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  1. 81

    Gravitational odd-parity perturbation of a Horndeski hairy black hole: quasinormal mode and parameter constraint by Zhen-Hao Yang, Yun-He Lei, Xiao-Mei Kuang, Bin Wang

    Published 2025-01-01
    “…Abstract During the binary black hole coalescence, gravitational waves emitted at the ringdown stage can be well described by black hole perturbation theory, where the quasinormal modes (QNMs) become the important ingredient in modeling the pattern waveform. …”
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    Article
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    Response to: Comment on “Does the Equivalence between Gravitational Mass and Energy Survive for a Composite Quantum Body?” by A. G. Lebed

    Published 2017-01-01
    “…We have recently shown that both passive and active gravitational masses of a composite body are not equivalent to its energy due to some quantum effects. …”
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    Article
  4. 84

    Slaying axion-like particles via gravitational waves and primordial black holes from supercooled phase transition by Angela Conaci, Luigi Delle Rose, P. S. Bhupal Dev, Anish Ghoshal

    Published 2024-12-01
    “…Moreover, the supercooled PT leads to a potentially observable stochastic gravitational wave (GW) signal at future GW observatories, such as aLIGO, LISA and ET, that acts as another complementary probe of the ALPs, as well as of the PBH dark matter. …”
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    Article
  5. 85

    The stability of anisotropic compact stars influenced by dark matter under teleparallel gravity: an extended gravitational deformation approach by Sneha Pradhan, Piyali Bhar, Sanjay Mandal, P. K. Sahoo, Kazuharu Bamba

    Published 2025-02-01
    “…Abstract In our investigation, we pioneer the development of geometrically deformed strange stars within the framework of teleparallel gravity theory through gravitational decoupling via the complete geometric deformation (CGD) technique. …”
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    Article
  6. 86

    Mixture Ratio Design Optimization of Coal Gangue-Based Geopolymer Concrete Based on Modified Gravitational Search Algorithm by Daming Zhang, Fangjin Sun, Tiantian Liu, Zhonghao Xu

    Published 2021-01-01
    “…Therefore, chaotic map is introduced in the work here. Gravitational search algorithm was modified based on Chebyshev map in chaotic theory, and the modified equations were derived. …”
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    Article
  7. 87

    CνB Damping of Primordial Gravitational Waves and the Fine-Tuning of the CγB Temperature Anisotropy by A. E. Bernardini, J. F. G. Santos

    Published 2014-01-01
    “…Damping of primordial gravitational waves due to the anisotropic stress contribution owing to the cosmological neutrino background (CνB) is investigated in the context of a radiation-to-matter dominated universe. …”
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  8. 88

    Searching for dark torsion signatures at LIGO in Nieh–Yan teleparallel chiral gravitational waves and Chern–Simons invariants by L. C. Garcia de Andrade

    Published 2024-12-01
    “…Abstract Romano has recently found that frequency modulation of gravitational waves (GWs) could be used as a dark matter probe. …”
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  9. 89

    Periodic orbits and gravitational wave radiation in short hair black hole spacetimes for an extreme mass ratio system by Lai Zhao, Meirong Tang, Zhaoyi Xu

    Published 2025-01-01
    “…In addition, an increase in $$Q_m$$ Q m or a decrease in $$k$$ k will lead to a reduction in the period of gravitational waves and a significant enhancement of the signal amplitude. …”
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    Article
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    Reduced Gain and Shortened Time Constant of Vestibular Velocity Storage as a Source of Balance and Movement Sensitivities in Gravitational Insecurity by Michael Potegal, Teresa A. May-Benson, Sara Oxborough, Amy Hall, Stefanie McKnight

    Published 2022-01-01
    “…Gravitational insecurity (GrI) involves lifetime movement and balance concerns whose pathophysiological origins are unclear. …”
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  15. 95

    Bulk Viscous Bianchi Type VI0 Cosmological Model in the Self-creation Theory of Gravitation and in the General Theory of Relativity by E. A. Hegazy

    Published 2019-04-01
    “…In the second self-creation theory of gravitation and in the general theory of relativity, Bianchi type VI0 cosmological model in the presence of viscous fluid is studied. …”
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