Cogenesis of baryon and dark matter with PBHs and the QCD axion
With entropy injection, an early matter-dominated epoch (EMD) impels the axion decay constant <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:msub><a:mi>f</a:mi><a:mi>a</a:mi></a:msub></a:math> toward larger values to produce correct axion dark matter (DM) abundance, thereby unfolding the low-mass axion (<c:math xmlns:c="http://www.w3.org/1998/Math/MathML" display="inline"><c:mrow><c:msub><c:mrow><c:mi>m</c:mi></c:mrow><c:mrow><c:mi>a</c:mi></c:mrow></c:msub><c:mo>≲</c:mo><c:msup><c:mrow><c:mn>10</c:mn></c:mrow><c:mrow><c:mo>−</c:mo><c:mn>5</c:mn></c:mrow></c:msup><c:mtext> </c:mtext><c:mtext> </c:mtext><c:mi>eV</c:mi></c:mrow></c:math>) parameter space to be searched for in axion experiments. We implement this proposition in a scenario where <e:math xmlns:e="http://www.w3.org/1998/Math/MathML" display="inline"><e:msub><e:mi>f</e:mi><e:mi>a</e:mi></e:msub></e:math> and the leptogenesis scale in a seesaw mechanism are equivalent. We show that if, instead, the EMD is provided by evaporating ultralight primordial black holes (PBHs), the scenario becomes strikingly testable with gravitational wave (GW) background alongside the axion searches. In particular, while being consistent with correct axion DM abundance, the scale <g:math xmlns:g="http://www.w3.org/1998/Math/MathML" display="inline"><g:mrow><g:msub><g:mrow><g:mi>f</g:mi></g:mrow><g:mrow><g:mi>a</g:mi></g:mrow></g:msub><g:mo>≳</g:mo><g:msup><g:mrow><g:mn>10</g:mn></g:mrow><g:mrow><g:mn>12</g:mn></g:mrow></g:msup><g:mtext> </g:mtext><g:mtext> </g:mtext><g:mi>GeV</g:mi></g:mrow></g:math>, corresponding to the unflavored regime of leptogenesis with hierarchical right-handed neutrinos, can be probed with GW and axion experiments, which is otherwise not testable at neutrino or collider experiments. Additionally, axions produced from PBH evaporation can give rise to dark radiation within reach of future cosmic microwave background experiments. Published by the American Physical Society 2024
Authors
- Debasish Borah (ORCID: https://orcid.org/0000-0001-8375-282X)
- Rome Samanta (ORCID: https://orcid.org/0000-0003-3670-4889)
- Nayan Das (ORCID: https://orcid.org/0000-0002-7627-0889)
- Suruj Jyoti Das (ORCID: https://orcid.org/0000-0002-4144-1799)
Institutions
- Indian Institute of Technology Guwahati (IN)
- Institute for Basic Science (KR)
- Istituto Nazionale di Fisica Nucleare, Sezione di Napoli (IT)
- Scuola Superiore Meridionale (IT)
Publication Details
- Journal
- Physical review. D/Physical review. D.
- Published
- 2024-12-11
- DOI
- https://doi.org/10.1103/physrevd.110.115013
- Citations
- 5
- Primary Topic
- Dark Matter and Cosmic Phenomena
- Type
- article
- Field-Weighted Citation Impact
- 3.30
Funders
- Tata Institute of Fundamental Research
- Ministry of Education, India
- Institute for Basic Science
- Istituto Nazionale di Fisica Nucleare
- Science and Engineering Research Board
- Instituto Nazionale di Fisica Nucleare