Built on

M. Mirbabayi, A. Gruzinov, and J. Norena, “Spin of Primordial Black Holes,” arXiv:1901.05963 [astro-ph.CO]
Original
1901
Earlier work this paper cites.
C. D. Kreisch, F.-Y. Cyr-Racine, and O. Dore, “The Neutrino Puzzle: Anomalies, Interactions, and Cosmological Tensions,” arXiv:1902.00534 [astro-ph.CO]
Original
1902
Earlier work this paper cites.
K. L. Pandey, T. Karwal, and S. Das, “Alleviating the H 0 H_{0} and σ 8 \sigma_{8} anomalies with a decaying dark matter model,” arXiv:1902.10636 [astro-ph.CO]
Original
1902
Earlier work this paper cites.
V. De Luca, V. Desjacques, G. Franciolini, A. Malhotra, and A. Riotto, “The initial spin probability distribution of primordial black holes,” JCAP
Original
1903
Earlier work this paper cites.
A. G. Riess, S. Casertano, W. Yuan, L. M. Macri, and D. Scolnic, “Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM,” arXiv:1903.07603 [astro-ph.CO]
Original
1903
Earlier work this paper cites.
K. Vattis, S. M. Koushiappas, and A. Loeb, “Dark matter decaying in the late Universe can relieve the H0 tension,” Phys. Rev
Original
1903
Earlier work this paper cites.
S. Kumar, R. C. Nunes, and S. K. Yadav, “Dark sector interaction: a remedy of the tensions between CMB and LSS data,” Eur. Phys. J
Original
1903
Earlier work this paper cites.
V. Atal, J. Garriga, and A. Marcos-Caballero, “Primordial black hole formation with non-Gaussian curvature perturbations,” arXiv:1905.13202 [astro-ph.CO]
Original
1905
Earlier work this paper cites.
G. Panagopoulos and E. Silverstein, “Primordial Black Holes from non-Gaussian tails,” arXiv:1906.02827 [hep-th]
Original
1906
Earlier work this paper cites.
W. Yang, O. Mena, S. Pan, and E. Di Valentino, “Dark sectors with dynamical coupling,” arXiv:1906.11697 [astro-ph.CO]
Original
1906
Earlier work this paper cites.
E. Di Valentino, R. Z. Ferreira, L. Visinelli, and U. Danielsson, “Late time transitions in the quintessence field and the H 0 H_{0} tension,” Phys. Dark Univ
Original
1906
Earlier work this paper cites.
J. Martin, T. Papanikolaou, and V. Vennin, “Primordial black holes from the preheating instability,” arXiv:1907.04236 [astro-ph.CO]
Original
1907
Earlier work this paper cites.
S. Hawking, “Gravitationally collapsed objects of very low mass,” Mon. Not. Roy. Astron. Soc
1971
Earlier work this paper cites.
H. Akaike, “A new look at the statistical model identification,” IEEE Transactions on Automatic Control
1974
Earlier work this paper cites.
D. N. Page, “Particle Emission Rates from a Black Hole: Massless Particles from an Uncharged, Nonrotating Hole,” Phys. Rev
1976
Earlier work this paper cites.
H. Kodama, M. Sasaki, and K. Sato, “Abundance of Primordial Holes Produced by Cosmological First Order Phase Transition,” Prog. Theor. Phys
1979
Earlier work this paper cites.
M. Crawford and D. N. Schramm, “Spontaneous Generation of Density Perturbations in the Early Universe,” Nature
1982
Earlier work this paper cites.
S. W. Hawking, I. G. Moss, and J. M. Stewart, “Bubble Collisions in the Very Early Universe,” Phys. Rev
1982
Earlier work this paper cites.
D. N. Page, “COMMENT ON ‘ENTROPY EVAPORATED BY A BLACK HOLE’,” Phys. Rev. Lett
1983
Earlier work this paper cites.
C. J. Hogan, “MASSIVE BLACK HOLES GENERATED BY COSMIC STRINGS,” Phys. Lett
1984
Earlier work this paper cites.
M. Khlopov, B. A. Malomed, and I. B. Zeldovich, “Gravitational instability of scalar fields and formation of primordial black holes,” Mon. Not. Roy. Astron. Soc
1985
Earlier work this paper cites.
S. W. Hawking, “Black Holes From Cosmic Strings,” Phys. Lett
1989
Earlier work this paper cites.
A. Polnarev and R. Zembowicz, “Formation of Primordial Black Holes by Cosmic Strings,” Phys. Rev
1991
Earlier work this paper cites.
J. H. MacGibbon, “Quark and gluon jet emission from primordial black holes. 2. The Lifetime emission,” Phys. Rev
1991
Earlier work this paper cites.
J. D. Barrow, E. J. Copeland, and A. R. Liddle, “The Evolution of black holes in an expanding universe,” Mon. Not. Roy. Astron. Soc
1991
Earlier work this paper cites.
J. Garriga and M. Sakellariadou, “Effects of friction on cosmic strings,” Phys. Rev
1993
Earlier work this paper cites.
I. G. Moss, “Singularity formation from colliding bubbles,” Phys. Rev
1994
Earlier work this paper cites.
B. J. Carr, J. H. Gilbert, and J. E. Lidsey, “Black hole relics and inflation: Limits on blue perturbation spectra,” Phys. Rev
1994
Earlier work this paper cites.

