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  1. 61

    A Universal Description of Pseudorapidity Distributions in Both Nucleus-Nucleus and p-p Collisions at Currently Available Energies by Z. J. Jiang, H. P. Deng, Y. Huang

    Published 2016-01-01
    “…The investigations of present paper show that this part of charged particles together with leading particles, which, by conventional definition, carry on the quantum numbers of colliding nucleons and take away the most part of incident energy, can give a proper universal description to the pseudorapidity distributions of charged particles measured in both nucleus-nucleus and p-p collisions at currently available energies.…”
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  2. 62

    Axion-like relics: new constraints from old comagnetometer data by Itay M. Bloch, Yonit Hochberg, Eric Kuflik, Tomer Volansky

    Published 2020-01-01
    “…Future planned improvements of comagnetometer measurements through altered geometry, constituent content and data analysis techniques could enhance the sensitivity to axion-like relics coupled to nucleons or electrons by many orders of magnitude.…”
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  3. 63

    Magnetic Hexadecapole γ Transitions and Neutrino-Nuclear Responses in Medium-Heavy Nuclei by Lotta Jokiniemi, Jouni Suhonen, Hiroyasu Ejiri

    Published 2016-01-01
    “…The M4 NMEs are reduced a little by the quasiparticle-phonon correlations of the MQPM wave functions but mainly by other nucleonic and nonnucleonic correlations which are not explicitly included in the MQPM. …”
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  4. 64

    Background-induced forces from dark relics by Sergio Barbosa, Sylvain Fichet

    Published 2025-01-01
    “…Abstract Light particles quadratically coupled to nucleons induce macroscopic forces in matter. While a quantum effect always exists, an additional force occurs in the presence of a finite density of the light particles. …”
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  5. 65

    Black Hole Supernovae, Their Equation of State Dependence, and Ejecta Composition by Oliver Eggenberger Andersen, Evan O’Connor, Haakon Andresen, André da Silva Schneider, Sean M. Couch

    Published 2025-01-01
    “…We employ Skyrme-type equations of state (EOSs) and vary the uncertain nucleonic effective mass, which affects the pressure inside the proto–neutron star through the thermal part of the EOS. …”
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