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N. Dadhich, “Buchdahl compactness limit and gravitational field energy,” JCAP
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1903
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D. z. Glavan and C. Lin, “Einstein-Gauss-Bonnet gravity in 4-dimensional space-time,” Phys. Rev. Lett
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1905
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R. Gannouji, Y. Rodríguez Baez, and N. Dadhich, “Pure Lovelock black holes in dimensions d = 3 N + 1 d=3N+1 are stable,” Phys. Rev. D
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1907
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A. K. Mishra and S. Chakraborty, “Strong Cosmic Censorship in higher curvature gravity,” Phys. Rev. D
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1911
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Similar

A. K. Mishra, “Quasinormal modes and Strong Cosmic Censorship in the novel 4D Einstein-Gauss-Bonnet gravity,” arXiv:2004.01243 [gr-qc]
Original
2004
Cited alongside, same era.
N. Dadhich, “On causal structure of 4 D 4D -Einstein-Gauss-Bonnet black hole,” arXiv:2005.05757 [gr-qc]
Original
2005
Cited alongside, same era.
C. Boehmer and T. Harko, “Minimum mass-radius ratio for charged gravitational objects,” Gen. Rel. Grav
2007
Cited alongside, same era.
H. Andreasson, “Sharp bounds on 2m/r of general spherically symmetric static objects,” J. Diff. Eq
2008
Cited alongside, same era.
P. Karageorgis and J. G. Stalker, “Sharp bounds on 2m/r for static spherical objects,” Class. Quant. Grav
Original
2008
Cited alongside, same era.

Then

S. Chakraborty, “Lanczos-Lovelock gravity from a thermodynamic perspective,” JHEP
Original
2015
Later among the works it cites.
S. Chakraborty and N. Dadhich, “Brown-York quasilocal energy in Lanczos-Lovelock gravity and black hole horizons,” JHEP
Original
2015
Later among the works it cites.
M. Wright, “Buchdahl’s inequality in five dimensional Gauss–Bonnet gravity,” Gen. Rel. Grav
Original
2016
Later among the works it cites.
N. Dadhich, “A distinguishing gravitational property for gravitational equation in higher dimensions,” Eur. Phys. J. C
Original
2016
Later among the works it cites.
X. O. Camanho and N. Dadhich, “On Lovelock analogs of the Riemann tensor,” Eur. Phys. J. C

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2020

Limits on stellar structures in Lovelock theories of gravity

Chakraborty, Sumanta, Dadhich, Naresh

Understand

We study the bound on the compactness of a stellar object in pure Lovelock theories of arbitrary order in arbitrary spacetime dimensions, involving electromagnetic field.

The bound we derive for a generic pure Lovelock theory, reproduces the known results in four dimensional Einstein gravity.
Both the case of a charged shell and that of a charge sphere demonstrates that for a given spacetime dimension, stars in general relativity are more compact than the stars in pure Lovelock theories.
In addition, as the strength of the Maxwell field increases, the stellar structures become more compact, i.e., the radius of the star decreases.