Reuse & Permissions

It is not necessary to obtain permission to reuse this article or its components as it is available under the terms of the Creative Commons Attribution 4.0 International license. This license permits unrestricted use, distribution, and reproduction in any medium, provided attribution to the author(s) and the published article's title, journal citation, and DOI are maintained. Please note that some figures may have been included with permission from other third parties. It is your responsibility to obtain the proper permission from the rights holder directly for these figures.

Export citation

Export citation

Choose format for download:

Download Citation
  • Open Access
  • Access by Xinjiang University

Making the Universe at 20 MeV

Gilly Elor1,* and Robert McGehee2,3,4,†

  • 1Department of Physics, University of Washington, Seattle, Washington 98195, USA
  • 2Leinweber Center for Theoretical Physics, Department of Physics, University of Michigan, Ann Arbor, Michigan 48109, USA
  • 3Berkeley Center for Theoretical Physics, University of California, Berkeley, California 94720, USA
  • 4Theory Group, Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA

  • *gelor@uw.edu
  • rmcgehee@umich.edu

Phys. Rev. D 103, 035005 – Published 5 February, 2021

DOI: https://doi.org/10.1103/PhysRevD.103.035005

Abstract

We present a testable mechanism of low-scale baryogenesis and dark matter production in which neither the baryon nor lepton number are violated. Charged D mesons are produced out of equilibrium at tens of MeV temperatures. The D mesons quickly undergo CP-violating decays to charged pions, which then decay into dark-sector leptons without violating the lepton number. To transfer this lepton asymmetry to the baryon asymmetry, the dark leptons scatter on additional dark-sector states charged under the lepton and baryon number. Amusingly, this transfer proceeds without electroweak sphalerons, which are no longer active at such low scales. We present two example models which can achieve this transfer while remaining consistent with current limits. The required amount of CP violation in charged D meson decays, while currently allowed, will be probed by colliders. Additionally, the relevant decays of charged pions to dark-sector leptons have been constrained by the PIENU and Paul Scherrer Institute experiments and will be further explored in upcoming experiments.

View figure in article

Physics Subject Headings (PhySH)

Article Text

References (75)

