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EDITORIAL article

Front. Astron. Space Sci.

Sec. Cosmology

Volume 12 - 2025 | doi: 10.3389/fspas.2025.1563337

This article is part of the Research Topic Experimental Predictions in General Relativity: What Now? View all 5 articles

Editorial: Experimental Predictions in General Relativity: What Now?

Provisionally accepted
  • 1 University of Salerno, Fisciano, Italy
  • 2 Rotonium Quantum Computing, Padua, Italy
  • 3 Institute for Scientific Methodology (ISEM), Palermo, Italy

The final, formatted version of the article will be published soon.

    data.Finally, in the review article Testing parity symmetry of gravity with gravitational waves, J. Qiao et al. examine the role of parity symmetry in gravitational interactions. While Einstein's general relativity preserves parity, various theories of parity-violating (PV) gravity have recently been proposed across different theoretical frameworks, driven by diverse motivations. In this review, the authors summarize recent advancements in these theories, focusing specifically on the observable effects of PV terms in gravitational waves (GWs), particularly the differences between left-hand and right-hand polarization modes. The authors emphasize the implications of these theories for GWs produced by compact binary coalescences and primordial GWs from the early universe. Deviations in the GW waveforms or the primordial power spectrum can be characterized by the energy scale at which parity violation occurs in each theory. By analyzing current and future observations from laser interferometers and the cosmic microwave background radiation, they present both the existing and potential constraints on the energy scale of PV. These constraints suggest that the parity symmetry of gravity can be tested at high energy scales in the emerging era of gravitational wave research.These four papers collectively provide a broad perspective on active research directions -some focusing on the dark energy and dark matter problem, while others explore potential deviations from general relativity. Strong-field gravitational lensing and gravitational wave physics are among the most promising avenues for detecting such deviations. Hopefully, the ideas presented in these papers will help refine our understanding and enhance our ability to identify these signatures.

    Keywords: general relativity, black holes, dark matter, dark energy, Expanding universe

    Received: 19 Jan 2025; Accepted: 19 Feb 2025.

    Copyright: © 2025 Feleppa, Benedetto, Iovane, Tamburini and Licata. This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) or licensor are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.

    * Correspondence: Elmo Benedetto, University of Salerno, Fisciano, Italy

    Disclaimer: All claims expressed in this article are solely those of the authors and do not necessarily represent those of their affiliated organizations, or those of the publisher, the editors and the reviewers. Any product that may be evaluated in this article or claim that may be made by its manufacturer is not guaranteed or endorsed by the publisher.

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