Built on

S. Gandolfi, J. Carlson and S. Reddy, “The maximum mass and radius of neutron stars and the nuclear symmetry energy,” Phys. Rev. C 85
Original
1921
Earlier work this paper cites.
L. Dolan and R. Jackiw, “Symmetry Behavior at Finite Temperature,” Phys. Rev. D 9
1974
Earlier work this paper cites.
D. Notzold and G. Raffelt, “Neutrino Dispersion at Finite Temperature and Density,” Nucl. Phys. B 307
1988
Earlier work this paper cites.
J. D. Bjorken et al
1988
Earlier work this paper cites.
M. Davier and H. Nguyen Ngoc, “An Unambiguous Search for a Light Higgs Boson,” Phys. Lett. B 229
1989
Earlier work this paper cites.
S. M. Barr, R. S. Chivukula and E. Farhi, “Electroweak Fermion Number Violation and the Production of Stable Particles in the Early Universe,” Phys. Lett. B 241
1990
Earlier work this paper cites.
H. Leutwyler and A. V. Smilga, “Nucleons At Finite Temperature,” Nucl. Phys. B 342
1990
Earlier work this paper cites.
J. A. Harvey and M. S. Turner, “Cosmological baryon and lepton number in the presence of electroweak fermion number violation,” Phys. Rev. D 42
1990
Earlier work this paper cites.
S. M. Barr, “Baryogenesis, sphalerons and the cogeneration of dark matter,” Phys. Rev. D 44
1991
Earlier work this paper cites.
D. B. Kaplan, “A Single explanation for both the baryon and dark matter densities,” Phys. Rev. Lett. 68
1992
Earlier work this paper cites.
J. M. Cline, “Constraints on almost Dirac neutrinos from neutrino - anti-neutrino oscillations,” Phys. Rev. Lett. 68
1992
Earlier work this paper cites.
C. A. Dominguez and M. Loewe, “Nucleon propagator at finite temperature,” Z. Phys. C 58
1993
Earlier work this paper cites.
P. F. Bedaque, “Chiral perturbation theory analysis of baryon temperature mass shifts,” Phys. Lett. B 387
1996
Earlier work this paper cites.
M. Kacir and I. Zahed, “Nucleons at finite temperature,” Phys. Rev. D 54
1996
Earlier work this paper cites.
J. Shelton and K. M. Zurek, “Darkogenesis: A baryon asymmetry from the dark matter sector,” Phys. Rev. D 82
Original
1997
Earlier work this paper cites.
V. L. Eletsky and B. L. Ioffe, “On the thermal mass shift of nucleons,” Phys. Lett. B 401
1997
Earlier work this paper cites.
N. Fettes, U. G. Meissner and S. Steininger, “Pion - nucleon scattering in chiral perturbation theory. 1. Isospin symmetric case,” Nucl. Phys. A 640
1998
Earlier work this paper cites.
D. N. Spergel and P. J. Steinhardt, “Observational evidence for self-interacting cold dark matter,” Phys. Rev. Lett. 84
2000
Earlier work this paper cites.
R. Foot and R. R. Volkas, “Was ordinary matter synthesized from mirror matter? An Attempt to explain why Omega(Baryon) approximately equal to 0.2 Omega(Dark),” Phys. Rev. D 68
2003
Earlier work this paper cites.
D. Hooper, J. March-Russell and S. M. West, “Asymmetric sneutrino dark matter and the Omega(b) / Omega(DM) puzzle,” Phys. Lett. B 605
2004
Earlier work this paper cites.
Z. Berezhiani and L. Bento, “Neutron - mirror neutron oscillations: How fast might they be?,” Phys. Rev. Lett. 96
2006
Earlier work this paper cites.
Z. Berezhiani and L. Bento, “Fast neutron: Mirror neutron oscillation and ultra high energy cosmic rays,” Phys. Lett. B 635
2006
Earlier work this paper cites.
S. B. Gudnason, C. Kouvaris and F. Sannino, “Dark Matter from new Technicolor Theories,” Phys. Rev. D 74
2006
Earlier work this paper cites.
S. W. Randall, M. Markevitch, D. Clowe, A. H. Gonzalez and M. Bradac, “Constraints on the Self-Interaction Cross-Section of Dark Matter from Numerical Simulations of the Merging Galaxy Cluster 1E 0657-56,” Astrophys. J. 679
Original
2008
Earlier work this paper cites.

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2018

Baryogenesis from neutron-dark matter oscillations

Bringmann, Torsten, Cline, James M., Cornell, Jonathan M.

Understand

It was recently suggested that dark matter consists of ~GeV particles that carry baryon number and mix with the neutron.

