Collider tests of nanohertz gravitational waves
Recently, compelling evidence of nanohertz gravitational waves is indicated by the pulsar timing array collaborations. We present an MeV-scale first-order phase transition from a minimal dark sector to explain the gravitational waves, with a focus on the collider tests via the Higgs portal interacti...
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EDP Sciences
2024-01-01
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Series: | EPJ Web of Conferences |
Online Access: | https://www.epj-conferences.org/articles/epjconf/pdf/2024/25/epjconf_lcws2024_01013.pdf |
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author | Li Shao-Ping |
author_facet | Li Shao-Ping |
author_sort | Li Shao-Ping |
collection | DOAJ |
description | Recently, compelling evidence of nanohertz gravitational waves is indicated by the pulsar timing array collaborations. We present an MeV-scale first-order phase transition from a minimal dark sector to explain the gravitational waves, with a focus on the collider tests via the Higgs portal interaction. We demonstrate that to explain the observed gravitational waves, the Higgs portal coupling should be so sizable that it can be probed through Higgs invisible decay at the LHC and future colliders such as HL-LHC, CEPC, ILC, and FCC-ee. It opens up a promising avenue to uncover the physical origin of the nanohertz gravitational waves via colliders and to hear and see the minimal dark sector. |
format | Article |
id | doaj-art-9f1bbf289f8f44beb91550940141eed8 |
institution | Kabale University |
issn | 2100-014X |
language | English |
publishDate | 2024-01-01 |
publisher | EDP Sciences |
record_format | Article |
series | EPJ Web of Conferences |
spelling | doaj-art-9f1bbf289f8f44beb91550940141eed82025-01-06T11:33:47ZengEDP SciencesEPJ Web of Conferences2100-014X2024-01-013150101310.1051/epjconf/202431501013epjconf_lcws2024_01013Collider tests of nanohertz gravitational wavesLi Shao-Ping0Department of Physics, Osaka UniversityRecently, compelling evidence of nanohertz gravitational waves is indicated by the pulsar timing array collaborations. We present an MeV-scale first-order phase transition from a minimal dark sector to explain the gravitational waves, with a focus on the collider tests via the Higgs portal interaction. We demonstrate that to explain the observed gravitational waves, the Higgs portal coupling should be so sizable that it can be probed through Higgs invisible decay at the LHC and future colliders such as HL-LHC, CEPC, ILC, and FCC-ee. It opens up a promising avenue to uncover the physical origin of the nanohertz gravitational waves via colliders and to hear and see the minimal dark sector.https://www.epj-conferences.org/articles/epjconf/pdf/2024/25/epjconf_lcws2024_01013.pdf |
spellingShingle | Li Shao-Ping Collider tests of nanohertz gravitational waves EPJ Web of Conferences |
title | Collider tests of nanohertz gravitational waves |
title_full | Collider tests of nanohertz gravitational waves |
title_fullStr | Collider tests of nanohertz gravitational waves |
title_full_unstemmed | Collider tests of nanohertz gravitational waves |
title_short | Collider tests of nanohertz gravitational waves |
title_sort | collider tests of nanohertz gravitational waves |
url | https://www.epj-conferences.org/articles/epjconf/pdf/2024/25/epjconf_lcws2024_01013.pdf |
work_keys_str_mv | AT lishaoping collidertestsofnanohertzgravitationalwaves |