Fetching the paper…
Reading the bibliography…
Lemaitre-Tolman-Bondi (LTB) solutions are used frequently to describe the collapse or expansion of spherically symmetric inhomogeneous mass distributions in the Universe.
G. Lemaître, Ann. soc. Sci. Bruxelles Ser.1, A53, 51, 1933; R. C. Tolman,Proc. Nat1. Acad. Sci. U.S.A. 20,410, 1934; H. Bondi, Mon. Not. R. Astron. Soc., 107, 343, 1947)
1947
Earlier work this paper cites.
P. J. E. Peebles, “The Large Scale structure of the Universe,” Princeton University Press (1980)
1980
Earlier work this paper cites.
C. P. Ma and E. Bertschinger, Astrophys. J. 4 55
1995
Earlier work this paper cites.
K. Tomita, Prog. Theor. Phys. 106
2001
Earlier work this paper cites.
D. W. Hogg, D. J. Eisenstein, M. R. Blanton, N. A. Bahcall, J. Brinkmann, J. E. Gunn and D. P. Schneider, Astrophys. J. 624
2005
Earlier work this paper cites.
D. E. Holz and E. V. Linder, Astrophys. J. 631
2005
Earlier work this paper cites.
S. Rasanen, JCAP 0611
2006
Earlier work this paper cites.
A. Notari, Mod. Phys. Lett. A 21
2006
Cited alongside, same era.
E. W. Kolb, S. Matarrese and A. Riotto, New J. Phys. 8
2006
Cited alongside, same era.
A. Ishibashi and R. M. Wald, Class. Quant. Grav. 23
2006
Cited alongside, same era.
H. Alnes, M. Amarzguioui and O. Gron, Phys. Rev. D 73
2006
Cited alongside, same era.
R. A. Vanderveld, E. E. Flanagan and I. Wasserman, Phys. Rev. D 74
2006
Cited alongside, same era.
D. L. Wiltshire, New J. Phys. 9
2007
Cited alongside, same era.
T. Biswas, R. Mansouri and A. Notari, JCAP 0712
2007
Cited alongside, same era.
N. Brouzakis, N. Tetradis and E. Tzavara, JCAP 0804
2007
Later among the works it cites.
V. Marra, E. W. Kolb, S. Matarrese and A. Riotto, Phys. Rev. D 76
2007
Later among the works it cites.
2008
Closest in time.
T. Buchert, Gen. Rel. Grav. 40
2008
Closest in time.
T. Biswas and A. Notari, JCAP 0806
2008
Closest in time.
alphaXiv searches the wider corpus for related work and actual follow-ups.
alphaXiv is searching for related work…
M. N. Celerier, arXiv:astro-ph/0702416
Cited in the paper.
J. Larena, J. M. Alimi, T. Buchert, M. Kunz and P. S. Corasaniti, arXiv:0808.1161 [astro-ph];
Cited in the paper.
E. W. Kolb, V. Marra and S. Matarrese, arXiv:0807.0401 [astro-ph]
Cited in the paper.
In [ 15 ] the term ξ 0 ′ 2 2 R ′ R \frac{{{\xi^{0}}^{\prime}}^{2}}{2R^{\prime}R} is missing on the right-hand side of Eq. (35). Taking this term into account one finds an additional term − 1 4 ( a v ~ ) 2 -\frac{1}{4}(a\tilde{v})^{2} in the field ψ ~ \tilde{\psi} , making A + ψ ~ = 0 A+\tilde{\psi}=0 , in agreement with our results
Cited in the paper.
2008
Closest in time.
2008
Closest in time.