SearcharxivSearch

arXiv · 2406.01202

A Study of Black Holes and Beyond: Shadows and Relativistic Orbits

Abstract

This doctoral thesis is organized into seven chapters. The first chapter introduces readers to the formation of black holes and naked singularities as an end state of continuous gravitational collapse. The physical and geometrical properties of the Schwarzschild black hole, JMN-1 naked singularity, and JNW naked singularity are summarised. The motivation and objectives to be derived are based on the literature reviews. The second chapter deals with the shadows of the mentioned compact objects. The equations of motion are explicitly calculated for general spherically symmetric and static spacetimes using the ray-tracing formalism and the null geodesics. The third chapter focuses on the construction of rotating naked singularity using the NJA. The NJA is used without complexification method and obtain rotating JNW naked singularity spacetime. The general formalism of the shadow shape is derived for rotating spacetime and obtain the shadow shapes for the rotating JNW, Kerr and deformed Kerr spacetimes. In the fourth chapter, the precession of timelike-bound orbits is investigated in the Schwarzschild, JMN-1, and JNW spacetimes. The fully relativistic orbit equations are derived for the provided models. The approximate solutions of the orbit equations are used to characterize the nature of orbital precession. The next chapter is on the precession of timelike bound orbits in the rotating Kerr and JNW spacetimes. The sixth chapter deals with the relativistic orbits of S-stars and discusses the orbital parameters of the real and apparent orbits. Astrometric data of the S2 star has been adopted from the available literature and use numerical techniques to study the relativistic orbits of the S2 star in the presence of a scalar field. The final chapter aims at summarising the results followed by some futuristic scopes that probe the nature of Sgr A* with a possible black hole mimicker.

Explore related subjects

Keep this discovery

BibTeXRIS

Parth Bambhaniya. 2024-06-03. A Study of Black Holes and Beyond: Shadows and Relativistic Orbits. https://arxiv.org/abs/2406.01202

Cite the original work for its findings. Save a collection to share your selection of sources.

KEEP EXPLORING

Related papers

Electrovacuum Black Hole Uniqueness

We prove the black hole uniqueness conjecture in the axially symmetric, stationary, electrovacuum setting, subject to the refined asymptotic analysis of the associated singular harmonic maps, which includes an analyticity hypothesis at the axes. More precisely, it is shown that any asymptotically flat solution of the Einstein--Maxwell equations in this class, with more than one black hole horizon component is either: Majumdar--Papapetrou, up to a duality rotation, in which case all logarithmic angle defects vanish, or every finite axis rod logarithmic angle defect is strictly negative and hence every interaction force is strictly attractive. The proof extends the singular harmonic map method used for vacuum Kerr uniqueness in [18].

gr-qc

Constraining Modified Mass-to-Horizon Cosmology Through Primordial Inflationary Observables

We investigate slow-roll inflation in a modified cosmological framework inspired by a generalized mass-to-horizon relation (MHR), $M=\gamma {c^2 L^n}/{G}$, where $n$ is a real parameter and $\gamma$ a dimensional constant. Using Padmanabhan's emergence paradigm, we derive the modified Friedmann equations for a flat FRW universe and analyze the dynamics of a canonical scalar field (inflaton) under the slow-roll approximation. We study the resulting inflationary phenomenology for power-law and Starobinsky potentials. For power-law potentials, the MHR modification fails to reconcile these models with current CMB constraints on $r$ and $n_s$. In contrast, Starobinsky inflation exhibits significant sensitivity to deviations from $n=1$. A perturbative analysis ($n=1+\Delta$) yields corrections to inflationary observables. We observe that the scalar power-spectrum normalization, under a fixed-Starobinsky prescription, imposes the stringent constraint $0.960 \lesssim n \lesssim 1.040$ for $N=60$ efolds. This is considerably tighter than spectral-index bounds. Our results establish inflation, particularly Starobinsky-like models, as a sensitive probe of generalized horizon thermodynamics and departures from standard MHR scaling.

gr-qc

Improving the Sensitivity of Gravitational Wave Detection with Weighted Conformal Prediction

In the last decade, kilometre-scale interferometric gravitational-wave detectors have observed hundreds of compact binary mergers, the majority of which are binary black holes. However, the data are noise-dominated, and multiple independent search algorithms (pipelines) are used to enhance sensitivity and improve robustness. Rather than the standard approach of selecting the most significant pipeline output, we combine the outputs from all pipelines using a conformal prediction-based framework to provide statistically rigorous confidence estimates for candidate events. While combining pipelines improves sensitivity and ranking robustness, it requires a principled statistical framework that remains valid as data properties evolve across observing runs. A key challenge is distribution shifts between simulated datasets used for training and calibration and the real, unlabelled, observations used for testing, which can invalidate coverage guarantees and bias confidence estimates. In this work, we address this challenge by incorporating likelihood-ratio reweighting into our conformal prediction framework to account for covariate shift. Using mock datasets containing simulated signals, we demonstrate that weighted conformal prediction restores well-calibrated coverage under covariate shift and increases the confidence of events near the detection threshold, recovering true signals that would otherwise be missed.

gr-qc