A consistent theory of decaying Dark Matter connecting IceCube to the Sesame Street

被引:27
|
作者
Chianese, Marco [1 ,2 ,3 ]
Merle, Alexander [3 ]
机构
[1] INFN, Sez Napoli, Complesso Univ Monte S Angelo, I-80126 Naples, Italy
[2] Univ Napoli Federico II, Dipartimento Fis Ettore Pancini, Complesso Univ Monte S Angelo, I-80126 Naples, Italy
[3] Werner Heisenberg Inst, Max Planck Inst Phys, Fohringer Ring 6, D-80805 Munich, Germany
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2017年 / 04期
关键词
dark matter theory; physics of the early universe; ultra high energy photons and neutrinos; MAJORANA NEUTRINO MASSES; X-RAY; SEARCHES; GRAVITY; EVENTS; MODEL;
D O I
10.1088/1475-7516/2017/04/017
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The high energy events observed at the IceCube Neutrino Observatory have triggered many investigations interpreting the highly energetic neutrinos detected as decay products of heavy unstable Dark Matter particles. However, while very detailed treatments of the IceCube phenomenology exist, only a few references focus on the (non-trivial) Dark Matter production part - and all of those rely on relatively complicated new models which are not always testable directly. We instead investigate two of the most minimal scenarios possible, where the operator responsible for the IceCube events is directly involved in Dark Matter production. We show that the simplest (four-dimensional) operator is not powerful enough to accommodate all constraints. A more non-minimal setting (at mass dimension six), however, can do both fitting all the data and also allowing for a comparatively small parameter space only, parts of which can be in reach of future observations. We conclude that minimalistic approaches can be enough to explain all data required, while complicated new physics seems not to be required by IceCube.
引用
收藏
页数:25
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