  1. P. A. R. Ade et al. (Planck Collaboration), Planck 2015 results. XIII. Cosmological parameters, Astron. Astrophys. 594, A13 (2016).
  2. N. Aghanim et al. (Planck Collaboration), Planck 2018 results. VI. Cosmological parameters, Astron. Astrophys. 641, A6 (2020).
  3. R. H. Cyburt, B. D. Fields, K. A. Olive, and T.-H. Yeh, Big bang nucleosynthesis: 2015, Rev. Mod. Phys. 88, 015004 (2016).
  4. M. Tanabashi et al. (Particle Data Group), Review of particle physics, Phys. Rev. D 98, 030001 (2018).
  5. A. D. Sakharov, Violation of CP invariance, c asymmetry, and baryon asymmetry of the universe, Pis’ma Zh. Eksp. Teor. Fiz. 5, 32 (1967) [Usp. Fiz. Nauk 161, 61 (1991)].
  6. V. A. Kuzmin, V. A. Rubakov, and M. E. Shaposhnikov, On the anomalous electroweak baryon number nonconservation in the early universe, Phys. Lett. 155B, 36 (1985).
  7. A. G. Cohen, D. B. Kaplan, and A. E. Nelson, Weak scale baryogenesis, Phys. Lett. B 245, 561 (1990).
  8. A. G. Cohen, D. B. Kaplan, and A. E. Nelson, Baryogenesis at the weak phase transition, Nucl. Phys. B349, 727 (1991).
  9. N. Turok and J. Zadrozny, Dynamical Generation of Baryons at the Electroweak Transition, Phys. Rev. Lett. 65, 2331 (1990).
  10. N. Turok and J. Zadrozny, Electroweak baryogenesis in the two doublet model, Nucl. Phys. B358, 471 (1991).
  11. L. D. McLerran, M. E. Shaposhnikov, N. Turok, and M. B. Voloshin, Why the baryon asymmetry of the universe is 1010, Phys. Lett. B 256, 477 (1991).
  12. M. Dine, P. Huet, R. L. Singleton, Jr., and L. Susskind, Creating the baryon asymmetry at the electroweak phase transition, Phys. Lett. B 257, 351 (1991).
  13. A. G. Cohen, D. B. Kaplan, and A. E. Nelson, Spontaneous baryogenesis at the weak phase transition, Phys. Lett. B 263, 86 (1991).
  14. A. E. Nelson, D. B. Kaplan, and A. G. Cohen, Why there is something rather than nothing: Matter from weak interactions, Nucl. Phys. B373, 453 (1992).
  15. A. G. Cohen, D. B. Kaplan, and A. E. Nelson, Debye screening and baryogenesis during the electroweak phase transition, Phys. Lett. B 294, 57 (1992).
  16. G. R. Farrar and M. E. Shaposhnikov, Baryon asymmetry of the universe in the standard electroweak theory, Phys. Rev. D 50, 774 (1994).
  17. M. Fukugita and T. Yanagida, Baryogenesis without grand unification, Phys. Lett. B 174, 45 (1986).
  18. V. Andreev et al. (ACME Collaboration), Improved limit on the electric dipole moment of the electron, Nature (London) 562, 355 (2018).
  19. J. A. Dror, T. Hiramatsu, K. Kohri, H. Murayama, and G. White, Testing the Seesaw Mechanism and Leptogenesis with Gravitational Waves, Phys. Rev. Lett. 124, 041804 (2020).
  20. P. Hernández, M. Kekic, J. López-Pavón, J. Racker, and J. Salvado, Testable baryogenesis in Seesaw models, J. High Energy Phys. 08 (2016) 157.
  21. C. Cheung, G. Elor, L. J. Hall, and P. Kumar, Origins of hidden sector dark matter I: Cosmology, J. High Energy Phys. 03 (2011) 042.
  22. X. Chu, T. Hambye, and M. H. Tytgat, The four basic ways of creating dark matter through a portal, J. Cosmol. Astropart. Phys. 05 (2012) 034.
  23. Y. Hochberg, E. Kuflik, T. Volansky, and J. G. Wacker, Mechanism for Thermal Relic Dark Matter of Strongly Interacting Massive Particles, Phys. Rev. Lett. 113, 171301 (2014).
  24. G. Elor, H. Liu, T. R. Slatyer, and Y. Soreq, Complementarity for dark sector bound states, Phys. Rev. D 98, 036015 (2018).
  25. Y. Tsai, L.-T. Wang, and Y. Zhao, Dark matter annihilation decay at the LHC, Phys. Rev. D 93, 035024 (2016).
  26. C. Cheung, G. Elor, L. J. Hall, and P. Kumar, Origins of hidden sector dark matter II: Collider physics, J. High Energy Phys. 03 (2011) 085.
