activity
20142024
most citedPhysical Characteristics and Maximum Allowable Mass of Hybrid Star in the Context of Gravity

104 citations · 463 across the 14 of their papers we have counts for

collaborators

14 papers

gr-qc2024

Properties of wormhole model in de Rham-Gabadadze-Tolley like massive gravity with specific matter density

Piyali Bhar

In the conventional method of studying wormhole (WH) geometry, traversability requires the presence of exotic matter, which also provides negative gravity effects to keep the wormh…

gr-qc202411 cited

Noncommutative wormhole in de Rham-Gabadadze-Tolley like massive gravity

Piyali Bhar, Allah Ditta, Abdelghani Errehymy

The wormhole solution in dRGT massive gravity is examined in this paper in the background of non-commutative geometry. In order to derive the wormhole model, along with the zero ti…

gr-qc20241 cited

Noncommutative black hole in de Rham-Gabadadze-Tolley like massive gravity

Piyali Bhar, Dhruba Jyoti Gogoi, Supakchai Ponglertsakul

We examine the behavior of non-commutative Schwarzschild black holes in the context of massive gravity. According to the investigation, corresponding to a minimal mass, the black h…

gr-qc20241 cited

(3+1)-D gravastar in de Rham-Gabadadze-Tolley-like massive gravity

Piyali Bhar

The physical properties of a (3+1)-D gravastar in the context of massive gravity are discussed in this work. In present investigation, the field equations have been solved for a st…

gr-qc202329 cited

Relativistic isotropic stellar model in gravity with Durgapal- IV Metric

Pramit Rej, Piyali Bhar

In this work, a new static, non-singular, spherically symmetric fluid model has been obtained in the background of gravity. Here we consider the isotropic metric potenti…

gr-qc2023104 cited

Physical Characteristics and Maximum Allowable Mass of Hybrid Star in the Context of Gravity

Piyali Bhar, Sneha Pradhan, Adnan Malik +1

In this study, we explore several new characteristics of a static anisotropic hybrid star with strange quark matter (SQM) and ordinary baryonic matter (OBM) distribution. Here, we…