Similar

R. V. Konoplich, S. G. Rubin, A. S. Sakharov, and M. Yu. Khlopov, “Formation of black holes in first-order phase transitions as a cosmological test of symmetry-breaking mechanisms,” Phys. Atom. Nucl
1999
Cited alongside, same era.
S. G. Rubin, M. Yu. Khlopov, and A. S. Sakharov, “Primordial black holes from nonequilibrium second order phase transition,” Grav. Cosmol
2000
Cited alongside, same era.
M. Yu. Khlopov, R. V. Konoplich, S. G. Rubin, and A. S. Sakharov, “First-order phase transitions as a source of black holes in the early universe,” Grav. Cosmol
2000
Cited alongside, same era.
S. G. Rubin, A. S. Sakharov, and M. Yu. Khlopov, “The Formation of primary galactic nuclei during phase transitions in the early universe,” J. Exp. Theor. Phys
2001
Cited alongside, same era.
R. Jimenez and A. Loeb, “Constraining cosmological parameters based on relative galaxy ages,” Astrophys. J

Then

R.-Y. Guo and X. Zhang, “Constraining dark energy with Hubble parameter measurements: an analysis including future redshift-drift observations,” Eur. Phys. J
Original
2016
Later among the works it cites.
J. Garcia-Bellido, “Massive Primordial Black Holes as Dark Matter and their detection with Gravitational Waves,” J. Phys. Conf. Ser
Original
2017
Later among the works it cites.
J. Garcia-Bellido and E. Ruiz Morales, “Primordial black holes from single field models of inflation,” Phys. Dark Univ
Original
2017
Later among the works it cites.
C. Germani and T. Prokopec, “On primordial black holes from an inflection point,” Phys. Dark Univ
Original
2017
Later among the works it cites.
E. Cotner and A. Kusenko, “Primordial black holes from supersymmetry in the early universe,” Phys. Rev. Lett

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2019

Evaporating primordial black holes as varying dark energy

Nesseris, Savvas, Sapone, Domenico, Sypsas, Spyros

Understand

If light enough primordial black holes (PBH) account for dark matter, then its density decreases with time as they lose mass via Hawking radiation.

We show that this time-dependence of the matter density can be formulated as an equivalent $w(z)$ dark energy model and we study its implications on the expansion history.
Using our approach and comparing with the latest cosmological data, including the supernovae type Ia, Baryon Acoustic Oscillations, Cosmic Microwave Background and the Hubble expansion H(z) data, we place observational constraints on the PBH model.
We find that it is statistically consistent with $\Lambda$CDM according to the AIC statistical tool.

