Built on

T. Cookmeyer, J. Cookmeyer, D. Grin and T. L. Smith, “How sound are our ultralight axion approximations?,” Phys. Rev. D 101
Original
1909
Earlier work this paper cites.
W. H. Press and P. Schechter, “Formation of galaxies and clusters of galaxies by selfsimilar gravitational condensation,” Astrophys. J. 187
1974
Earlier work this paper cites.
J. R. Bond, G. Efstathiou and J. Silk, “Massive Neutrinos and the Large Scale Structure of the Universe,” Phys. Rev. Lett. 45
1980
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.
L. F. Abbott and P. Sikivie, “A Cosmological Bound on the Invisible Axion,” Phys. Lett. B 120
1983
Earlier work this paper cites.
M. Dine and W. Fischler, “The Not So Harmless Axion,” Phys. Lett. B 120
1983
Earlier work this paper cites.
C. P. Ma and E. Bertschinger, “Cosmological perturbation theory in the synchronous and conformal Newtonian gauges,” Astrophys. J. 455
1995
Earlier work this paper cites.
U. Seljak and M. Zaldarriaga, “A Line of sight integration approach to cosmic microwave background anisotropies,” Astrophys. J. 469
1996
Earlier work this paper cites.
J. F. Navarro, C. S. Frenk and S. D. M. White, “A Universal density profile from hierarchical clustering,” Astrophys. J. 490
1997
Earlier work this paper cites.
W. Hu, “Structure formation with generalized dark matter,” Astrophys. J. 506
1998
Earlier work this paper cites.
F. Perrotta and C. Baccigalupi, “Early time perturbations behavior in scalar field cosmologies,” Phys. Rev. D 59
1999
Earlier work this paper cites.
R. K. Sheth and G. Tormen, “Large scale bias and the peak background split,” Mon. Not. Roy. Astron. Soc. 308
1999
Earlier work this paper cites.
W. Hu, R. Barkana and A. Gruzinov, “Cold and fuzzy dark matter,” Phys. Rev. Lett. 85
2000
Earlier work this paper cites.
M. Bucher, K. Moodley and N. Turok, “The General primordial cosmic perturbation,” Phys. Rev. D 62
2000
Earlier work this paper cites.
K. Schutz, “Subhalo mass function and ultralight bosonic dark matter,” Phys. Rev. D 101
Original
2001
Earlier work this paper cites.
P. Bode, J. P. Ostriker and N. Turok, “Halo formation in warm dark matter models,” Astrophys. J. 556
2001
Earlier work this paper cites.
J. Eby, M. Leembruggen, L. Street, P. Suranyi and L. C. R. Wijewardhana, “Galactic Condensates composed of Multiple Axion Species,” JCAP 10
Original
2002
Earlier work this paper cites.
W. Hu, “Covariant linear perturbation formalism,” ICTP Lect. Notes Ser. 14
2003
Earlier work this paper cites.
M. Doran, “Speeding up cosmological Boltzmann codes,” JCAP 06
2005
Earlier work this paper cites.
L. Amendola and R. Barbieri, “Dark matter from an ultra-light pseudo-Goldsone-boson,” Phys. Lett. B 642
2006
Earlier work this paper cites.
K. K. Rogers and H. V. Peiris, “Strong Bound on Canonical Ultralight Axion Dark Matter from the Lyman-Alpha Forest,” Phys. Rev. Lett. 126
Original
2007
Earlier work this paper cites.
B. Schwabe, M. Gosenca, C. Behrens, J. C. Niemeyer and R. Easther, “Simulating mixed fuzzy and cold dark matter,” Phys. Rev. D 102
Original
2007
Earlier work this paper cites.
J. c. Hwang and H. Noh, “Axion as a Cold Dark Matter candidate,” Phys. Lett. B 680
Original
2009
Earlier work this paper cites.

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Then

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Later among the works it cites.
J. S. Bullock and M. Boylan-Kolchin, “Small-Scale Challenges to the Λ \Lambda CDM Paradigm,” Ann. Rev. Astron. Astrophys. 55
Original
2017
Later among the works it cites.
A. Fitts, M. Boylan-Kolchin, O. D. Elbert, J. S. Bullock, P. F. Hopkins, J. Onorbe, A. R. Wetzel, C. Wheeler, C. A. Faucher-Giguere and D. Keres, et al
Original
2017
Later among the works it cites.
R. Hložek, D. J. E. Marsh, D. Grin, R. Allison, J. Dunkley and E. Calabrese, “Future CMB tests of dark matter: Ultralight axions and massive neutrinos,” Phys. Rev. D 95
Original
2017
Later among the works it cites.
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2023

Implications of multi-axion dark matter on structure formation

Chen, Chong-Bin, Soda, Jiro

Understand

Axions are candidates for dark matter in the universe.We develop an accurate Boltzmann code to calculate the linear growth of the plasma.

