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      Magnetic neutron star cooling and microphysics

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      Astronomy & Astrophysics
      EDP Sciences

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          An accurate nucleon-nucleon potential with charge-independence breaking

          We present a new high-quality nucleon-nucleon potential with explicit charge dependence and charge asymmetry, which we designate Argonne \(v_{18}\). The model has a charge-independent part with fourteen operator components that is an updated version of the Argonne \(v_{14}\) potential. Three additional charge-dependent and one charge-asymmetric operators are added, along with a complete electromagnetic interaction. The potential has been fit directly to the Nijmegen \(pp\) and \(np\) scattering data base, low-energy \(nn\) scattering parameters, and deuteron binding energy. With 40 adjustable parameters it gives a \(\chi^{2}\) per datum of 1.09 for 4301 \(pp\) and \(np\) data in the range 0--350 MeV.
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            Direct URCA process in neutron stars.

            (1991)
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              Electron Radiative Transitions in a Coulomb Field.

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                Author and article information

                Journal
                Astronomy & Astrophysics
                A&A
                EDP Sciences
                0004-6361
                1432-0746
                January 2018
                January 10 2018
                January 2018
                : 609
                : A74
                Article
                10.1051/0004-6361/201731866
                3eac45cf-9356-490b-a12d-0f716393d457
                © 2018
                History

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