A couplet from flavored dark matter

被引:32
作者
Agrawal, Prateek [1 ]
Chacko, Zackaria [2 ]
Kilic, Can [3 ,4 ]
Verhaaren, Christopher B. [2 ]
机构
[1] Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA
[2] Univ Maryland, Dept Phys, Maryland Ctr Fundamental Phys, College Pk, MD 20742 USA
[3] Univ Texas Austin, Dept Phys, Theory Grp, Austin, TX 78712 USA
[4] Univ Texas Austin, Texas Cosmol Ctr, Austin, TX 78712 USA
来源
JOURNAL OF HIGH ENERGY PHYSICS | 2015年 / 08期
基金
美国国家科学基金会; 美国能源部;
关键词
Beyond Standard Model; Cosmology of Theories beyond the SM; Global Symmetries; X-RAY-LINE; SIGNAL; MODELS; HIGGS;
D O I
10.1007/JHEP08(2015)072
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We show that a couplet, a pair of closely spaced photon lines, in the X-ray spectrum is a distinctive feature of lepton flavored dark matter models for which the mass spectrum is dictated by Minimal Flavor Violation. In such a scenario, mass splittings between different dark matter flavors are determined by Standard Model Yukawa couplings and can naturally be small, allowing all three flavors to be long-lived and contribute to the observed abundance. Then, in the presence of a tiny source of flavor violation, heavier dark matter flavors can decay via a dipole transition on cosmological timescales, giving rise to three photon lines. Two of these lines are closely spaced, and constitute the couplet. Provided the flavor violation is sufficiently small, the ratios of the line energies are determined in terms of the charged lepton masses, and constitute a prediction of this framework. For dark matter masses of order the weak scale, the couplet lies in the keV-MeV region, with a much weaker line in the eV-keV region. This scenario constitutes a potential explanation for the recent claim of the observation of a 3.5 keV line. The next generation of X-ray telescopes may have the necessary resolution to resolve the double line structure of such a couplet.
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页数:21
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