Implications of Sgr A$^\ast$ on the $γ$-rays searches of Bino Dark Matter with $(g-2)_μ$
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| Format: | Preprint |
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2024
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| author | Chattopadhyay, Utpal Das, Debottam Poddar, Sujoy Puri, Rahul Saha, Abhijit Kumar |
| author_facet | Chattopadhyay, Utpal Das, Debottam Poddar, Sujoy Puri, Rahul Saha, Abhijit Kumar |
| contents | We analyse the impact of dark matter density spike around the Milky Way's supermassive black hole (SMBH), Sgr A$^*$, in probing the Bino-dominated neutralino dark matter (DM) $\tilde χ_1^0$ within the MSSM, which typically produces relatively faint signals in the conventional DM halos. In particular, we explore the indirect search prospects of sub-TeV Bino-Higgsino and Bino-Wino-Higgsino DM in the MSSM, consistent with the supersymmetric predictions required to explain the anomalous magnetic moment of the muon. Typical over-abundance of Bino DM is ameliorated with slepton and/or Wino coannihilations. The lightest neutralino, thus, may be associated with a compressed supersymmetric particle spectrum, which, in general, is difficult to probe at conventional LHC searches. Similarly, for a rather tiny Higgsino mixing, $\tilde χ_1^0$ does not offer much prospect to assess its predictions at dark matter direct detection searches. Accommodating the inclusive effects of density spike, here, we present the requisite boost factor to facilitate $γ-$ray searches of Bino-dominated DM in the MSSM, especially focusing on the Fermi-LAT and HESS observations. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2407_14603 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Implications of Sgr A$^\ast$ on the $γ$-rays searches of Bino Dark Matter with $(g-2)_μ$ Chattopadhyay, Utpal Das, Debottam Poddar, Sujoy Puri, Rahul Saha, Abhijit Kumar High Energy Physics - Phenomenology Cosmology and Nongalactic Astrophysics We analyse the impact of dark matter density spike around the Milky Way's supermassive black hole (SMBH), Sgr A$^*$, in probing the Bino-dominated neutralino dark matter (DM) $\tilde χ_1^0$ within the MSSM, which typically produces relatively faint signals in the conventional DM halos. In particular, we explore the indirect search prospects of sub-TeV Bino-Higgsino and Bino-Wino-Higgsino DM in the MSSM, consistent with the supersymmetric predictions required to explain the anomalous magnetic moment of the muon. Typical over-abundance of Bino DM is ameliorated with slepton and/or Wino coannihilations. The lightest neutralino, thus, may be associated with a compressed supersymmetric particle spectrum, which, in general, is difficult to probe at conventional LHC searches. Similarly, for a rather tiny Higgsino mixing, $\tilde χ_1^0$ does not offer much prospect to assess its predictions at dark matter direct detection searches. Accommodating the inclusive effects of density spike, here, we present the requisite boost factor to facilitate $γ-$ray searches of Bino-dominated DM in the MSSM, especially focusing on the Fermi-LAT and HESS observations. |
| title | Implications of Sgr A$^\ast$ on the $γ$-rays searches of Bino Dark Matter with $(g-2)_μ$ |
| topic | High Energy Physics - Phenomenology Cosmology and Nongalactic Astrophysics |
| url | https://arxiv.org/abs/2407.14603 |