  27. J. A. Dror, G. Elor, and R. McGehee, Directly Detecting Signals from Absorption of Fermionic Dark Matter, Phys. Rev. Lett. 124, 18 (2020).
  28. J. A. Dror, G. Elor, and R. McGehee, Absorption of fermionic dark matter by nuclear targets, J. High Energy Phys. 02 (2020) 134.
  29. J. A. Dror, G. Elor, R. McGehee, and T.-T. Yu, Absorption of sub-MeV fermionic dark matter by electron targets, arXiv:2011.01940 [Phys. Rev. D (to be published)].
  30. R. Essig, M. Fernandez-Serra, J. Mardon, A. Soto, T. Volansky, and T.-T. Yu, Direct detection of sub-GeV dark matter with semiconductor targets, J. High Energy Phys. 05 (2016) 046.
  31. G. Krnjaic, Freezing in, heating up, and freezing out: Predictive nonthermal dark matter and low-mass direct detection, J. High Energy Phys. 10 (2018) 136.
  32. M. Geller and O. Telem, Self destructing atomic DM, arXiv:2001.11514.
  33. D. Hooper, R. K. Leane, Y.-D. Tsai, S. Wegsman, and S. J. Witte, A systematic study of hidden sector dark matter: Application to the gamma-ray and antiproton excesses, J. High Energy Phys. 07 (2020) 163.
  34. G. Elor, N. L. Rodd, T. R. Slatyer, and W. Xue, Model-independent indirect detection constraints on hidden sector dark matter, J. Cosmol. Astropart. Phys. 06 (2016) 024.
  35. P. Barnes, Z. Johnson, A. Pierce, and B. Shakya, Simple hidden sector dark matter, Phys. Rev. D 102, 075019 (2020).
  36. H. Davoudiasl and R. N. Mohapatra, On relating the genesis of cosmic baryons and dark matter, New J. Phys. 14, 095011 (2012).
  37. K. Petraki and R. R. Volkas, Review of asymmetric dark matter, Int. J. Mod. Phys. A 28, 1330028 (2013).
  38. K. M. Zurek, Asymmetric dark matter: Theories, signatures, and constraints, Phys. Rep. 537, 91 (2014).
  39. H. Davoudiasl, D. E. Morrissey, K. Sigurdson, and S. Tulin, Hylogenesis: A Unified Origin for Baryonic Visible Matter and Antibaryonic Dark Matter, Phys. Rev. Lett. 105, 211304 (2010).
  40. E. Hall, T. Konstandin, R. McGehee, and H. Murayama, Asymmetric matters from a dark first-order phase transition, arXiv:1911.12342.
  41. J. Shelton and K. M. Zurek, Darkogenesis: A baryon asymmetry from the dark matter sector, Phys. Rev. D 82, 123512 (2010).
  42. G. Servant and S. Tulin, Baryogenesis and Dark Matter Through a Higgs Asymmetry, Phys. Rev. Lett. 111, 151601 (2013).
  43. E. Hall, T. Konstandin, R. McGehee, H. Murayama, and G. Servant, Baryogenesis from a dark first-order phase transition, J. High Energy Phys. 04 (2020) 042.
  44. E. W. Kolb and M. S. Turner, The early Universe, Front. Phys. 69, 1 (1990).
  45. S. Dimopoulos and L. J. Hall, Baryogenesis at the {MeV} Era, Phys. Lett. B 196, 135 (1987).
  46. T. Cohen, D. J. Phalen, and A. Pierce, Supersymmetric baryogenesis from exotic quark decays, Phys. Rev. D 81, 035020 (2010).
  47. N. Arkani-Hamed, T. Cohen, R. T. D’Agnolo, A. Hook, H. D. Kim, and D. Pinner, Solving the Hierarchy Problem at Reheating with a Large Number of Degrees of Freedom, Phys. Rev. Lett. 117, 251801 (2016).
  48. P. W. Graham, D. E. Kaplan, and S. Rajendran, Cosmological Relaxation of the Electroweak Scale, Phys. Rev. Lett. 115, 221801 (2015).
  49. G. Elor, M. Escudero, and A. Nelson, Baryogenesis and dark matter from B mesons, Phys. Rev. D 99, 035031 (2019).
  50. G. Alonso-Álvarez, G. Elor, A. E. Nelson, and H. Xiao, A supersymmetric theory of baryogenesis and sterile sneutrino dark matter from B mesons, J. High Energy Phys. 03 (2020) 046.
  51. G. Alonso-Álvarez, G. Elor, and M. Escudero, Collider signals of baryogenesis and dark matter from B mesons: A roadmap to discovery, arXiv:2101.02706.
