- Letter
- Open Access
scalar in the early Universe and
Phys. Rev. D 105, L051702 – Published 14 March, 2022
DOI: https://doi.org/10.1103/PhysRevD.105.L051702
Abstract
We investigate a concrete scenario of a light scalar with a mass around 1 MeV which can be connected to the origin of neutrino masses and simultaneously survive current bounds on relativistic degrees of freedom in the early universe. A feeble coupling to the Standard Model neutrinos can relax stringent bounds on the decays to photons inferred from the measured value of . Interestingly, we find that such a scalar whose diphoton coupling is generated by a tree-level coupling to the muon of similar strength as that of the Standard Model Higgs boson can simultaneously explain the longstanding discrepancy in the measured value of the muon magnetic moment. We present a possible ultraviolet (UV) completion of this scenario providing a link between new physics in the early universe and the generation of neutrino masses.
Physics Subject Headings (PhySH)
Article Text
Supplemental Material
References (59)
- P. A. Zyla et al. (Particle Data Group), Prog. Theor. Exp. Phys. 2020, 083C01 (2020).
- M. Trodden and S. M. Carroll, in Theoretical Advanced Study Institute in Elementary Particle Physics (TASI 2002): Particle Physics and Cosmology: The Quest for Physics Beyond the Standard Model(s) (2004), pp. 703–793, .
- K. A. Olive and D. Thomas, Astropart. Phys. 11, 403 (1999).
- S. Hannestad and G. Raffelt, J. Cosmol. Astropart. Phys. 04 (2004) 008.
- M. Millea, L. Knox, and B. Fields, Phys. Rev. D 92, 023010 (2015).
- N. Sabti, J. Alvey, M. Escudero, M. Fairbairn, and D. Blas, J. Cosmol. Astropart. Phys. 01 (2020) 004.
- P. F. Depta, M. Hufnagel, and K. Schmidt-Hoberg, J. Cosmol. Astropart. Phys. 05 (2020) 009.
- P. Carenza, O. Straniero, B. Döbrich, M. Giannotti, G. Lucente, and A. Mirizzi, Phys. Lett. B 809, 135709 (2020).
- C. Giovanetti, M. Lisanti, H. Liu, and J. T. Ruderman, arXiv:2109.03246.
- B. Batell and A. Ghalsasi, arXiv:2109.04476.
- G.-y. Huang and W. Rodejohann, Phys. Rev. D 103, 123007 (2021).
- B. Abi et al. (Muon g-2 Collaboration), Phys. Rev. Lett. 126, 141801 (2021).
- M. Davier, A. Hoecker, B. Malaescu, and Z. Zhang, Eur. Phys. J. C 71, 1515 (2011); 72, 1874(E) (2012).
- T. Aoyama, M. Hayakawa, T. Kinoshita, and M. Nio, Phys. Rev. Lett. 109, 111808 (2012).
- T. Aoyama, T. Kinoshita, and M. Nio, Atoms 7, 28 (2019).
- A. Czarnecki, W. J. Marciano, and A. Vainshtein, Phys. Rev. D 67, 073006 (2003); 73, 119901(E) (2006).
- C. Gnendiger, D. Stöckinger, and H. Stöckinger-Kim, Phys. Rev. D 88, 053005 (2013).
- M. Davier, A. Hoecker, B. Malaescu, and Z. Zhang, Eur. Phys. J. C 77, 827 (2017).
- A. Keshavarzi, D. Nomura, and T. Teubner, Phys. Rev. D 97, 114025 (2018).
- G. Colangelo, M. Hoferichter, and P. Stoffer, J. High Energy Phys. 02 (2019) 006.
- M. Hoferichter, B.-L. Hoid, and B. Kubis, J. High Energy Phys. 08 (2019) 137.
- M. Davier, A. Hoecker, B. Malaescu, and Z. Zhang, Eur. Phys. J. C 80, 241 (2020); 80, 410(E) (2020).
- A. Keshavarzi, D. Nomura, and T. Teubner, Phys. Rev. D 101, 014029 (2020).
- A. Kurz, T. Liu, P. Marquard, and M. Steinhauser, Phys. Lett. B 734, 144 (2014).
- K. Melnikov and A. Vainshtein, Phys. Rev. D 70, 113006 (2004).
- P. Masjuan and P. Sánchez-Puertas, Phys. Rev. D 95, 054026 (2017).
