利用米格达尔效应的WIMP非弹性散射有效模型的低质量约束

IF 5.3 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Sunghyun Kang, Stefano Scopel and Gaurav Tomar
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引用次数: 0

摘要

我们利用米格达尔效应将质量为mχ且自旋为1/2的WIMP的非相对论有效场论的有效耦合边界扩展到低质量,通过上散射到质量分裂δ >的较重状态或下散射到δ < 0的较轻状态来与原子核进行非弹性相互作用。为了做到这一点,我们对mχ-δ参数空间中的Migdal界进行了系统的分析,并将它们与核反冲搜索的边界进行了比较。米格达尔效应允许将δ < 0的核反冲界显著扩展到低WIMP质量。在这种情况下,边界是由XENON1T驱动的,除非δ消失或非常小,当,取决于wimp -核相互作用,在mχ范围的下端DS50或SuperCDMS更有约束。另一方面,当δ >和WIMP粒子向上散射到较重的状态时,核反冲界比米格达尔效应强。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Low-mass constraints on WIMP effective models of inelastic scattering using the Migdal effect
We use the Migdal effect to extend to low masses the bounds on each of the effective couplings of the non-relativistic effective field theory of a WIMP of mass mχ and spin 1/2 that interacts inelastically with nuclei by either upscattering to a heavier state with mass splitting δ > 0 or by downscattering to a lighter state with δ < 0. In order to do so we perform a systematic analysis of the Migdal bounds in the mχ-δ parameter space comparing them to those from nuclear recoil searches. The Migdal effect allows to significantly extend to low WIMP masses the nuclear recoil bounds for δ < 0. In this case the bounds are driven by XENON1T, except when δ is vanishing or very small, when, depending on the WIMP-nucleus interaction, in the lower end of the mχ range either DS50 or SuperCDMS are more constraining. On the other hand, when δ > 0 and the WIMP particle upscatters to a heavier state nuclear recoil bounds are stronger than those from the Migdal effect.
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来源期刊
Journal of Cosmology and Astroparticle Physics
Journal of Cosmology and Astroparticle Physics 地学天文-天文与天体物理
CiteScore
10.20
自引率
23.40%
发文量
632
审稿时长
1 months
期刊介绍: Journal of Cosmology and Astroparticle Physics (JCAP) encompasses theoretical, observational and experimental areas as well as computation and simulation. The journal covers the latest developments in the theory of all fundamental interactions and their cosmological implications (e.g. M-theory and cosmology, brane cosmology). JCAP''s coverage also includes topics such as formation, dynamics and clustering of galaxies, pre-galactic star formation, x-ray astronomy, radio astronomy, gravitational lensing, active galactic nuclei, intergalactic and interstellar matter.
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