Cosmic ray propagation and dark matter in light of the latest AMS-02 data
Cosmic ray propagation and dark matter in light of the latest AMS-02 data
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根据最新的 AMS-02 数据研究宇宙射线传播和暗物质
DOI：
10.1088/1475-7516/2015/09/049
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发表时间：
2014-10
影响因子：
6.4
通讯作者：
Zhou Yu Feng
中科院分区：
文献类型：
--
作者：
Jin Hong Bo;Wu Yue Liang;Zhou Yu Feng
The AMS-02 experiment is measuring the high energy cosmic rays with unprecedented accuracy. We explore the possibility of determining the cosmic-ray propagation models using the AMS-02 data alone. A global Bayesian analysis of the constraints on the cosmic-ray propagation models from the preliminary AMS-02 data on the Boron to Carbon nuclei flux ratio and proton flux is performed, with the assumption that the primary nucleon source is a broken power law in rigidity. The ratio of the diffusion coefficient D0 to the diffusive halo height Zh is determined with high accuracy D0/Zh≃ 2.00±0.07 cm2s−1kpc−1, and the value of the halo width is found to be Zh≃ 3.3 kpc with uncertainty less than 50%. As a consequence, the typical uncertainties in the positron fraction predicted from dark matter (DM) annihilation is reduced to a factor of two, and that in the antiproton flux is about an order of magnitude. Both of them are significantly smaller than that from the analyses prior to AMS-02. Taking into account the uncertainties and correlations in the propagation parameters, we derive conservative upper limits on the cross sections for DM annihilating into various standard model final states from the current PAMELA antiproton data. We also investigate the reconstruction capability of the future high precision AMS-02 antiproton data on the DM properties. The results show that for DM particles lighter than 0∼ 10 GeV and with typical thermal annihilation cross section, the cross section can be well reconstructed with uncertainties about a factor of two for the AMS-02 three-year data taking.
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影响因子：
6.5
作者：
Brigiano, Flavio Siro;Jeanvoine, Yannick;Spezia, Riccardo
通讯作者：
Spezia, Riccardo
影响因子：
6.4
作者：
Hong-Bo Jin;Yue-Liang Wu;Yu-feng Zhou
通讯作者：
Hong-Bo Jin;Yue-Liang Wu;Yu-feng Zhou
影响因子：
8.6
作者：
O. Adriani;G. Barbarino;G. Bazilevskaya;R. Bellotti;M. Boezio;É. Bogomolov;L. Bonechi;M. Bongi;V. Bonvicini;S. Bottai;A. Bruno;F. Cafagna;D. Campana;P. Carlson;M. Casolino;G. Castellini;M. P. Pascale;G. Rosa;D. Fedele;A. Galper;L. Grishantseva;P. Hofverberg;S. Koldashov;S. Krutkov;A. Kvashnin;A. Leonov;V. Malvezzi;L. Marcelli;W. Menn;V. Mikhailov;M. Minori;E. Mocchiutti;M. Nagni;S. Orsi;G. Osteria;P. Papini;M. Pearce;P. Picozza;M. Ricci;S. Ricciarini;M. Simon;R. Sparvoli;P. Spillantini;Y. Stozhkov;E. Taddei;A. Vacchi;E. Vannuccini;G. Vasilyev;S. Voronov;Y. Yurkin;G. Zampa;N. Zampa;V. Zverev
通讯作者：
O. Adriani;G. Barbarino;G. Bazilevskaya;R. Bellotti;M. Boezio;É. Bogomolov;L. Bonechi;M. Bongi;V. Bonvicini;S. Bottai;A. Bruno;F. Cafagna;D. Campana;P. Carlson;M. Casolino;G. Castellini;M. P. Pascale;G. Rosa;D. Fedele;A. Galper;L. Grishantseva;P. Hofverberg;S. Koldashov;S. Krutkov;A. Kvashnin;A. Leonov;V. Malvezzi;L. Marcelli;W. Menn;V. Mikhailov;M. Minori;E. Mocchiutti;M. Nagni;S. Orsi;G. Osteria;P. Papini;M. Pearce;P. Picozza;M. Ricci;S. Ricciarini;M. Simon;R. Sparvoli;P. Spillantini;Y. Stozhkov;E. Taddei;A. Vacchi;E. Vannuccini;G. Vasilyev;S. Voronov;Y. Yurkin;G. Zampa;N. Zampa;V. Zverev
DOI：
10.1088/0004-637x/728/2/122
发表时间：
2011-01
期刊：
The Astrophysical Journal
影响因子：
--
作者：
Y. Yoon;H. Ahn;P. Allison;M. G. Bagliesi;J. Beatty;G. Bigongiari;P. Boyle;P. Boyle;J. T. Childers-J
通讯作者：
Y. Yoon;H. Ahn;P. Allison;M. G. Bagliesi;J. Beatty;G. Bigongiari;P. Boyle;P. Boyle;J. T. Childers-J
DOI：
10.1088/1475-7516/2011/03/051
发表时间：
2011-03-01
影响因子：
6.4
作者：
Cirelli, Marco;Corcella, Gennaro;Strumia, Alessandro
通讯作者：
Strumia, Alessandro