- G. Colangelo, M. Hoferichter, M. Procura, and P. Stoffer, J. High Energy Phys. 04 (2017) 161.
- M. Hoferichter, B.-L. Hoid, B. Kubis, S. Leupold, and S. P. Schneider, J. High Energy Phys. 10 (2018) 141.
- A. Gérardin, H. B. Meyer, and A. Nyffeler, Phys. Rev. D 100, 034520 (2019).
- J. Bijnens, N. Hermansson-Truedsson, and A. Rodríguez-Sánchez, Phys. Lett. B 798, 134994 (2019).
- G. Colangelo, F. Hagelstein, M. Hoferichter, L. Laub, and P. Stoffer, J. High Energy Phys. 03 (2020) 101.
- T. Blum, N. Christ, M. Hayakawa, T. Izubuchi, L. Jin, C. Jung, and C. Lehner, Phys. Rev. Lett. 124, 132002 (2020).
- G. Colangelo, M. Hoferichter, A. Nyffeler, M. Passera, and P. Stoffer, Phys. Lett. B 735, 90 (2014).
- T. Aoyama et al., Phys. Rep. 887, 1 (2020).
- T. Kinoshita and W. J. Marciano, Adv. Ser. Dir. High Energy Phys. 7, 419 (1990).
- Y.-F. Zhou and Y.-L. Wu, Eur. Phys. J. C 27, 577 (2003).
- V. Barger, C.-W. Chiang, W.-Y. Keung, and D. Marfatia, Phys. Rev. Lett. 106, 153001 (2011).
- D. Tucker-Smith and I. Yavin, Phys. Rev. D 83, 101702 (2011).
- C.-Y. Chen, H. Davoudiasl, W. J. Marciano, and C. Zhang, Phys. Rev. D 93, 035006 (2016).
- B. Batell, N. Lange, D. McKeen, M. Pospelov, and A. Ritz, Phys. Rev. D 95, 075003 (2017).
- J. Liu, C. E. M. Wagner, and X.-P. Wang, J. High Energy Phys. 03 (2019) 008.
- A. Caputo, G. Raffelt, and E. Vitagliano, arXiv:2109.03244 [Phys. Rev. D (to be published)].
- R. Delbourgo and D.-s. Liu, Aust. J. Phys. 53, 647 (2000).
- J. S. Lee, arXiv:1808.10136.
- N. Bar, K. Blum, and G. D’Amico, Phys. Rev. D 101, 123025 (2020).
- G. Lucente, P. Carenza, T. Fischer, M. Giannotti, and A. Mirizzi, J. Cosmol. Astropart. Phys. 12 (2020) 008.
- J. P. Lees et al. (BABAR Collaboration), Phys. Rev. Lett. 125, 181801 (2020).
- M. Campajola (Belle-II Collaboration), Phys. Scr. 96, 084005 (2021).
- C. Boehm, M. J. Dolan, and C. McCabe, J. Cosmol. Astropart. Phys. 08 (2013) 041.
- G. B. Gelmini and M. Roncadelli, Phys. Lett. 99B, 411 (1981).
- N. Blinov, K. J. Kelly, G. Z. Krnjaic, and S. D. McDermott, Phys. Rev. Lett. 123, 191102 (2019).
- A. De Gouvêa, M. Sen, W. Tangarife, and Y. Zhang, Phys. Rev. Lett. 124, 081802 (2020).
- K.-F. Lyu, E. Stamou, and L.-T. Wang, Phys. Rev. D 103, 015004 (2021).
- K. J. Kelly, M. Sen, and Y. Zhang, Phys. Rev. Lett. 127, 041101 (2021).
- E. W. Kolb, M. S. Turner, and T. P. Walker, Phys. Rev. D 34, 2197 (1986).
- M. Srednicki, R. Watkins, and K. A. Olive, Nucl. Phys. B310, 693 (1988).
- C. Boehm, M. J. Dolan, and C. McCabe, J. Cosmol. Astropart. Phys. 12 (2012) 027.
- N. Aghanim et al. (Planck Collaboration), Astron. Astrophys. 641, A6 (2020); 652, C4(E) (2021).
- See Supplemental Material at http://link.aps.org/supplemental/10.1103/PhysRevD.105.L051702 for diagonalization procedure for the active and sterile neutrino mass matrix.