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We construct cosmological long-wavelength solutions without symmetry in general gauge conditions compatible with the long-wavelength scheme.
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M. Shibata and M. Sasaki, “Black hole formation in the Friedmann universe: Formulation and computation in numerical relativity,” Phys. Rev. D 60
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The corresponding expressions in Shibata and Sasaki (1999) [ 9 ] are slightly different seemingly because of typos there
1999
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A. M. Green, A. R. Liddle, K. A. Malik and M. Sasaki, “A New calculation of the mass fraction of primordial black holes,” Phys. Rev. D 70
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2010
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2011
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2012
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2012
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I. Musco, J. C. Miller and L. Rezzolla, “Computations of primordial black hole formation,” Class. Quant. Grav. 22
2005
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D. H. Lyth, K. A. Malik and M. Sasaki, “A general proof of the conservation of the curvature perturbation,” JCAP 05
2005
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T. Suyama, T. Tanaka, B. Bassett and H. Kudoh, “Are black holes over-produced during preheating?,” Phys. Rev. D 71
2005
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T. Suyama, T. Tanaka, B. Bassett and H. Kudoh, “Black hole production in tachyonic preheating,” JCAP 04
2006
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A. G. Polnarev and I. Musco, “Curvature profiles as initial conditions for primordial black hole formation,” Class. Quant. Grav. 24
2007
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2009
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Y. Tada and S. Yokoyama, “Primordial black holes as biased tracers,” arXiv:1502.01124 [astro-ph.CO]
Cited in the paper.
2013
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2013
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2014
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T. Nakama, “The double formation of primordial black holes,” JCAP 10
2014
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2014
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T. Harada, C. M. Yoo and K. Kohri, “Threshold of primordial black hole formation,” Phys. Rev. D 88
2014
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Nakama (2014) [ 16 ] used a similar double top-hat curvature model to simulate the double formation of PBHs, in which the central perturbation first collapses and this is followed by another collapse of the larger perturbation swallowing the smaller PBH already formed
2014
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