Complementarity of Galactic radio and collider data in constraining WIMP dark matter models

被引：28

作者：

Mambrini, Yann ^{[1
]}

Tytgat, Michel H. G. ^{[2
]}

Zaharijas, Gabrijela ^{[3
,4
]}

Zaldivar, Bryan ^{[5
]}

机构：

[1] Univ Paris 11, Phys Theor Lab, F-91405 Orsay, France

[2] Univ Libre Bruxelles, Serv Phys Theor, B-1050 Brussels, Belgium

[3] Abdus Salam Int Ctr Theoret Phys, I-34014 Trieste, Italy

[4] CEA Saclay, Inst Phys Theor, F-91191 Gif Sur Yvette, France

[5] UAM, CSIC, IFT, Madrid 28049, Spain

来源：

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2012年 / 11期

关键词：

dark matter theory; dark matter experiments; absorption and radiation processes; COSMIC-RAY PROPAGATION; ROTATION MEASURES; MAGNETIC-FIELD; HIGGS; PHOTON; ANNIHILATION; RADIATION; EMISSION; SPECTRUM;

D O I：

10.1088/1475-7516/2012/11/038

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In this work we confront dark matter models to constraints that may be derived from radio synchrotron radiation from the Galaxy, taking into account the astrophysical uncertainties and we compare these to bounds set by accelerator and complementary indirect dark matter searches. Specifically we apply our analysis to three popular particle physics models. First, a generic effective operator approach, in which case we set bounds on the corresponding mass scale, and then, two specific UV completions, the Z' and Higgs portals. We show that for many candidates, the radio synchrotron limits are competitive with the other searches, and could even give the strongest constraints (as of today) with some reasonable assumptions regarding the astrophysical uncertainties.

引用

页数：39

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