We demonstrate that this could allow for resonant dark matter-neutron oscillations in the early universe, at finite temperature, leading to low-scale baryogenesis starting from a primordial dark matter asymmetry.
In this scenario, the asymmetry transfer happens around 30 MeV, just before big bang nucleosynthesis.
We illustrate the idea using a model with a dark U(1)' gauge interaction, which has recently been suggested as a way of addressing the neutron lifetime anomaly.

Built on

S. Gandolfi, J. Carlson and S. Reddy, “The maximum mass and radius of neutron stars and the nuclear symmetry energy,” Phys. Rev. C 85
Original
1921
Earlier work this paper cites.
L. Dolan and R. Jackiw, “Symmetry Behavior at Finite Temperature,” Phys. Rev. D 9
1974
Earlier work this paper cites.
D. Notzold and G. Raffelt, “Neutrino Dispersion at Finite Temperature and Density,” Nucl. Phys. B 307
1988
Earlier work this paper cites.
J. D. Bjorken et al
1988
Earlier work this paper cites.
M. Davier and H. Nguyen Ngoc, “An Unambiguous Search for a Light Higgs Boson,” Phys. Lett. B 229
1989
Earlier work this paper cites.
S. M. Barr, R. S. Chivukula and E. Farhi, “Electroweak Fermion Number Violation and the Production of Stable Particles in the Early Universe,” Phys. Lett. B 241
1990
Earlier work this paper cites.
H. Leutwyler and A. V. Smilga, “Nucleons At Finite Temperature,” Nucl. Phys. B 342
1990
Earlier work this paper cites.
J. A. Harvey and M. S. Turner, “Cosmological baryon and lepton number in the presence of electroweak fermion number violation,” Phys. Rev. D 42
1990
Earlier work this paper cites.
S. M. Barr, “Baryogenesis, sphalerons and the cogeneration of dark matter,” Phys. Rev. D 44
1991
Earlier work this paper cites.
D. B. Kaplan, “A Single explanation for both the baryon and dark matter densities,” Phys. Rev. Lett. 68
1992
Earlier work this paper cites.
J. M. Cline, “Constraints on almost Dirac neutrinos from neutrino - anti-neutrino oscillations,” Phys. Rev. Lett. 68
1992
Earlier work this paper cites.
C. A. Dominguez and M. Loewe, “Nucleon propagator at finite temperature,” Z. Phys. C 58
1993
Earlier work this paper cites.
P. F. Bedaque, “Chiral perturbation theory analysis of baryon temperature mass shifts,” Phys. Lett. B 387
1996
Earlier work this paper cites.
M. Kacir and I. Zahed, “Nucleons at finite temperature,” Phys. Rev. D 54
1996
Earlier work this paper cites.
J. Shelton and K. M. Zurek, “Darkogenesis: A baryon asymmetry from the dark matter sector,” Phys. Rev. D 82
Original
1997
Earlier work this paper cites.
V. L. Eletsky and B. L. Ioffe, “On the thermal mass shift of nucleons,” Phys. Lett. B 401
1997
Earlier work this paper cites.
N. Fettes, U. G. Meissner and S. Steininger, “Pion - nucleon scattering in chiral perturbation theory. 1. Isospin symmetric case,” Nucl. Phys. A 640
1998
Earlier work this paper cites.
D. N. Spergel and P. J. Steinhardt, “Observational evidence for self-interacting cold dark matter,” Phys. Rev. Lett. 84
2000
Earlier work this paper cites.
R. Foot and R. R. Volkas, “Was ordinary matter synthesized from mirror matter? An Attempt to explain why Omega(Baryon) approximately equal to 0.2 Omega(Dark),” Phys. Rev. D 68
2003
Earlier work this paper cites.
D. Hooper, J. March-Russell and S. M. West, “Asymmetric sneutrino dark matter and the Omega(b) / Omega(DM) puzzle,” Phys. Lett. B 605
2004
Earlier work this paper cites.
Z. Berezhiani and L. Bento, “Neutron - mirror neutron oscillations: How fast might they be?,” Phys. Rev. Lett. 96
2006
Earlier work this paper cites.
Z. Berezhiani and L. Bento, “Fast neutron: Mirror neutron oscillation and ultra high energy cosmic rays,” Phys. Lett. B 635
2006
Earlier work this paper cites.
S. B. Gudnason, C. Kouvaris and F. Sannino, “Dark Matter from new Technicolor Theories,” Phys. Rev. D 74
2006
Earlier work this paper cites.
S. W. Randall, M. Markevitch, D. Clowe, A. H. Gonzalez and M. Bradac, “Constraints on the Self-Interaction Cross-Section of Dark Matter from Numerical Simulations of the Merging Galaxy Cluster 1E 0657-56,” Astrophys. J. 679
Original
2008
Earlier work this paper cites.