As an interesting example, we investigate a mixed dark matter model consisting of cold dark matter (CDM) and two-axion dark matter.
We analyze the growth of the structure numerically and analytically.
We find that an effective single axion with an effective mass and an effective abundance is useful to characterize the two-axion cosmology.

Built on

T. Cookmeyer, J. Cookmeyer, D. Grin and T. L. Smith, “How sound are our ultralight axion approximations?,” Phys. Rev. D 101
Original
1909
Earlier work this paper cites.
W. H. Press and P. Schechter, “Formation of galaxies and clusters of galaxies by selfsimilar gravitational condensation,” Astrophys. J. 187
1974
Earlier work this paper cites.
J. R. Bond, G. Efstathiou and J. Silk, “Massive Neutrinos and the Large Scale Structure of the Universe,” Phys. Rev. Lett. 45
1980
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.
L. F. Abbott and P. Sikivie, “A Cosmological Bound on the Invisible Axion,” Phys. Lett. B 120
1983
Earlier work this paper cites.
M. Dine and W. Fischler, “The Not So Harmless Axion,” Phys. Lett. B 120
1983
Earlier work this paper cites.
C. P. Ma and E. Bertschinger, “Cosmological perturbation theory in the synchronous and conformal Newtonian gauges,” Astrophys. J. 455
1995
Earlier work this paper cites.
U. Seljak and M. Zaldarriaga, “A Line of sight integration approach to cosmic microwave background anisotropies,” Astrophys. J. 469
1996
Earlier work this paper cites.
J. F. Navarro, C. S. Frenk and S. D. M. White, “A Universal density profile from hierarchical clustering,” Astrophys. J. 490
1997
Earlier work this paper cites.
W. Hu, “Structure formation with generalized dark matter,” Astrophys. J. 506
1998
Earlier work this paper cites.
F. Perrotta and C. Baccigalupi, “Early time perturbations behavior in scalar field cosmologies,” Phys. Rev. D 59
1999
Earlier work this paper cites.
R. K. Sheth and G. Tormen, “Large scale bias and the peak background split,” Mon. Not. Roy. Astron. Soc. 308
1999
Earlier work this paper cites.
W. Hu, R. Barkana and A. Gruzinov, “Cold and fuzzy dark matter,” Phys. Rev. Lett. 85
2000
Earlier work this paper cites.
M. Bucher, K. Moodley and N. Turok, “The General primordial cosmic perturbation,” Phys. Rev. D 62
2000
Earlier work this paper cites.
K. Schutz, “Subhalo mass function and ultralight bosonic dark matter,” Phys. Rev. D 101
Original
2001
Earlier work this paper cites.
P. Bode, J. P. Ostriker and N. Turok, “Halo formation in warm dark matter models,” Astrophys. J. 556
2001
Earlier work this paper cites.
J. Eby, M. Leembruggen, L. Street, P. Suranyi and L. C. R. Wijewardhana, “Galactic Condensates composed of Multiple Axion Species,” JCAP 10
Original
2002
Earlier work this paper cites.
W. Hu, “Covariant linear perturbation formalism,” ICTP Lect. Notes Ser. 14
2003
Earlier work this paper cites.
M. Doran, “Speeding up cosmological Boltzmann codes,” JCAP 06
2005
Earlier work this paper cites.
L. Amendola and R. Barbieri, “Dark matter from an ultra-light pseudo-Goldsone-boson,” Phys. Lett. B 642
2006
Earlier work this paper cites.
K. K. Rogers and H. V. Peiris, “Strong Bound on Canonical Ultralight Axion Dark Matter from the Lyman-Alpha Forest,” Phys. Rev. Lett. 126
Original
2007
Earlier work this paper cites.
B. Schwabe, M. Gosenca, C. Behrens, J. C. Niemeyer and R. Easther, “Simulating mixed fuzzy and cold dark matter,” Phys. Rev. D 102
Original
2007
Earlier work this paper cites.
J. c. Hwang and H. Noh, “Axion as a Cold Dark Matter candidate,” Phys. Lett. B 680
Original
2009
Earlier work this paper cites.