表时间：
2021
影响因子：
5
通讯作者：
Deichert, G.
中科院分区：
文献类型：
--
作者：
Andriamirado, M.;Balantekin, A. B.;Band, H. R.;Bass, C. D.;Bergeron, D. E.;Bowden, N. S.;Bryan, C. D.;Classen, T.;Conant, A. J.;Deichert, G.
如果暗物质的质量低于1GeV左右，它将不会提供足够的能量来在许多直接探测实验中产生可检测到的核反冲。然而，如果暗物质通过与宇宙射线的碰撞被向上散射到高能，那么它可能在直接探测实验和中微子实验中都能被检测到。我们报告了一项专门寻找被宇宙射线向上散射的增强暗物质的结果，使用的是前景反应堆反中微子实验的太阳日数据。我们证明了这样的上散射暗物质通量将显示出特征的昼夜恒星调制，并利用这一点对表现出大相互作用截面的亚GeV暗物质设置了新的实验约束。
If dark matter has mass lower than around 1 GeV, it will not impart enough energy to cause detectable nuclear recoils in many direct-detection experiments. However, if dark matter is upscattered to high energy by collisions with cosmic rays, it may be detectable in both direct-detection experiments and neutrino experiments. We report the results of a dedicated search for boosted dark matter upscattered by cosmic rays, usingsolar days of data from the PROSPECT reactor antineutrino experiment. We show that such a flux of upscattered dark matter would display characteristic diurnal sidereal modulation, and use this to set new experimental constraints on sub-GeV dark matter exhibiting large interaction cross sections.
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速度最快的局部暗物质粒子来自大麦哲伦星云
影响因子：
6.4
作者：
Besla, G.;Peter, A.H.G.;Garavito-Camargo, N.
通讯作者：
Garavito-Camargo, N.
DOI：
10.3847/1538-4357/aad90c
发表时间：
2018-05
期刊：
The Astrophysical Journal
影响因子：
--
作者：
A. Abeysekara;R. Alfaro;C. Álvarez;J. Álvarez;R. Arceo;J. C. Arteaga-Vel'azquez;D. Rojas;H. Solares;A. Becerril;E. Belmont-Moreno;S. BenZvi;A. Bernal;J. Braun;K. Caballero-Mora;T. Capistrán;A. Carramiñana;S. Casanova;M. Castillo;U. Cotti;J. Cotzomi;C. D. Le'on;E. D. L. Fuente;R. Hernández;S. Dichiara;B. Dingus;M. DuVernois;J. C. Díaz-Vélez;K. Engel;D. Fiorino;N. Fraija;J. A. Garc'ia-Gonz'alez;F. Garfias;A. G. Muñoz;M. Gonz'alez;J. Goodman;Z. Hampel-Arias;J. P. Harding;S. Hernández;B. Hona;F. Hueyotl-Zahuantitla;C. Hui;P. Hüntemeyer;A. Iriarte;A. Jardin-Blicq;V. Joshi;S. Kaufmann;A. Lara;R. Lauer;W. Lee;H. L. Vargas;A. Longinotti;G. Luis-Raya;R. Luna-Garc'ia;D. L'opez-C'amara;R. L'opez-Coto;K. Malone;S. Marinelli;O. Martinez;I. Martinez-Castellanos;J. Mart'inez-Castro;H. Mart'inez-Huerta;J. Matthews;P. Miranda-Romagnoli;E. Moreno;M. Mostafá;A. Nayerhoda;L. Nellen;M. Newbold;M. Nisa;R. Noriega-Papaqui;R. Pelayo;J. Pretz;E. Pérez-Pérez-E.-Pérez-Pérez-1431205495;Z. Ren;C. Rho;C. Rivière;D. Rosa-Gonz'alez;M. Rosenberg;E. Ruiz-Velasco;F. Greus;A. Sandoval;M. Schneider;H. Schoorlemmer;M. Arroyo;G. Sinnis;A. Smith;R. Springer;P. Surajbali;I. Taboada;O. Tibolla;K. Tollefson;I. Torres;G. Vianello;L. Villaseñor;T. Weisgarber;F. Werner;S. Westerhoff;J. Wood;T. Yapici;A. Zepeda;H. Zhou
通讯作者：
A. Abeysekara;R. Alfaro;C. Álvarez;J. Álvarez;R. Arceo;J. C. Arteaga-Vel'azquez;D. Rojas;H. Solares;A. Becerril;E. Belmont-Moreno;S. BenZvi;A. Bernal;J. Braun;K. Caballero-Mora;T. Capistrán;A. Carramiñana;S. Casanova;M. Castillo;U. Cotti;J. Cotzomi;C. D. Le'on;E. D. L. Fuente;R. Hernández;S. Dichiara;B. Dingus;M. DuVernois;J. C. Díaz-Vélez;K. Engel;D. Fiorino;N. Fraija;J. A. Garc'ia-Gonz'alez;F. Garfias;A. G. Muñoz;M. Gonz'alez;J. Goodman;Z. Hampel-Arias;J. P. Harding;S. Hernández;B. Hona;F. Hueyotl-Zahuantitla;C. Hui;P. Hüntemeyer;A. Iriarte;A. Jardin-Blicq;V. Joshi;S. Kaufmann;A. Lara;R. Lauer;W. Lee;H. L. Vargas;A. Longinotti;G. Luis-Raya;R. Luna-Garc'ia;D. L'opez-C'amara;R. L'opez-Coto;K. Malone;S. Marinelli;O. Martinez;I. Martinez-Castellanos;J. Mart'inez-Castro;H. Mart'inez-Huerta;J. Matthews;P. Miranda-Romagnoli;E. Moreno;M. Mostafá;A. Nayerhoda;L. Nellen;M. Newbold;M. Nisa;R. Noriega-Papaqui;R. Pelayo;J. Pretz;E. Pérez-Pérez-E.-Pérez-Pérez-1431205495;Z. Ren;C. Rho;C. Rivière;D. Rosa-Gonz'alez;M. Rosenberg;E. Ruiz-Velasco;F. Greus;A. Sandoval;M. Schneider;H. Schoorlemmer;M. Arroyo;G. Sinnis;A. Smith;R. Springer;P. Surajbali;I. Taboada;O. Tibolla;K. Tollefson;I. Torres;G. Vianello;L. Villaseñor;T. Weisgarber;F. Werner;S. Westerhoff;J. Wood;T. Yapici;A. Zepeda;H. Zhou
宇宙学和宇宙粒子物理学杂志用 TeV 伽马射线天空探测银河系宇宙射线分布
DOI：
--
发表时间：
--
期刊：
影响因子：
--
作者：
H. Weber
通讯作者：
H. Weber
银河系中的暗物质碎片流动
影响因子：
5.5
作者：
M. Lisanti;D. Spergel
通讯作者：
D. Spergel
DOI：
10.3847/1538-4357/ab3afc
发表时间：
2018-10
期刊：
The Astrophysical Journal
影响因子：
--
作者：
L. Necib;M. Lisanti;S. Garrison-Kimmel;A. Wetzel;R. Sanderson;P. Hopkins;C. Faucher-Giguère;D. Ke
通讯作者：
L. Necib;M. Lisanti;S. Garrison-Kimmel;A. Wetzel;R. Sanderson;P. Hopkins;C. Faucher-Giguère;D. Ke