Indirect search for dark matter from the Galactic Center and halo with the Super-Kamiokande detector
Indirect search for dark matter from the Galactic Center and halo with the Super-Kamiokande detector
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DOI：
10.1103/physrevd.102.072002
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发表时间：
2020-05
影响因子：
5
通讯作者：
K. Abe;C. Bronner;Y. Haga;Y. Hayato;M. Ikeda;S. Imaizumi;H. Ito;K. Iyogi;J. Kameda;Y. Kataoka;Y. Kato;Y. Kishimoto;L. Marti;M. Miura;S. Moriyama;T. Mochizuki;Y. Nagao;M. Nakahata;Y. Nakajima;T. Nakajima;S. Nakayama;T. Okada;K. Okamoto;A. Orii;G. Pronost;H. Sekiya;M. Shiozawa;Y. Sonoda;A. Takeda;A. Takenaka;H. Tanaka;S. Tasaka;T. Tomura;K. Ueno;T. Yano;T. Yokozawa;R. Akutsu;S. Han;T. Irvine;T. Kajita;I. Kametani;K. P. Lee-K. P.-Lee-2110644566;T. McLachlan;K. Okumura;E. Richard;T. Tashiro;R. Wang;J. Xia;D. Bravo-Berguño;L. Labarga;P. Fernandez;F. Blaszczyk;J. Gustafson;C. Kachulis;E. Kearns;J. Raaf;J. Stone;L. Sulak;S. Sussman;L. Wan;T. Wester;S. Berkman;S. Tobayama;J. Bian;G. Carminati;M. Elnimr;N. J. Griskevich;W. Kropp;S. Locke;S. Mine;A. Renshaw;M. Smy;H. Sobel;V. Takhistov;P. Weatherly;B. Hartfiel;J. Hill;W. Keig;N. Hong;J. Y. Kim-J. Y.-Kim-2110622921;I. Lim;R. Park;T. Akiri;B. Bodur;A. Himmel;Z. Li;E. O’Sullivan;K. Scholberg;C. Walter;T. Wongjirad;A. Coffani;O. Drapier;S. El Hedri;A. Giampaolo;M. Gonin;J. Imber;T. Mueller;P. Paganini;B. Quilain;T. Ishizuka;T. Nakamura;J. Jang;K. Choi;J. Learned;S. Matsuno;S. Smith;J. Amey;L. Anthony;R. P. Litchfield;W. Ma;A. Sztuc;Y. Uchida;M. Wascko;V. Berardi;M. Catanesi;R. A. Intonti;E. Radicioni;N. Calabria;L. Machado;G. De Rosa;G. Collazuol;F. Iacob;M. Lamoureux;N. Ospina;L. Ludovici;T. Boschi;F. Di Lodovico;S. Molina Sedgwick;S. Zsoldos;Y. Nishimura;S. Cao;M. Friend;T. Hasegawa;T. Ishida;T. Ishii;T. Kobayashi;T. Nakadaira;K. Nakamura;Y. Oyama;K. Sakashita;T. Sekiguchi;T. Tsukamoto;K. Abe;M. Hasegawa;Y. Isobe;H. Miyabe;Y. Nakano;T. Shiozawa;T. Sugimoto;A. Suzuki;Y. Takeuchi;S. Yamamoto;A. Ali;Y. Ashida;T. Hayashino;T. Hiraki;S. Hirota;K. Huang;K. Ieki;M. Jiang;T. Kikawa;M. Mori;A. Murakami;K. Nakamura;T. Nakaya;N. Patel;K. Suzuki;S. Takahashi;K. Tateishi;R. Wendell;N. McCauley;P. Mehta;A. Pritchard;K. Tsui;Y. Fukuda;Y. Itow;H. Menjo;G. Mitsuka;M. Murase;F. Muto;T. Niwa;K. Sato;T. Suzuki;M. Taani;M. Tsukada;P. Mijakowski;K. Frankiewicz;J. Hignight;C. Jung;X. Li;J. Palomino;G. Santucci;C. Vilela;M. Wilking;C. Yanagisawa;D. Fukuda;K. Hagiwara;M. Harada;T. Horai;H. Ishino;S. Ito;T. Kayano;A. Kibayashi;Y. Koshio;W. Ma;T. Mori;H. Nagata;N. Piplani;M. Sakuda;S. Seiya;Y. Takahira;C. Xu;R. Yamaguchi;Y. Kuno;G. Barr;D. Barrow;L. Cook;C. Simpson;D. Wark;F. Nova;R. Tacik;J. Y. Yang-J. Y.