  52. T. Hasegawa, N. Hiroshima, K. Kohri, R. S. Hansen, T. Tram, and S. Hannestad, MeV-scale reheating temperature and thermalization of oscillating neutrinos by radiative and hadronic decays of massive particles, J. Cosmol. Astropart. Phys. 12 (2019) 012.
  53. M. Kawasaki, K. Kohri, and N. Sugiyama, Cosmological Constraints on Late Time Entropy Production, Phys. Rev. Lett. 82, 4168 (1999).
  54. M. Kawasaki, K. Kohri, and N. Sugiyama, MeV scale reheating temperature and thermalization of neutrino background, Phys. Rev. D 62, 023506 (2000).
  55. A. Ibarra and S. Wild, Dirac dark matter with a charged mediator: A comprehensive one-loop analysis of the direct detection phenomenology, J. Cosmol. Astropart. Phys. 05 (2015) 047.
  56. A. Aguilar-Arevalo et al. (PIENU Collaboration), Improved search for heavy neutrinos in the decay πeν, Phys. Rev. D 97, 072012 (2018).
  57. D. Bryman and R. Shrock, Constraints on sterile neutrinos in the MeV to GeV mass range, Phys. Rev. D 100, 073011 (2019).
  58. R. Abela, M. Daum, G. Eaton, R. Frosch, B. Jost, P. Kettle, and E. Steiner, Search for an admixture of heavy neutrino in pion decay, Phys. Lett. 105B, 263 (1981); Erratum, 106B, 513 (1981).
  59. A. Aguilar-Arevalo et al. (PIENU Collaboration), Search for heavy neutrinos in πμν decay, Phys. Lett. B 798, 134980 (2019).
  60. D. Bryman (private communication).
  61. D. McKeen, A. E. Nelson, S. Reddy, and D. Zhou, Neutron Stars Exclude Light Dark Baryons, Phys. Rev. Lett. 121, 061802 (2018).
  62. K. Harigaya, R. McGehee, H. Murayama, and K. Schutz, A predictive mirror twin Higgs with small Z2 breaking, J. High Energy Phys. 05 (2020) 155.
  63. Y.-D. Tsai, R. McGehee, and H. Murayama, Resonant self-interacting dark matter from dark QCD, arXiv:2008.08608.
  64. S. Dobbs et al. (CLEO Collaboration), Measurement of absolute hadronic branching fractions of D mesons and e+e> D anti-D cross-sections at the psi(3770), Phys. Rev. D 76, 112001 (2007).
  65. A. V. Artamonov et al. (E949 Collaboration), Search for heavy neutrinos in K+μ+νH decays, Phys. Rev. D 91, 052001 (2015); Erratum, 91, 059903 (2015).
  66. E. Cortina Gil et al. (NA62 Collaboration), Search for heavy neutral lepton production in K+ decays, Phys. Lett. B 778, 137 (2018).
  67. R. Aaij et al. (LHCb Collaboration), Updated determination of D0D¯0 mixing and CP violation parameters with D0K+π decays, Phys. Rev. D 97, 031101 (2018).
  68. Y. Nir, Lessons from BABAR and Belle measurements of D0—anti-D0 mixing parameters, J. High Energy Phys. 05 (2007) 102.
  69. E. Golowich, J. Hewett, S. Pakvasa, and A. A. Petrov, Implications of D0D¯0 mixing for new physics, Phys. Rev. D 76, 095009 (2007).
  70. G. Barenboim, W. H. Kinney, and W.-I. Park, Flavor versus mass eigenstates in neutrino asymmetries: Implications for cosmology, Eur. Phys. J. C 77, 590 (2017).
  71. T. Venumadhav, F.-Y. Cyr-Racine, K. N. Abazajian, and C. M. Hirata, Sterile neutrino dark matter: Weak interactions in the strong coupling epoch, Phys. Rev. D 94, 043515 (2016).
  72. R. J. Scherrer and M. S. Turner, Primordial nucleosynthesis with decaying particles. 1. Entropy producing decays. 2. Inert decays, Astrophys. J. 331, 19 (1988).
  73. S. Hannestad, What is the lowest possible reheating temperature?, Phys. Rev. D 70, 043506 (2004).
  74. M. Laine and Y. Schroder, Quark mass thresholds in QCD thermodynamics, Phys. Rev. D 73, 085009 (2006).
  75. P. Zyla et al. (Particle Data Group), Review of particle physics, Prog. Theor. Exp. Phys. 2020, 083C01 (2020).

Outline

Information

Sign In to Your Journals Account

Filter

Filter

Article Lookup

Enter a citation