Primordial gravitational waves as probe of dark matter in interferometer missions: Fisher forecast and MCMC
Abstract We propose novel inflationary primordial gravitational wave (GW) spectral shapes at interferometer-based current and future GW missions to test dark matter (DM) production via gravity-portal. We consider three right-handed neutrinos (RHNs), required to generate Standard Model (SM) neutrino...
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2024-12-01
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| Series: | Journal of High Energy Physics |
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| Online Access: | https://doi.org/10.1007/JHEP12(2024)150 |
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| author | Anish Ghoshal Debarun Paul Supratik Pal |
| author_facet | Anish Ghoshal Debarun Paul Supratik Pal |
| author_sort | Anish Ghoshal |
| collection | DOAJ |
| description | Abstract We propose novel inflationary primordial gravitational wave (GW) spectral shapes at interferometer-based current and future GW missions to test dark matter (DM) production via gravity-portal. We consider three right-handed neutrinos (RHNs), required to generate Standard Model (SM) neutrino masses via seesaw mechanism, are produced via gravity-portal in early universe. The lightest among them is stable and is the DM candidate of the Universe. The other two RHNs decay and generate matter-antimatter asymmetry due to baryogenesis via leptogenesis. We find that future GW detectors BBO, DECIGO, ET, for instance, are able to probe DM mass for 5 × 106 GeV < M DM < 1.6 × 107 GeV with a signal-to-noise ratio (SNR) > 10, along with the observed amount of baryon asymmetry due to gravitational leptogenesis for heavy RHN mass M N $$ {M}_{\mathcal{N}} $$ to be around 8 × 1012 GeV. Employing Fisher matrix forecast analysis, we identify the parameter space involving non-minimal coupling to gravity ξ, reheating temperature of the Universe T rh and DM mass M DM where the GW detector-sensitivities will be the maximum with the least error, along with SNR > 10. Finally, utilizing mock data for each GW detector, we perform MCMC analysis to find out the combined constraints on the various microphysics parameters. We also explore production of other cosmological relics such as QCD axion relic as DM candidate, produced via gravity-portal in early universe. We find that ET, for instance, can probe the decay constant of such DM candidates (fa) as 109 GeV ≲ fa ≲ 1014 GeV for misalignment angle θ i ∈ [0.1, π/ 3 $$ \sqrt{3} $$ ] and ξ = 1 with SNR > 10, whereas this range decreases with the increase of non-minimal coupling. Thus the upcoming GW missions will be able to test such non-thermal DM and baryogenesis scenarios involving very high energy scales, which is otherwise impossible to reach in particle physics experiments in laboratories. |
| format | Article |
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| institution | Kabale University |
| issn | 1029-8479 |
| language | English |
| publishDate | 2024-12-01 |
| publisher | SpringerOpen |
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| series | Journal of High Energy Physics |
| spelling | doaj-art-0c0670b7653a4f849ec368251fca00e62025-01-05T12:06:49ZengSpringerOpenJournal of High Energy Physics1029-84792024-12-0120241214410.1007/JHEP12(2024)150Primordial gravitational waves as probe of dark matter in interferometer missions: Fisher forecast and MCMCAnish Ghoshal0Debarun Paul1Supratik Pal2Institute of Theoretical Physics, Faculty of Physics, University of WarsawPhysics and Applied Mathematics Unit, Indian Statistical InstitutePhysics and Applied Mathematics Unit, Indian Statistical InstituteAbstract We propose novel inflationary primordial gravitational wave (GW) spectral shapes at interferometer-based current and future GW missions to test dark matter (DM) production via gravity-portal. We consider three right-handed neutrinos (RHNs), required to generate Standard Model (SM) neutrino masses via seesaw mechanism, are produced via gravity-portal in early universe. The lightest among them is stable and is the DM candidate of the Universe. The other two RHNs decay and generate matter-antimatter asymmetry due to baryogenesis via leptogenesis. We find that future GW detectors BBO, DECIGO, ET, for instance, are able to probe DM mass for 5 × 106 GeV < M DM < 1.6 × 107 GeV with a signal-to-noise ratio (SNR) > 10, along with the observed amount of baryon asymmetry due to gravitational leptogenesis for heavy RHN mass M N $$ {M}_{\mathcal{N}} $$ to be around 8 × 1012 GeV. Employing Fisher matrix forecast analysis, we identify the parameter space involving non-minimal coupling to gravity ξ, reheating temperature of the Universe T rh and DM mass M DM where the GW detector-sensitivities will be the maximum with the least error, along with SNR > 10. Finally, utilizing mock data for each GW detector, we perform MCMC analysis to find out the combined constraints on the various microphysics parameters. We also explore production of other cosmological relics such as QCD axion relic as DM candidate, produced via gravity-portal in early universe. We find that ET, for instance, can probe the decay constant of such DM candidates (fa) as 109 GeV ≲ fa ≲ 1014 GeV for misalignment angle θ i ∈ [0.1, π/ 3 $$ \sqrt{3} $$ ] and ξ = 1 with SNR > 10, whereas this range decreases with the increase of non-minimal coupling. Thus the upcoming GW missions will be able to test such non-thermal DM and baryogenesis scenarios involving very high energy scales, which is otherwise impossible to reach in particle physics experiments in laboratories.https://doi.org/10.1007/JHEP12(2024)150Early Universe Particle PhysicsParticle Nature of Dark MatterBaryo-and Leptogenesis |
| spellingShingle | Anish Ghoshal Debarun Paul Supratik Pal Primordial gravitational waves as probe of dark matter in interferometer missions: Fisher forecast and MCMC Journal of High Energy Physics Early Universe Particle Physics Particle Nature of Dark Matter Baryo-and Leptogenesis |
| title | Primordial gravitational waves as probe of dark matter in interferometer missions: Fisher forecast and MCMC |
| title_full | Primordial gravitational waves as probe of dark matter in interferometer missions: Fisher forecast and MCMC |
| title_fullStr | Primordial gravitational waves as probe of dark matter in interferometer missions: Fisher forecast and MCMC |
| title_full_unstemmed | Primordial gravitational waves as probe of dark matter in interferometer missions: Fisher forecast and MCMC |
| title_short | Primordial gravitational waves as probe of dark matter in interferometer missions: Fisher forecast and MCMC |
| title_sort | primordial gravitational waves as probe of dark matter in interferometer missions fisher forecast and mcmc |
| topic | Early Universe Particle Physics Particle Nature of Dark Matter Baryo-and Leptogenesis |
| url | https://doi.org/10.1007/JHEP12(2024)150 |
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