SearcharxivSearch

arXiv · 2506.06783

Across the Horizon: On Gravitational Wave Flux Laws and Tests of Gravity

Abstract

Motivated by the first detection of gravitational waves, this dissertation develops analytical, numerical, and data analysis techniques to address persistent blind spots in our understanding of gravity. Beginning with asymptotically flat spacetimes and the geometry of null geodesic congruences, the derivation of the shear tensor--encoding gravitational radiation--is revisited. The covariant phase space formulation of General Relativity is then employed to derive a non-conservation law associated with the symmetry group at null infinity, generalizing prior constructions of radiative phase space and yielding consistent results. These flux laws are used to derive constraint equations that enable the evaluation and comparison of state-of-the-art numerical waveform models, leading to new insights and a robust algorithm for benchmarking future improvements. These flux laws are further applied to compute quantum corrections to gravitational waveforms arising from the gravitational wave echo effect. Two leading phenomenological scenarios involving echoes from binary black hole mergers are analyzed. The structure of both the primary echo signal and its induced corrections to nonlinear features of the waveform are studied for observability by the upcoming LISA mission. The results indicate that LISA could detect such signals, potentially probing black hole area quantization. Finally, motivated by recent hints of a stochastic gravitational wave background from Pulsar Timing Array data, this work reviews its theoretical basis and studies several astrophysical and cosmological source scenarios. A forecast for detection prospects with LISA is presented using a modern data analysis pipeline. The results suggest LISA will constrain the extra-galactic stochastic background to a spectral energy density below $ \Omega_\text{GW} \lesssim 10^{-8}$.

Explore related subjects

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

David Maibach. 2025-06-07. Across the Horizon: On Gravitational Wave Flux Laws and Tests of Gravity. https://arxiv.org/abs/2506.06783

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