activity
20122026
most citedTesting loop quantum gravity from observational consequences of non-singular rotating black holes

145 citations · 2.1k across the 96 of their papers we have counts for

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Showing 2019Show all

9 papers · 1 filter

gr-qc2019★ 33 cited

Annihilation-to-nothing: a quantum gravitational boundary condition for the Schwarzschild black hole

Mariam Bouhmadi-López, Suddhasattwa Brahma, Che-Yu Chen +2

The interior of a static Schwarzschild metric can be written in terms of two functions, similar to some models of anisotropic cosmology. With a suitable choice of canonical variabl…

gr-qc2019★ 11 cited

Deformed covariance in spherically symmetric vacuum models of loop quantum gravity: Consistency in Euclidean and self-dual gravity

Martin Bojowald, Suddhasattwa Brahma, Ding Ding +1

Different versions of consistent canonical realizations of hypersurface deformations of spherically symmetric space-times have been derived in models of loop quantum gravity, modif…

hep-th2019★ 44 cited

The trans-Planckian censorship conjecture from the swampland distance conjecture

Suddhasattwa Brahma

Starting from the swampland distance conjecture, and using the species bound for a large number of weakly-coupled particles, we give a derivation of the recently proposed trans-Pla…

hep-th2019★ 63 cited

Trans-Planckian censorship, inflation and excited initial states for perturbations

Suddhasattwa Brahma

The recently proposed trans-Planckian censorship conjecture (TCC) seems to require that the energy scale of inflation is significantly lower than the Planck scale $(H_\text{inf}<10…

gr-qc2019★ 9 cited

Can a false vacuum bubble remove the singularity inside a black hole?

Suddhasattwa Brahma, Dong-han Yeom

We investigate a regular black hole model with a de Sitter-like core at its center. This type of a black hole model with a false vacuum core was introduced with the hope of singula…

hep-th2019★ 38 cited

Stochastic eternal inflation is in the swampland

Suddhasattwa Brahma, Sarah Shandera

We demonstrate that there is no controlled description of stochastic eternal inflation consistent with the refined swampland de Sitter conjecture.

hep-th2019★ 29 cited

Relating the scalar weak gravity conjecture and the swampland distance conjecture for an accelerating universe

Suddhasattwa Brahma, Md. Wali Hossain

For any quasi de Sitter background, we show that a recently proposed scalar weak gravity conjecture (sWGC) follows from the swampland distance conjecture, together with the covaria…

hep-th2019★ 60 cited

Dark energy beyond quintessence: Constraints from the swampland

Suddhasattwa Brahma, Md. Wali Hossain

The string theory swampland proposes that there is no UV-completion for an effective field theory with an exact (metastable) de Sitter vacua, thereby ruling out standard CDM cos…

gr-qc2019★ 48 cited

Asymptotic non-flatness of an effective black hole model based on loop quantum gravity

Mariam Bouhmadi-López, Suddhasattwa Brahma, Che-Yu Chen +2

For any non-rotating effective quantum (uncharged) black hole model to be viable, its asymptotic structure of spacetime should reduce to that of a Schwarzschild black hole. After e…