Showing 1 - 20 results of 49 for search '"neutron star"', query time: 0.07s Refine Results
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    Physical Environment of Accreting Neutron Stars by J. Wang

    Published 2016-01-01
    “…Neutron stars (NSs) powered by accretion, which are known as accretion-powered NSs, always are located in binary systems and manifest themselves as X-ray sources. …”
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    Analyzing the speed of sound in neutron star with machine learning by Sagnik Chatterjee, Harsha Sudhakaran, Ritam Mallick

    Published 2024-12-01
    “…It has a negative trough beyond the maximal central densities of neutron stars. The change in sign of the trace anomaly hints towards a near-conformal matter at the centre of neutron stars, which may not necessarily be conformal quark matter.…”
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    GRB 130603B: No Compelling Evidence for Neutron Star Merger by Shlomo Dado, Arnon Dar

    Published 2015-01-01
    “…Moreover, SHB plus a kilonova can be produced also by the collapse of a compact star (neutron star, strange star, or quark star) to a more compact object due to cooling, loss of angular momentum, or mass accretion.…”
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    Analysis of the Conformally Flat Approximation for Binary Neutron Star Initial Conditions by In-Saeng Suh, Grant J. Mathews, J. Reese Haywood, N. Q. Lan

    Published 2017-01-01
    “…The spatially conformally flat approximation (CFA) is a viable method to deduce initial conditions for the subsequent evolution of binary neutron stars employing the full Einstein equations. …”
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    Constraining the equation of state in neutron-star cores via the long-ringdown signal by Christian Ecker, Tyler Gorda, Aleksi Kurkela, Luciano Rezzolla

    Published 2025-02-01
    “…Abstract Multimessenger signals from binary neutron star (BNS) mergers are promising tools to infer the properties of nuclear matter at densities inaccessible to laboratory experiments. …”
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    Neutron stars in extended scalar-Gauss–Bonnet gravity: the richness of the solution spectrum by Kalin V. Staykov, Peter Y. Yordanov, Daniela D. Doneva, Stoytcho S. Yazadjiev

    Published 2024-12-01
    “…Abstract Neutron stars are natural laboratories for testing gravity in the strong field regime. …”
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    Nucleonic Direct Urca Processes and Cooling of the Massive Neutron Star by Antikaon Condensations by Yan Xu, Wen Bo Ding, Cheng Zhi Liu, J. L. Han

    Published 2020-01-01
    “…Nucleonic direct Urca processes and cooling of the massive neutron stars are studied by considering antikaon condensations. …”
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    On Possible Reduction of Equilibrium Radius of a Neutron Star Influenced by Superstrong Magnetic Field by Vladimir V. Skobelev

    Published 2012-01-01
    “…Based on this, it is shown that, in superstrong magnetic field, equilibrium radius of a neutron star is approximately several times smaller than without the field influence. …”
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    X-ray pulsed light curves of highly compact neutron stars as probes of scalar–tensor theories of gravity by Tulio Ottoni, Jaziel G. Coelho, Rafael C. R. de Lima, Jonas P. Pereira, Jorge A. Rueda

    Published 2024-12-01
    “…Abstract The strong gravitational potential of neutron stars (NSs) makes them ideal astrophysical objects for testing extreme gravity phenomena. …”
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