-Yang-2124818644;A. Cole;S. Jenkins;J. McElwee;M. Thiesse;L. Thompson;H. Okazawa;S. B. Kim-S. B.-Kim-2109632697;Y. Choi;K. Itô;K. Nishijima;K. Iwamoto;M. Koshiba;Y. Suda;M. Yokoyama;R. Calland;A. Goldsack;K. Martens;M. Murdoch;Y. Suzuki;M. Vagins;D. Hamabe;M. Kuze;Y. Okajima;M. Tanaka;T. Yoshida;M. Inomoto;M. Ishitsuka;R. Matsumoto;K. Ohta;M. Shinoki;J. F. Martin-J. F.-Martin-2110018099;C. Nantais;H. A. Tanaka-H. A.-Tanaka-1390470446;T. Towstego;M. Hartz;A. Konaka;P. de Perio;N. Prouse;S. Chen;B. D. Xu-B. D.-Xu-2258291899;Y. Zhang;B. Richards;K. Connolly;R. Wilkes;B. Jamieson;J. Walker;P. Giorgio;A. Minamino;G. Pintaudi
中科院分区：
文献类型：
--
作者：
K. Abe;C. Bronner;Y. Haga;Y. Hayato;M. Ikeda;S. Imaizumi;H. Ito;K. Iyogi;J. Kameda;Y. Kataoka;Y. Kato;Y. Kishimoto;L. Marti;M. Miura;S. Moriyama;T. Mochizuki;Y. Nagao;M. Nakahata;Y. Nakajima;T. Nakajima;S. Nakayama;T. Okada;K. Okamoto;A. Orii;G. Pronost;H. Sekiya;M. Shiozawa;Y. Sonoda;A. Takeda;A. Takenaka;H. Tanaka;S. Tasaka;T. Tomura;K. Ueno;T. Yano;T. Yokozawa;R. Akutsu;S. Han;T. Irvine;T. Kajita;I. Kametani;K. P. Lee-K. P.-Lee-2110644566;T. McLachlan;K. Okumura;E. Richard;T. Tashiro;R. Wang;J. Xia;D. Bravo-Berguño;L. Labarga;P. Fernandez;F. Blaszczyk;J. Gustafson;C. Kachulis;E. Kearns;J. Raaf;J. Stone;L. Sulak;S. Sussman;L. Wan;T. Wester;S. Berkman;S. Tobayama;J. Bian;G. Carminati;M. Elnimr;N. J. Griskevich;W. Kropp;S. Locke;S. Mine;A. Renshaw;M. Smy;H. Sobel;V. Takhistov;P. Weatherly;B. Hartfiel;J. Hill;W. Keig;N. Hong;J. Y. Kim-J. Y.-Kim-2110622921;I. Lim;R. Park;T. Akiri;B. Bodur;A. Himmel;Z. Li;E. O’Sullivan;K. Scholberg;C. Walter;T. Wongjirad;A. Coffani;O. Drapier;S. El Hedri;A. Giampaolo;M. Gonin;J. Imber;T. Mueller;P. Paganini;B. Quilain;T. Ishizuka;T. Nakamura;J. Jang;K. Choi;J. Learned;S. Matsuno;S. Smith;J. Amey;L. Anthony;R. P. Litchfield;W. Ma;A. Sztuc;Y. Uchida;M. Wascko;V. Berardi;M. Catanesi;R. A. Intonti;E. Radicioni;N. Calabria;L. Machado;G. De Rosa;G. Collazuol;F. Iacob;M. Lamoureux;N. Ospina;L. Ludovici;T. Boschi;F. Di Lodovico;S. Molina Sedgwick;S. Zsoldos;Y. Nishimura;S. Cao;M. Friend;T. Hasegawa;T. Ishida;T. Ishii;T. Kobayashi;T. Nakadaira;K. Nakamura;Y. Oyama;K. Sakashita;T. Sekiguchi;T. Tsukamoto;K. Abe;M. Hasegawa;Y. Isobe;H. Miyabe;Y. Nakano;T. Shiozawa;T. Sugimoto;A. Suzuki;Y. Takeuchi;S. Yamamoto;A. Ali;Y. Ashida;T. Hayashino;T. Hiraki;S. Hirota;K. Huang;K. Ieki;M. Jiang;T. Kikawa;M. Mori;A. Murakami;K. Nakamura;T. Nakaya;N. Patel;K. Suzuki;S. Takahashi;K. Tateishi;R. Wendell;N. McCauley;P. Mehta;A. Pritchard;K. Tsui;Y. Fukuda;Y. Itow;H. Menjo;G. Mitsuka;M. Murase;F. Muto;T. Niwa;K. Sato;T. Suzuki;M. Taani;M. Tsukada;P. Mijakowski;K. Frankiewicz;J. Hignight;C. Jung;X. Li;J. Palomino;G. Santucci;C. Vilela;M. Wilking;C. Yanagisawa;D. Fukuda;K. Hagiwara;M. Harada;T. Horai;H. Ishino;S. Ito;T. Kayano;A. Kibayashi;Y. Koshio;W. Ma;T. Mori;H. Nagata;N. Piplani;M. Sakuda;S. Seiya;Y. Takahira;C. Xu;R. Yamaguchi;Y. Kuno;G. Barr;D. Barrow;L. Cook;C. Simpson;D. Wark;F. Nova;R. Tacik;J. Y. Yang-J. Y.-Yang-2124818644;A. Cole;S. Jenkins;J. McElwee;M. Thiesse;L. Thompson;H. Okazawa;S. B. Kim-S. B.-Kim-2109632697;Y. Choi;K. Itô;K. Nishijima;K. Iwamoto;M. Koshiba;Y. Suda;M. Yokoyama;R. Calland;A. Goldsack;K. Martens;M. Murdoch;Y. Suzuki;M. Vagins;D. Hamabe;M. Kuze;Y. Okajima;M. Tanaka;T. Yoshida;M. Inomoto;M. Ishitsuka;R. Matsumoto;K. Ohta;M. Shinoki;J. F. Martin-J. F.-Martin-2110018099;C. Nantais;H. A. Tanaka-H. A.-Tanaka-1390470446;T. Towstego;M. Hartz;A. Konaka;P. de Perio;N. Prouse;S. Chen;B. D. Xu-B. D.-Xu-2258291899;Y. Zhang;B. Richards;K. Connolly;R. Wilkes;B. Jamieson;J. Walker;P. Giorgio;A. Minamino;G. Pintaudi
我们基于1996年至2016年的Super-Kamiokande-I，-II，-III和-IV的数据集，以弱相互作用大质量粒子（WIMPs）的形式在银河系中心或晕中湮灭，从而寻找由于暗物质导致的过量中微子相互作用。假设WIMP自湮灭对$\nu \overline{\nu}$、$\mu^+\mu^-$、$B\overline{B}$或$W^+W^-$起主导作用，我们模拟了中微子的通量、能量和味分布。过量是在比较大气中微子相互作用的详细建模和拟合数据。对于1 GeV至10 TeV范围内的WIMP质量，推导出自湮没截面$\langle \sigma_{A} V \rangle$的极限，对于$B\bar B$模式下的5 GeV WIMP，最低可达9.6\times 10 ^{-23}$cm $^3 $ s$^{-1}$，对于$模式下的1 GeV WIMP，最低可达1.2\times 10 ^{-24}$cm $^3 $ s$^{-1}$。\nu \bar \nu$模式。所获得的灵敏度的超级神冈探测器的WIMP质量低于几十个GeV是最好的类似的间接搜索到目前为止。
We present a search for an excess of neutrino interactions due to dark matter in the form of Weakly Interacting Massive Particles (WIMPs) annihilating in the galactic center or halo based on the data set of Super-Kamiokande-I, -II, -III and -IV taken from 1996 to 2016. We model the neutrino flux, energy, and flavor distributions assuming WIMP self-annihilation is dominant to $\nu \overline{\nu}$, $\mu^+\mu^-$, $b\overline{b}$, or $W^+W^-$. The excess is in comparison to atmospheric neutrino interactions which are modeled in detail and fit to data. Limits on the self-annihilation cross section $\langle \sigma_{A} V \rangle$ are derived for WIMP masses in the range 1 GeV to 10 TeV, reaching as low as $9.6 \times10^{-23}$ cm$^3$ s$^{-1}$ for 5 GeV WIMPs in $b\bar b$ mode and $1.2 \times10^{-24}$ cm$^3$ s$^{-1}$ for 1 GeV WIMPs in $\nu \bar \nu$ mode. The obtained sensitivity of the Super-Kamiokande detector to WIMP masses below several tens of GeV is the best among similar indirect searches to date.