Built on

M. Mirbabayi, A. Gruzinov, and J. Norena, “Spin of Primordial Black Holes,” arXiv:1901.05963 [astro-ph.CO]
Original
1901
Earlier work this paper cites.
C. D. Kreisch, F.-Y. Cyr-Racine, and O. Dore, “The Neutrino Puzzle: Anomalies, Interactions, and Cosmological Tensions,” arXiv:1902.00534 [astro-ph.CO]
Original
1902
Earlier work this paper cites.
K. L. Pandey, T. Karwal, and S. Das, “Alleviating the H 0 H_{0} and σ 8 \sigma_{8} anomalies with a decaying dark matter model,” arXiv:1902.10636 [astro-ph.CO]
Original
1902
Earlier work this paper cites.
V. De Luca, V. Desjacques, G. Franciolini, A. Malhotra, and A. Riotto, “The initial spin probability distribution of primordial black holes,” JCAP
Original
1903
Earlier work this paper cites.
A. G. Riess, S. Casertano, W. Yuan, L. M. Macri, and D. Scolnic, “Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM,” arXiv:1903.07603 [astro-ph.CO]
Original
1903
Earlier work this paper cites.
K. Vattis, S. M. Koushiappas, and A. Loeb, “Dark matter decaying in the late Universe can relieve the H0 tension,” Phys. Rev
Original
1903
Earlier work this paper cites.
S. Kumar, R. C. Nunes, and S. K. Yadav, “Dark sector interaction: a remedy of the tensions between CMB and LSS data,” Eur. Phys. J
Original
1903
Earlier work this paper cites.
V. Atal, J. Garriga, and A. Marcos-Caballero, “Primordial black hole formation with non-Gaussian curvature perturbations,” arXiv:1905.13202 [astro-ph.CO]
Original
1905
Earlier work this paper cites.
G. Panagopoulos and E. Silverstein, “Primordial Black Holes from non-Gaussian tails,” arXiv:1906.02827 [hep-th]
Original
1906
Earlier work this paper cites.
W. Yang, O. Mena, S. Pan, and E. Di Valentino, “Dark sectors with dynamical coupling,” arXiv:1906.11697 [astro-ph.CO]
Original
1906
Earlier work this paper cites.
E. Di Valentino, R. Z. Ferreira, L. Visinelli, and U. Danielsson, “Late time transitions in the quintessence field and the H 0 H_{0} tension,” Phys. Dark Univ
Original
1906
Earlier work this paper cites.
J. Martin, T. Papanikolaou, and V. Vennin, “Primordial black holes from the preheating instability,” arXiv:1907.04236 [astro-ph.CO]
Original
1907
Earlier work this paper cites.
S. Hawking, “Gravitationally collapsed objects of very low mass,” Mon. Not. Roy. Astron. Soc
1971
Earlier work this paper cites.
H. Akaike, “A new look at the statistical model identification,” IEEE Transactions on Automatic Control
1974
Earlier work this paper cites.
D. N. Page, “Particle Emission Rates from a Black Hole: Massless Particles from an Uncharged, Nonrotating Hole,” Phys. Rev
1976
Earlier work this paper cites.
H. Kodama, M. Sasaki, and K. Sato, “Abundance of Primordial Holes Produced by Cosmological First Order Phase Transition,” Prog. Theor. Phys
1979
Earlier work this paper cites.
M. Crawford and D. N. Schramm, “Spontaneous Generation of Density Perturbations in the Early Universe,” Nature
1982
Earlier work this paper cites.
S. W. Hawking, I. G. Moss, and J. M. Stewart, “Bubble Collisions in the Very Early Universe,” Phys. Rev
1982
Earlier work this paper cites.
D. N. Page, “COMMENT ON ‘ENTROPY EVAPORATED BY A BLACK HOLE’,” Phys. Rev. Lett
1983
Earlier work this paper cites.
C. J. Hogan, “MASSIVE BLACK HOLES GENERATED BY COSMIC STRINGS,” Phys. Lett
1984
Earlier work this paper cites.
M. Khlopov, B. A. Malomed, and I. B. Zeldovich, “Gravitational instability of scalar fields and formation of primordial black holes,” Mon. Not. Roy. Astron. Soc
1985
Earlier work this paper cites.
S. W. Hawking, “Black Holes From Cosmic Strings,” Phys. Lett
1989
Earlier work this paper cites.
A. Polnarev and R. Zembowicz, “Formation of Primordial Black Holes by Cosmic Strings,” Phys. Rev
1991
Earlier work this paper cites.
J. H. MacGibbon, “Quark and gluon jet emission from primordial black holes. 2. The Lifetime emission,” Phys. Rev
1991
Earlier work this paper cites.
J. D. Barrow, E. J. Copeland, and A. R. Liddle, “The Evolution of black holes in an expanding universe,” Mon. Not. Roy. Astron. Soc
1991
Earlier work this paper cites.
J. Garriga and M. Sakellariadou, “Effects of friction on cosmic strings,” Phys. Rev
1993
Earlier work this paper cites.
I. G. Moss, “Singularity formation from colliding bubbles,” Phys. Rev
1994
Earlier work this paper cites.
B. J. Carr, J. H. Gilbert, and J. E. Lidsey, “Black hole relics and inflation: Limits on blue perturbation spectra,” Phys. Rev
1994
Earlier work this paper cites.

Similar

R. V. Konoplich, S. G. Rubin, A. S. Sakharov, and M. Yu. Khlopov, “Formation of black holes in first-order phase transitions as a cosmological test of symmetry-breaking mechanisms,” Phys. Atom. Nucl
1999
Cited alongside, same era.
S. G. Rubin, M. Yu. Khlopov, and A. S. Sakharov, “Primordial black holes from nonequilibrium second order phase transition,” Grav. Cosmol
2000
Cited alongside, same era.
M. Yu. Khlopov, R. V. Konoplich, S. G. Rubin, and A. S. Sakharov, “First-order phase transitions as a source of black holes in the early universe,” Grav. Cosmol
2000
Cited alongside, same era.
S. G. Rubin, A. S. Sakharov, and M. Yu. Khlopov, “The Formation of primary galactic nuclei during phase transitions in the early universe,” J. Exp. Theor. Phys
2001
Cited alongside, same era.
R. Jimenez and A. Loeb, “Constraining cosmological parameters based on relative galaxy ages,” Astrophys. J