Probing Dark Sectors with Neutron Stars

Tensions in the measurements of neutron and kaon weak decays, such as of the neutron lifetime, may speak to the existence of new particles and dynamics not present in the Standard Model (SM). In scenarios with dark sectors, particles that couple feebly to those of the SM appear. We offer a focused o...

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Main Authors: Susan Gardner, Mohammadreza Zakeri
Format: Article
Language:English
Published: MDPI AG 2024-02-01
Series:Universe
Subjects:
Online Access:https://www.mdpi.com/2218-1997/10/2/67
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author Susan Gardner
Mohammadreza Zakeri
author_facet Susan Gardner
Mohammadreza Zakeri
author_sort Susan Gardner
collection DOAJ
description Tensions in the measurements of neutron and kaon weak decays, such as of the neutron lifetime, may speak to the existence of new particles and dynamics not present in the Standard Model (SM). In scenarios with dark sectors, particles that couple feebly to those of the SM appear. We offer a focused overview of such possibilities and describe how the observations of neutron stars, which probe either their structure or dynamics, limit them. In realizing these constraints, we highlight how the assessment of particle processes within dense baryonic matter impacts the emerging picture—and we emphasize both the flavor structure of the constraints and their broader connections to cogenesis models of dark matter and baryogenesis.
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spelling doaj.art-ce529f52b8de45719a2d5b902be743f12024-02-23T15:36:45ZengMDPI AGUniverse2218-19972024-02-011026710.3390/universe10020067Probing Dark Sectors with Neutron StarsSusan Gardner0Mohammadreza Zakeri1Department of Physics and Astronomy, University of Kentucky, Lexington, KY 40506-0055, USADepartment of Physics and Astronomy, University of Kentucky, Lexington, KY 40506-0055, USATensions in the measurements of neutron and kaon weak decays, such as of the neutron lifetime, may speak to the existence of new particles and dynamics not present in the Standard Model (SM). In scenarios with dark sectors, particles that couple feebly to those of the SM appear. We offer a focused overview of such possibilities and describe how the observations of neutron stars, which probe either their structure or dynamics, limit them. In realizing these constraints, we highlight how the assessment of particle processes within dense baryonic matter impacts the emerging picture—and we emphasize both the flavor structure of the constraints and their broader connections to cogenesis models of dark matter and baryogenesis.https://www.mdpi.com/2218-1997/10/2/67neutron starsbaryon numberneutron lifetime anomalydark matterdark sectors
spellingShingle Susan Gardner
Mohammadreza Zakeri
Probing Dark Sectors with Neutron Stars
Universe
neutron stars
baryon number
neutron lifetime anomaly
dark matter
dark sectors
title Probing Dark Sectors with Neutron Stars
title_full Probing Dark Sectors with Neutron Stars
title_fullStr Probing Dark Sectors with Neutron Stars
title_full_unstemmed Probing Dark Sectors with Neutron Stars
title_short Probing Dark Sectors with Neutron Stars
title_sort probing dark sectors with neutron stars
topic neutron stars
baryon number
neutron lifetime anomaly
dark matter
dark sectors
url https://www.mdpi.com/2218-1997/10/2/67
work_keys_str_mv AT susangardner probingdarksectorswithneutronstars
AT mohammadrezazakeri probingdarksectorswithneutronstars