Search:
Match:
3 results
Physics#Black Holes, Dark Matter, General Relativity🔬 ResearchAnalyzed: Jan 3, 2026 08:43

Probing Magnetically Charged Black Hole in Dark Matter Halo

Published:Dec 31, 2025 09:55
1 min read
ArXiv

Analysis

The paper investigates the combined effects of non-linear electrodynamics (NED) and dark matter (DM) on a magnetically charged black hole (BH) within a Hernquist DM halo. The study focuses on how magnetic charge and halo parameters influence BH observables, particularly event horizon position, critical impact parameter, and strong gravitational lensing (GL) phenomena. A key finding is the potential for charge and halo parameters to nullify each other's effects, making the BH indistinguishable from a Schwarzschild BH in terms of certain observables. The paper also uses observational data from super-massive BHs (SMBHs) to constrain the model parameters.
Reference

“The paper finds combinations of charge and halo parameters that leave the deflection angle unchanged from the Schwarzschild case, thereby leading to a situation where an MHDM BH and a Schwarzschild BH become indistinguishable.”

PermalinkArXiv
Research Paper#Astrophysics, Stellar Dynamics, Accretion Disks🔬 ResearchAnalyzed: Jan 3, 2026 16:58

Orbital Dynamics in Dense Stellar Systems with Accretion Disks

Published:Dec 29, 2025 19:46
1 min read
ArXiv

Analysis

This paper provides a high-level overview of the complex dynamics within dense stellar systems and nuclear star clusters, particularly focusing on the interplay between stellar orbits, gravitational interactions, physical collisions, and the influence of an accretion disk around a supermassive black hole. It highlights the competing forces at play and their impact on stellar distribution, black hole feeding, and observable phenomena. The paper's value lies in its concise description of these complex interactions.
Reference

“The paper outlines the influences in their mutual competition.”

PermalinkArXiv
Research Paper#Astrophysics, Cosmology, Dark Matter, Black Holes🔬 ResearchAnalyzed: Jan 3, 2026 18:29

Dark Matter's Role in Early Black Hole Formation

Published:Dec 29, 2025 19:00
1 min read
ArXiv

Analysis

This paper addresses the challenge of explaining the early appearance of supermassive black holes (SMBHs) observed by JWST. It proposes a novel mechanism where dark matter (DM) interacts with Population III stars, causing them to collapse into black hole seeds. This offers a potential solution to the SMBH formation problem and suggests testable predictions for future experiments and observations.
Reference

“The paper proposes a mechanism in which non-annihilating dark matter (DM) with non-gravitational interactions with the Standard Model (SM) particles accumulates inside Population III (Pop III) stars, inducing their premature collapse into BH seeds having the same mass as the parent star.”

PermalinkArXiv