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  2. Nuclear matter - Wikipedia

    en.wikipedia.org/wiki/Nuclear_matter

    [9] [10] In a neutron star, pressure rises from zero (at the surface) to an unknown large value in the center. Methods capable of treating finite regions have been applied to stars and to atomic nuclei. [11] [12] One such model for finite nuclei is the liquid drop model, which includes surface effects and Coulomb interactions.

  3. Neutron star - Wikipedia

    en.wikipedia.org/wiki/Neutron_star

    In neutron stars, the neutron drip is the transition point where nuclei become so neutron-rich that they can no longer hold additional neutrons, leading to a sea of free neutrons being formed. The sea of neutrons formed after neutron drip provides additional pressure support, which helps maintain the star's structural integrity and prevents ...

  4. Urca process - Wikipedia

    en.wikipedia.org/wiki/Urca_process

    In astroparticle physics, an Urca process is a reaction which emits a neutrino and which is assumed to take part in cooling processes in neutron stars and white dwarfs.The process was first discussed by George Gamow and Mário Schenberg while they were visiting a casino named Cassino da Urca in Urca, Rio de Janeiro.

  5. Neutron Star Interior Composition Explorer - Wikipedia

    en.wikipedia.org/wiki/Neutron_star_Interior...

    The Neutron Star Interior Composition ExploreR (NICER) is a NASA telescope on the International Space Station, designed and dedicated to the study of the extraordinary gravitational, electromagnetic, and nuclear physics environments embodied by neutron stars, exploring the exotic states of matter where density and pressure are higher than in atomic nuclei.

  6. Scientists reveal source of mysterious radio signal that ...

    www.aol.com/scientists-reveal-source-mysterious...

    A mysterious radio blast from space detected in 2022 originated in the magnetic field of an ultra-dense neutron star 200 million light years away.. Known as fast radio bursts, or FRB, such brief ...

  7. Nuclear astrophysics - Wikipedia

    en.wikipedia.org/wiki/Nuclear_astrophysics

    Nuclear physics experiments address stability (i.e., lifetimes and masses) for atomic nuclei well beyond the regime of stable nuclides into the realm of radioactive/unstable nuclei, almost to the limits of bound nuclei (the drip lines), and under high density (up to neutron star matter) and high temperature (plasma temperatures up to 10 9 K ...

  8. Gravitational collapse - Wikipedia

    en.wikipedia.org/wiki/Gravitational_collapse

    Neutron stars are expected to have a skin or "atmosphere" of normal matter on the order of a millimeter thick, underneath which they are composed almost entirely of closely packed neutrons called neutron matter [5] with a slight dusting of free electrons and protons mixed in. This degenerate neutron matter has a density of about 6.65 × 10 17 ...

  9. QCD matter - Wikipedia

    en.wikipedia.org/wiki/QCD_matter

    Compact stars (neutron stars). A neutron star is much cooler than 10 12 K, but gravitational collapse has compressed it to such high densities, that it is reasonable to surmise that quark matter may exist in the core. [6] Compact stars composed mostly or entirely of quark matter are called quark stars or strange stars.

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