Built on

D. Fixsen, “The temperature of the cosmic microwave background,” Astrophys. J. 707
Original
1955
Earlier work this paper cites.
R.D. Peccei and H.R. Quinn, “CP conservation in the presence of pseudoparticles,” Phys. Rev. Lett. 38
1977
Earlier work this paper cites.
S. Weinberg, “A new light boson?,” Phys. Rev. Lett. 40
1978
Earlier work this paper cites.
P. di Vecchia and G. Veneziano, “ Chiral dynamics in the large N N limit,” Nuclear Physics B 171
1980
Earlier work this paper cites.
D. J. Gross, R. D. Pisarski and L. G. Yaffe, “QCD and instantons at finite temperature,” Rev. Mod. Phys. 53
1981
Earlier work this paper cites.
J. Preskill, M.B. Wise and F. Wilczek, “Cosmology of the invisible axion,” Phys. Lett. B 120
1983
Earlier work this paper cites.
M.S. Turner, “Cosmic and local mass density of ‘invisible’ axions,” Phys. Rev. D 33
1986
Earlier work this paper cites.
C. J. Hogan and M. J. Rees “Axion Miniclusters,” Phys. Lett. B 205
Original
1988
Earlier work this paper cites.
D.H. Lyth, “Axions and inflation: Vacuum fluctuations,” Phys. Rev. D 45
1992
Earlier work this paper cites.
E. Kolb and M. Turner, The Early Universe,
1994
Earlier work this paper cites.
K. Strobl and T.J. Weiler, “Anharmonic evolution of the cosmic axion density spectrum,” Phys. Rev. D 50
1994
Earlier work this paper cites.
J. Frieman, C. Hill, A. Stebbins and I. Waga, “Cosmology with ultra-light pseudo-Nambu-Goldstone bosons,” Phys. Rev. Lett. 75
1995
Earlier work this paper cites.
M.E. Peskin and D.V. Schroeder, An Introduction to Quantum Field Theory,
1995
Earlier work this paper cites.
S. Kachru, R. Kallosh, A. Linde and S.P. Trivedi, “de Sitter vacua in string theory,” Phys. Rev. D 86
2003
Earlier work this paper cites.
K. Sigurdson and A. Cooray, “Cosmic 21-cm delensing of microwave background polarization and the minimum detectable energy scale of inflation,” Phys. Rev. Lett. 95
2005
Earlier work this paper cites.
P. Sikivie, “Axion Cosmology,” Lect. Notes Phys. 741
2008
Earlier work this paper cites.
M.P Hertzberg, M. Tegmark and F. Wilczek, “Axion cosmology and the energy scale of inflation,” Phys. Rev. D 78
2008
Earlier work this paper cites.
G.G. Raffelt, “Astrophysical axion bounds,” Lect. Notes Phys. 741
2008
Earlier work this paper cites.
K.J. Bae, J.H. Huh and J.E. Kim, “Update of axion CDM energy density,” JCAP 0809
Original
2008
Earlier work this paper cites.

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Later among the works it cites.
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Original
2016
Later among the works it cites.
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Original

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2017

Cosmological production of ultralight dark matter axions

Diez-Tejedor, Alberto, Marsh, David J. E.

Understand

The highly populated, low-energy excitations of a scalar field of mass $m_a\sim 10^{-22}\,\textrm{eV}$ can represent the full dark matter content of the universe and alleviate some tensions in the standard cosmological scenario on small-scales.

This {\it fuzzy dark matter} component is commonly assumed to arise as the consequence of a new axion-like particle in the matter sector, yet for simplicity it is usually modeled in terms of a simple free quadratic field.
In this paper we consider how the cosmological constraints are modified when the effects of an instanton potential and temperature-dependent mass are included.
Current isocurvature and tensor bounds confirms that this particle should be formed before the end of a low-scale inflation period with Hubble parameter $H_I\lesssim 2.5\times 10^{12}\,\textrm{GeV}$, in accordance with previous free-field analysis.

Built on

D. Fixsen, “The temperature of the cosmic microwave background,” Astrophys. J. 707
Original
1955
Earlier work this paper cites.
R.D. Peccei and H.R. Quinn, “CP conservation in the presence of pseudoparticles,” Phys. Rev. Lett. 38
1977
Earlier work this paper cites.
S. Weinberg, “A new light boson?,” Phys. Rev. Lett. 40
1978
Earlier work this paper cites.
P. di Vecchia and G. Veneziano, “ Chiral dynamics in the large N N limit,” Nuclear Physics B 171
1980
Earlier work this paper cites.
D. J. Gross, R. D. Pisarski and L. G. Yaffe, “QCD and instantons at finite temperature,” Rev. Mod. Phys. 53
1981
Earlier work this paper cites.
J. Preskill, M.B. Wise and F. Wilczek, “Cosmology of the invisible axion,” Phys. Lett. B 120
1983
Earlier work this paper cites.
M.S. Turner, “Cosmic and local mass density of ‘invisible’ axions,” Phys. Rev. D 33
1986
Earlier work this paper cites.
C. J. Hogan and M. J. Rees “Axion Miniclusters,” Phys. Lett. B 205
Original
1988
Earlier work this paper cites.
D.H. Lyth, “Axions and inflation: Vacuum fluctuations,” Phys. Rev. D 45
1992
Earlier work this paper cites.
E. Kolb and M. Turner, The Early Universe,
1994
Earlier work this paper cites.
K. Strobl and T.J. Weiler, “Anharmonic evolution of the cosmic axion density spectrum,” Phys. Rev. D 50
1994
Earlier work this paper cites.
J. Frieman, C. Hill, A. Stebbins and I. Waga, “Cosmology with ultra-light pseudo-Nambu-Goldstone bosons,” Phys. Rev. Lett. 75
1995
Earlier work this paper cites.
M.E. Peskin and D.V. Schroeder, An Introduction to Quantum Field Theory,
1995
Earlier work this paper cites.
S. Kachru, R. Kallosh, A. Linde and S.P. Trivedi, “de Sitter vacua in string theory,” Phys. Rev. D 86
2003
Earlier work this paper cites.
K. Sigurdson and A. Cooray, “Cosmic 21-cm delensing of microwave background polarization and the minimum detectable energy scale of inflation,” Phys. Rev. Lett. 95
2005
Earlier work this paper cites.
P. Sikivie, “Axion Cosmology,” Lect. Notes Phys. 741
2008
Earlier work this paper cites.
M.P Hertzberg, M. Tegmark and F. Wilczek, “Axion cosmology and the energy scale of inflation,” Phys. Rev. D 78
2008
Earlier work this paper cites.
G.G. Raffelt, “Astrophysical axion bounds,” Lect. Notes Phys. 741
2008
Earlier work this paper cites.
K.J. Bae, J.H. Huh and J.E. Kim, “Update of axion CDM energy density,” JCAP 0809
Original
2008
Earlier work this paper cites.