Built on

B. Eggemeier and J. C. Niemeyer, Formation and mass growth of axion stars in axion miniclusters , Phys. Rev. D 100
Original
1906
Earlier work this paper cites.
L. Dai and J. Miralda-Escudé, Gravitational Lensing Signatures of Axion Dark Matter Minihalos in Highly Magnified Stars , Astron. J. 159
Original
1908
Earlier work this paper cites.
A. Kalaja, N. Bellomo, N. Bartolo, D. Bertacca, S. Matarrese, I. Musco et al., From Primordial Black Holes Abundance to Primordial Curvature Power Spectrum (and back) , JCAP 10
Original
1908
Earlier work this paper cites.
A. Arvanitaki, S. Dimopoulos, M. Galanis, L. Lehner, J. O. Thompson and K. Van Tilburg, Large-misalignment mechanism for the formation of compact axion structures: Signatures from the QCD axion to fuzzy dark matter , Phys. Rev. D 101
Original
1909
Earlier work this paper cites.
T. Patel, H. Tashiro and Y. Urakawa, Resonant magnetogenesis from axions , JCAP 2001
Original
1909
Earlier work this paper cites.
B. Eggemeier, J. Redondo, K. Dolag, J. C. Niemeyer and A. Vaquero, First simulations of axion minicluster halos , 1911.09417
Original
1911
Earlier work this paper cites.
N. Blinov, M. J. Dolan and P. Draper, Imprints of the Early Universe on Axion Dark Matter Substructure , Phys. Rev. D 101
Original
1911
Earlier work this paper cites.
J. C. Niemeyer, Small-scale structure of fuzzy and axion-like dark matter , 1912.07064
Original
1912
Earlier work this paper cites.
P. Meszaros, The behaviour of point masses in an expanding cosmological substratum. , Astronomy and Astrophysics 37
1974
Earlier work this paper cites.
R. D. Peccei and H. R. Quinn, CP Conservation in the Presence of Instantons , Phys. Rev. Lett. 38
1977
Earlier work this paper cites.
R. D. Peccei and H. R. Quinn, Constraints Imposed by CP Conservation in the Presence of Instantons , Phys. Rev. D16
1977
Earlier work this paper cites.
S. Weinberg, A New Light Boson? , Phys. Rev. Lett. 40
1978
Earlier work this paper cites.
F. Wilczek, Problem of Strong P P and T T Invariance in the Presence of Instantons , Phys. Rev. Lett. 40
1978
Earlier work this paper cites.
P. Di Vecchia and G. Veneziano, Chiral Dynamics in the Large n Limit , Nucl. Phys. B171
1980
Earlier work this paper cites.
J. M. Bardeen, Gauge Invariant Cosmological Perturbations , Phys. Rev. D22
1980
Earlier work this paper cites.
P. Sikivie, Of Axions, Domain Walls and the Early Universe , Phys. Rev. Lett. 48
1982
Earlier work this paper cites.
J. Preskill, M. B. Wise and F. Wilczek, Cosmology of the Invisible Axion , Phys. Lett. 120B
1983
Earlier work this paper cites.
L. F. Abbott and P. Sikivie, A Cosmological Bound on the Invisible Axion , Phys. Lett. 120B
1983
Earlier work this paper cites.
M. Dine and W. Fischler, The Not So Harmless Axion , Phys. Lett. 120B
1983
Earlier work this paper cites.
L. Abbott and P. Sikivie, A cosmological bound on the invisible axion , Physics Letters B 120
1983
Earlier work this paper cites.
H. Kodama and M. Sasaki, Cosmological Perturbation Theory , Prog. Theor. Phys. Suppl. 78
1984
Earlier work this paper cites.
M. S. Turner, Cosmic and Local Mass Density of Invisible Axions , Phys. Rev. D33
1986
Earlier work this paper cites.
C. J. Hogan and M. J. Rees, AXION MINICLUSTERS , Phys. Lett. B205
1988
Earlier work this paper cites.
R. Mayle, J. R. Wilson, J. R. Ellis, K. A. Olive, D. N. Schramm and G. Steigman, Constraints on Axions from SN 1987a , Phys. Lett. B203
1988
Earlier work this paper cites.

