Pure gravitational dark matter, its mass and signatures
Wu, YL; Tang, Y; Tang, Y (reprint author), Korea Inst Adv Study, Seoul 02455, South Korea.
刊名PHYSICS LETTERS B
2016
卷号758页码:402-406
DOIhttp://dx.doi.org/10.1016/j.physletb.2016.05.045
英文摘要In this study, we investigate a scenario that dark matter (DM) has only gravitational interaction. In the framework of effective field theory of gravity, we find that DM is still stable at tree level even if there is no symmetry to protect its longevity, but could decay into standard model particles due to gravitational loop corrections. The radiative corrections can lead to both higher-and lower-dimensional effective operators. We also first explore how DM can be produced in the early universe. Through gravitational interaction at high temperature, DM is then found to have mass around TeV less than or similar to m(X) less than or similar to 10(11) GeV to get the right relic abundance. When DM decays, it mostly decays into gravitons, which could be tested by current and future CMB experiments. We also estimate the resulting fluxes for cosmic rays, gamma-ray and neutrino. (C) 2016 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/). Funded by SCOAP(3).
学科主题Astronomy & Astrophysics ; Physics
语种英语
内容类型期刊论文
源URL[http://ir.itp.ac.cn/handle/311006/21596]  
专题理论物理研究所_理论物理所1978-2010年知识产出
通讯作者Tang, Y (reprint author), Korea Inst Adv Study, Seoul 02455, South Korea.
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GB/T 7714
Wu, YL,Tang, Y,Tang, Y . Pure gravitational dark matter, its mass and signatures[J]. PHYSICS LETTERS B,2016,758:402-406.
APA Wu, YL,Tang, Y,&Tang, Y .(2016).Pure gravitational dark matter, its mass and signatures.PHYSICS LETTERS B,758,402-406.
MLA Wu, YL,et al."Pure gravitational dark matter, its mass and signatures".PHYSICS LETTERS B 758(2016):402-406.
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