Built on

D.J. Kaup, Klein-Gordon geon, Phys. Rev. 172
1968
Earlier work this paper cites.
R. Ruffini and S. Bonazzola, Systems of self-gravitating particles in general relativity and the concept of an equation of state, Phys. Rev. 187
1969
Earlier work this paper cites.
J. Katz, On the number of unstable modes of an equilibrium, Mon. Not. R. Astr. Soc. 183
1978
Earlier work this paper cites.
J.D. Breit, S. Gupta and A. Zaks, Cold Bose stars, Phys. Lett. B 140
1984
Earlier work this paper cites.
C.J. Hogan and M.J. Rees, Axion miniclusters, Phys. Lett. B 205
1988
Earlier work this paper cites.
I.I. Tkachev, On the possibility of Bose star formation, Phys. Lett. B 261
1991
Earlier work this paper cites.
E.W. Kolb and I.I. Tkachev, Axion miniclusters and Bose stars, Phys. Rev. Lett. 71
1993
Earlier work this paper cites.

Similar

G. Baym and C.J. Pethick, Ground-state properties of magnetically trapped Bose-condensed rubidium gas, Phys. Rev. Lett. 76
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2009
Cited alongside, same era.
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Then

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Original
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2013
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J. Eby, P. Suranyi, C. Vaz and L.C.R. Wijewardhana, Axion stars in the infrared limit, JHEP 1503
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2015
Closest in time.
A.H. Guth, M.P. Hertzberg and C. Prescod-Weinstein, Do dark matter axions form a condensate with long-range correlation?, Phys. Rev. D 92

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2015

Dense Axion Stars

Braaten, Eric, Mohapatra, Abhishek, Zhang, Hong

Understand

If the dark matter particles are axions, gravity can cause them to coalesce into axion stars, which are stable gravitationally bound systems of axions.

In the previously known solutions for axion stars, gravity and the attractive force between pairs of axions are balanced by the kinetic pressure.
The mass of these dilute axion stars cannot exceed a critical mass, which is about $10^{-14} M_\odot$ if the axion mass is $10^{-4}$~eV.
We study axion stars using a simple approximation to the effective potential of the nonrelativistic effective field theory for axions.

Built on

D.J. Kaup, Klein-Gordon geon, Phys. Rev. 172
1968
Earlier work this paper cites.
R. Ruffini and S. Bonazzola, Systems of self-gravitating particles in general relativity and the concept of an equation of state, Phys. Rev. 187
1969
Earlier work this paper cites.
J. Katz, On the number of unstable modes of an equilibrium, Mon. Not. R. Astr. Soc. 183
1978
Earlier work this paper cites.
J.D. Breit, S. Gupta and A. Zaks, Cold Bose stars, Phys. Lett. B 140
1984
Earlier work this paper cites.
C.J. Hogan and M.J. Rees, Axion miniclusters, Phys. Lett. B 205
1988
Earlier work this paper cites.
I.I. Tkachev, On the possibility of Bose star formation, Phys. Lett. B 261
1991
Earlier work this paper cites.
E.W. Kolb and I.I. Tkachev, Axion miniclusters and Bose stars, Phys. Rev. Lett. 71
1993
Earlier work this paper cites.

Similar

G. Baym and C.J. Pethick, Ground-state properties of magnetically trapped Bose-condensed rubidium gas, Phys. Rev. Lett. 76
1996
Cited alongside, same era.
E.A. Donley, N.R. Claussen, S.L. Cornish, J.L. Roberts, E.A. Cornell, and C.E. Wieman, Dynamics of collapsing and exploding Bose-Einstein condensates, Nature 412
2001
Cited alongside, same era.
X.Z. Wang, Cold Bose stars: self-gravitating Bose-Einstein condensates, Phys. Rev. D 64
2001
Cited alongside, same era.
P. Tisserand et al
2007
Cited alongside, same era.
P. Sikivie and Q. Yang, Bose-Einstein condensation of dark matter axions, Phys. Rev. Lett. 103
Original
2009
Cited alongside, same era.
J. E. Kim and G. Carosi, Axions and the strong CP problem, Rev. Mod. Phys. 82