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19962008
most citedThe Spatial Averaging Limit of Covariant Macroscopic Gravity - Scalar Corrections to the Cosmological Equations

55 citations · 216 across the 12 of their papers we have counts for

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Showing 2007Show all

7 papers · 1 filter

gr-qc200742 cited

Mass Spectrum and Statistical Entropy of the BTZ black hole from Canonical Quantum Gravity

Cenalo Vaz, Sashideep Gutti, Claus Kiefer +2

In a recent publication we developed a canonical quantization program describing the gravitational collapse of a spherical dust cloud in 2+1 dimensions with a negative cosmological…

gr-qc200714 cited

Classical and Quantum Gravitational Collapse in d-dim AdS Spacetime I. Classical Solutions

Rakesh Tibrewala, Sashideep Gutti, T. P. Singh +1

We study the collapse of a spherically symmetric dust distribution in -dimensional AdS spacetime. We investigate the role of dimensionality, and the presence of a negative cosmo…

gr-qc200724 cited

Quantum Gravitational Collapse and Hawking Radiation in 2+1 Dimensions

Cenalo Vaz, Sashideep Gutti, Claus Kiefer +1

We develop the canonical theory of gravitational collapse in 2+1 dimensions with a negative cosmological constant and obtain exact solutions of the Wheeler--DeWitt equation regular…

gr-qc20072 cited

The inevitable nonlinearity of quantum gravity falsifies the many-worlds interpretation of quantum mechanics

T. P. Singh

There are fundamental reasons as to why there should exist a reformulation of quantum mechanics which does not refer to a classical spacetime manifold. It follows as a consequence…

gr-qc20078 cited

Particle creation in (2+1) circular dust collapse

Sashideep Gutti, T. P. Singh

We investigate the quantum particle creation during the circularly symmetric collapse of a 2+1 dust cloud, for the cases when the cosmological constant is either zero or negative.…

gr-qc200755 cited

The Spatial Averaging Limit of Covariant Macroscopic Gravity - Scalar Corrections to the Cosmological Equations

Aseem Paranjape, T. P. Singh

It is known that any explicit averaging scheme of the type essential for describing the large scale behaviour of the Universe, must necessarily yield corrections to the Einstein eq…