Dark matter indirect searches: Multi-wavelength and anisotropies

14th International Conference on Topics in Astroparticle and Underground Physics

物理学;天文学

Ando, Shin'Ichiro^1

GRAPPA Institute, University of Amsterdam, Amsterdam

1098 XH, Netherlands^1

关键词: Analysis techniques;    Angular power spectrum;    Electromagnetic interactions;    Gamma ray flux distribution;    Gamma-ray background;    Spatial clustering;    The standard model;    Very high energies;   

Others  :  https://iopscience.iop.org/article/10.1088/1742-6596/718/2/022002/pdf
DOI  :  10.1088/1742-6596/718/2/022002

学科分类：天文学(综合)

来源: IOP

【 摘 要 】

If dark matter is made of particles governed by weak-scale physics, they may annihilate or decay to leave observable signatures in high-energy gamma-ray sky. In addition, any charged particles produced by the same process will also give low-frequency photons through successive electromagnetic interactions. Plenty of data from modern astrophysical measurements of various wavelengths, especially gamma rays, enabled new analysis techniques to search for these dark matter signatures with an unprecedented sensitivities. Since it is very likely that signatures of dark matter annihilation or decay is hidden in the gamma-ray data, one should fully utilize all available data including: (1) energy spectrum of all wavelengths ranging from radio to very-high-energy gamma rays; (2) spatial clustering probed with the angular power spectrum of the gamma-ray background; (3) cross correlation between the gamma-ray distribution with nearby galaxy catalogs; and (4) gamma-ray-flux distribution. I will review recent theoretical and observational developments in all these aspects, and discuss prospects for the future towards discovery of dark matter as an elementary particle in physics beyond the standard model.