Abstract
Einstein’s general theory of relativity is plagued by cosmological and black-hole type singularities Recently, it has been shown that infinite derivative, ghost free, gravity can yield nonsingular cosmological and mini-black hole solutions. In particular, the theory possesses a mass-gap determined by the scale of new physics. This paper provides a plausible argument, not a no-go theorem, based on the Area-law of gravitational entropy that within infinite derivative, ghost free, gravity nonsingular compact objects in the static limit need not have horizons.
Original language | English |
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Article number | 084069 |
Number of pages | 6 |
Journal | Physical Review D |
Volume | 96 |
DOIs | |
Publication status | Published - 31-Oct-2017 |
Keywords
- COSMOLOGY
- BACKGROUNDS
- BLACK-HOLE ENTROPY
- FIELD-THEORY
- GRAVITATIONAL COLLAPSE
- QUANTUM-GRAVITY
- NOETHER CHARGE
- SPACE-TIME
- SINGULARITIES