Similar

D. H. Lyth, Axions and inflation: Sitting in the vacuum , Phys. Rev. D45
1992
Cited alongside, same era.
E. W. Kolb and I. I. Tkachev, Axion miniclusters and Bose stars , Phys. Rev. Lett. 71
1993
Cited alongside, same era.
E. W. Kolb and I. I. Tkachev, Nonlinear axion dynamics and formation of cosmological pseudosolitons , Phys. Rev. D49
1994
Cited alongside, same era.
E. W. Kolb and I. I. Tkachev, Large amplitude isothermal fluctuations and high density dark matter clumps , Phys. Rev. D50
1994
Cited alongside, same era.
E. Seidel and W.-M. Suen, Formation of solitonic stars through gravitational cooling , Phys. Rev. Lett. 72
1994
Cited alongside, same era.
E. W. Kolb and I. I. Tkachev, Femtolensing and picolensing by axion miniclusters , Astrophys. J. 460

Then

I. Tkachev, Phenomenology of Axion Miniclusters , in Proceedings, 11th Patras Workshop on Axions, WIMPs and WISPs (Axion-WIMP 2015): Zaragoza, Spain, June 22-26, 2015 , pp. 173–178, 2015, DOI
2015
Later among the works it cites.
I. I. Tkachev, Fast Radio Bursts and Axion Miniclusters , JETP Lett. 101
Original
2015
Later among the works it cites.
E. Berkowitz, M. I. Buchoff and E. Rinaldi, Lattice QCD input for axion cosmology , Phys. Rev. D92
Original
2015
Later among the works it cites.
D. J. E. Marsh, Axion Cosmology , Phys. Rept. 643
Original
2016
Later among the works it cites.
L. Fleury and G. D. Moore, Axion dark matter: strings and their cores , JCAP 01
Original

Beyond the bibliography

alphaXiv searches the wider corpus for related work and actual follow-ups.

Open on alphaXiv

alphaXiv is searching for related work…

Reading the bibliography…

2021

New scenario of QCD axion clump formation I: Linear analysis

Kitajima, Naoya, Kogai, Kazuhiro, Urakawa, Yuko

Understand

The QCD axion acquires the potential through the non-perturbative effect of the QCD matters around the QCD phase transition.

During this period, the direct interaction between the axion and the QCD matters sets in.
Focusing on the impact of this direct interaction, we propose two scenarios where the fluctuation of the axion can rapidly grow, potentially leading to the formation of axion miniclusters even if the Peccei-Quinn (PQ) symmetry was already broken during inflation.
The first scenario assumes that the primordial curvature perturbation at the horizon scale during the QCD epoch was significantly enhanced and the second one assumes that the initial misalignment was tuned around the hilltop of the potential.

