期刊
PHYSICS LETTERS B
卷 732, 期 -, 页码 373-379出版社
ELSEVIER
DOI: 10.1016/j.physletb.2014.04.003
关键词
Light dark matter; Fermi-LAT; Gamma ray; CDMS; CoGeNT
资金
- National Research Foundation of Korea (NRF) - Ministry of Education [2013R1A1A2006904, 2011-0029758, 2013R1A1A2061561]
- Korea Institute for Advanced Study (KIAS) - Korea government
- National Research Foundation of Korea [2013R1A1A2006904, 2013R1A1A2061561, 2011-0029758] Funding Source: Korea Institute of Science & Technology Information (KISTI), National Science & Technology Information Service (NTIS)
Light fermionic/scalar dark matter (DM) (m(Dm) approximate to 8 GeV) neutral under the standard model can be responsible for the CDMS and CoGeNT signals, and the Fermi-LAT gamma-ray excesses. In order to explain them in a relatively simple framework, we have explored various DM annihilation and scattering processes, discussing important phenomenological constraints coming from particle physics. Assuming that the two independent observations have a common DM origin and the processes arise through a common mediator, DM should annihilate into tau/anti-tau lepton pairs through an s-channel, and scatter with nuclei through a t-channel process. To avoid the p-wave suppression, a new Higgs-like scalar field with a mass of O(1) TeV is necessary as a common mediator of both the processes. We propose a supersymmetric model realizing the scenario. (C) 2014 The Authors. Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/3.0/).
作者
我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。
推荐
Article
Astronomy & Astrophysics
Inhomogeneity of a rotating quark-gluon plasma from holography
Nelson R. F. Braga, Octavio C. Junqueira
Summary: This study investigates the influence of rotation on the transition temperature of strongly interacting matter produced in non-central heavy ion collisions. By using a holographic description of an AdS black hole, the authors extend the analysis to the more realistic case where the matter spreads over a region around the rotational axis. The results show the coexistence of confined and deconfined phases and are consistent with the concept of local temperature in rotating frames developed by Tolman and Ehrenfest.
PHYSICS LETTERS B (2024)
Article
Astronomy & Astrophysics
Constrain the time variation of the gravitational constant via the propagation of gravitational waves
Bing Sun, Jiachen An, Zhoujian Cao
Summary: This paper investigates the effect of gravitational constant variation on the propagation of gravitational waves. By employing two analytical methods, the study finds that variations in the gravitational constant result in amplitude and phase corrections for gravitational waves, and the time variation of the gravitational constant can be constrained through the propagation of gravitational waves.
PHYSICS LETTERS B (2024)
Article
Astronomy & Astrophysics
Quantum tunneling from Schwarzschild black hole in non-commutative gauge theory of gravity
Abdellah Touati, Zaim Slimane
Summary: This letter presents the first study of Hawking radiation as a tunneling process within the framework of non-commutative gauge theory of gravity. The non-commutative Schwarzschild black hole is reconstructed using the Seiberg-Witten map and the star product. The emission spectrum of outgoing massless particles is computed using the quantum tunneling mechanism. The results reveal pure thermal radiation in the low-frequency scenario, but a deviation from pure thermal radiation in the high-frequency scenario due to energy conservation. It is also found that noncommutativity enhances the correlations between successively emitted particles.
PHYSICS LETTERS B (2024)
Article
Astronomy & Astrophysics
Compact stars: To cross or go around? That is the question
Shahar Hod
Summary: The travel times of light signals between two antipodal points on a compact star's surface are calculated for two different trajectories. It is shown that, for highly dense stars, the longer trajectory along the surface may have a shorter travel time as measured by asymptotic observers. A critical value of the dimensionless density-area parameter is determined for constant density stars to distinguish cases where crossing through the star's center or following a semi-circular trajectory on the surface has a shorter travel time as measured by asymptotic observers.
PHYSICS LETTERS B (2024)