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DC Field | Value | Language |
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dc.contributor.author | Banerjee, Vivek | - |
dc.contributor.author | Mishra, Sasmita | - |
dc.date.accessioned | 2024-02-09T04:56:45Z | - |
dc.date.available | 2024-02-09T04:56:45Z | - |
dc.date.issued | 2024-01 | - |
dc.identifier.citation | International Conference on Future Prospect in Neutrino and Astroparticle Physics (ICFPNAP), Assam Don Bosco University, 23-24 January 2024 | en_US |
dc.identifier.uri | http://hdl.handle.net/2080/4373 | - |
dc.description | Copyright belongs to proceeding publisher | en_US |
dc.description.abstract | The gap between experimental average and standard model value for the muon anomalous magnetic moment is a direct hint of fields beyond standard model. In this work we investigate the contribution of heavy right-handed neutrino for muon (g - 2) in left-right symmetric model. Simultaneously we have checked the dominance(type-I and type-II) patterns for the Majorana type Yukawa coupling matrix and found the effective ones. Our study shows two energy range solutions for right-neutrino, one at low energy (1 Gev) and another at high energy (around 5 TeV to 100 TeV) both giving viable contributions in the gap ∆aµ. Study shows that two of the included right-handed neutrinos may be the possible candidate for dark matter as they satisfy the 3.55 keV line spectra. | en_US |
dc.subject | Neutrino magnetic moment | en_US |
dc.subject | Dark matter | en_US |
dc.title | Dark Connection of Muon (g − 2) | en_US |
dc.type | Presentation | en_US |
Appears in Collections: | Conference Papers |
Files in This Item:
File | Description | Size | Format | |
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2024_ICFPNAP_VBanerjee_Dark.pdf | 6.1 MB | Adobe PDF | View/Open Request a copy |
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