Built on

B. Eggemeier and J. C. Niemeyer, Formation and mass growth of axion stars in axion miniclusters , Phys. Rev. D 100
Original
1906
Earlier work this paper cites.
L. Dai and J. Miralda-Escudé, Gravitational Lensing Signatures of Axion Dark Matter Minihalos in Highly Magnified Stars , Astron. J. 159
Original
1908
Earlier work this paper cites.
A. Kalaja, N. Bellomo, N. Bartolo, D. Bertacca, S. Matarrese, I. Musco et al., From Primordial Black Holes Abundance to Primordial Curvature Power Spectrum (and back) , JCAP 10
Original
1908
Earlier work this paper cites.
A. Arvanitaki, S. Dimopoulos, M. Galanis, L. Lehner, J. O. Thompson and K. Van Tilburg, Large-misalignment mechanism for the formation of compact axion structures: Signatures from the QCD axion to fuzzy dark matter , Phys. Rev. D 101
Original
1909
Earlier work this paper cites.
T. Patel, H. Tashiro and Y. Urakawa, Resonant magnetogenesis from axions , JCAP 2001
Original
1909
Earlier work this paper cites.
B. Eggemeier, J. Redondo, K. Dolag, J. C. Niemeyer and A. Vaquero, First simulations of axion minicluster halos , 1911.09417
Original
1911
Earlier work this paper cites.
N. Blinov, M. J. Dolan and P. Draper, Imprints of the Early Universe on Axion Dark Matter Substructure , Phys. Rev. D 101
Original
1911
Earlier work this paper cites.
J. C. Niemeyer, Small-scale structure of fuzzy and axion-like dark matter , 1912.07064
Original
1912
Earlier work this paper cites.
P. Meszaros, The behaviour of point masses in an expanding cosmological substratum. , Astronomy and Astrophysics 37
1974
Earlier work this paper cites.
R. D. Peccei and H. R. Quinn, CP Conservation in the Presence of Instantons , Phys. Rev. Lett. 38
1977
Earlier work this paper cites.
R. D. Peccei and H. R. Quinn, Constraints Imposed by CP Conservation in the Presence of Instantons , Phys. Rev. D16
1977
Earlier work this paper cites.
S. Weinberg, A New Light Boson? , Phys. Rev. Lett. 40
1978
Earlier work this paper cites.
F. Wilczek, Problem of Strong P P and T T Invariance in the Presence of Instantons , Phys. Rev. Lett. 40
1978
Earlier work this paper cites.
P. Di Vecchia and G. Veneziano, Chiral Dynamics in the Large n Limit , Nucl. Phys. B171
1980
Earlier work this paper cites.
J. M. Bardeen, Gauge Invariant Cosmological Perturbations , Phys. Rev. D22
1980
Earlier work this paper cites.
P. Sikivie, Of Axions, Domain Walls and the Early Universe , Phys. Rev. Lett. 48
1982
Earlier work this paper cites.
J. Preskill, M. B. Wise and F. Wilczek, Cosmology of the Invisible Axion , Phys. Lett. 120B
1983
Earlier work this paper cites.
L. F. Abbott and P. Sikivie, A Cosmological Bound on the Invisible Axion , Phys. Lett. 120B
1983
Earlier work this paper cites.
M. Dine and W. Fischler, The Not So Harmless Axion , Phys. Lett. 120B
1983
Earlier work this paper cites.
L. Abbott and P. Sikivie, A cosmological bound on the invisible axion , Physics Letters B 120
1983
Earlier work this paper cites.
H. Kodama and M. Sasaki, Cosmological Perturbation Theory , Prog. Theor. Phys. Suppl. 78
1984
Earlier work this paper cites.
M. S. Turner, Cosmic and Local Mass Density of Invisible Axions , Phys. Rev. D33
1986
Earlier work this paper cites.
C. J. Hogan and M. J. Rees, AXION MINICLUSTERS , Phys. Lett. B205
1988
Earlier work this paper cites.
R. Mayle, J. R. Wilson, J. R. Ellis, K. A. Olive, D. N. Schramm and G. Steigman, Constraints on Axions from SN 1987a , Phys. Lett. B203
1988
Earlier work this paper cites.

Similar

D. H. Lyth, Axions and inflation: Sitting in the vacuum , Phys. Rev. D45
1992
Cited alongside, same era.
E. W. Kolb and I. I. Tkachev, Axion miniclusters and Bose stars , Phys. Rev. Lett. 71
1993
Cited alongside, same era.
E. W. Kolb and I. I. Tkachev, Nonlinear axion dynamics and formation of cosmological pseudosolitons , Phys. Rev. D49
1994
Cited alongside, same era.
E. W. Kolb and I. I. Tkachev, Large amplitude isothermal fluctuations and high density dark matter clumps , Phys. Rev. D50
1994
Cited alongside, same era.
E. Seidel and W.-M. Suen, Formation of solitonic stars through gravitational cooling , Phys. Rev. Lett. 72
1994
Cited alongside, same era.
E. W. Kolb and I. I. Tkachev, Femtolensing and picolensing by axion miniclusters , Astrophys. J. 460