activity
20212026
most citedMinimal Length, Nuclear Matter, and Neutron Stars

12 citations · 18 across the 6 of their papers we have counts for

collaborators

6 papers

gr-qc2026

Black holes in effective loop quantum gravity: Hawking radiation

Idrus Husin Belfaqih, Martin Bojowald, Suddhasattwa Brahma +1

Emergent modified gravity provides a covariant framework for holonomy effects in models of loop quantum gravity with consistent black hole solutions coupled to a scalar field. Seve…

gr-qc2025

Hawking evaporation and the fate of black holes in loop quantum gravity

Idrus Husin Belfaqih, Martin Bojowald, Suddhasattwa Brahma +1

A recent covariant formulation, that includes non-perturbative effects from loop quantum gravity (LQG) as self-consistent effective models, has revealed the possibility of non-sing…

gr-qc2024★ 3 cited

Lessons for loop quantum gravity from emergent modified gravity

Idrus Husin Belfaqih, Martin Bojowald, Suddhasattwa Brahma +1

Most of the potential physical effects of loop quantum gravity have been derived in effective models that modify the constraints of canonical general relativity in specific forms.…

gr-qc2024★ 1 cited

Black holes in effective loop quantum gravity: Covariant holonomy modifications

Idrus Husin Belfaqih, Martin Bojowald, Suddhasattwa Brahma +1

Emergent modified gravity provides a covariant, effective framework for obtaining spherically symmetric black hole solutions in models of loop quantum gravity with scale-dependent…

nucl-th2022★ 12 cited

Minimal Length, Nuclear Matter, and Neutron Stars

I. Prasetyo, I. H. Belfaqih, A. B. Wahidin +2

In this paper, we employ one variant of the Generalized Uncertainty Principle (GUP) model, i.e., the Kempf-Mangano-Mann (KMM) model, and discuss the impact of GUP on the EoS of nuc…

gr-qc2021★ 2 cited

White dwarfs and generalized uncertainty principle

Idrus Husin Belfaqih, Harris Maulana, Anto Sulaksono

This work is motivated by the sign problem in a logarithmic parameter of black hole entropy and the existing more massive white dwarfs than the Chandrasekhar mass limit. We examine…