Quantum magnetic collapse of a partially bosonized npe-gas: Implications for astrophysical jets. (arXiv:1911.09147v1 [astro-ph.HE])
<a href="http://arxiv.org/find/astro-ph/1/au:+Felipe_R/0/1/0/all/0/1">R. Gonzalez Felipe</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Martinez_A/0/1/0/all/0/1">A. Perez Martınez</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Rojas_H/0/1/0/all/0/1">H. Perez Rojas</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Angulo_G/0/1/0/all/0/1">G. Quintero Angulo</a>
We study a possible mechanism for astrophysical jet production from a neutron
star composed by a partially bosonized npe-gas. We obtain that the expulsion of
a stable stream of matter might be triggered by the quantum magnetic collapse
of one or various components of the gas, while its collimation is due to the
formation of a strong self-generated magnetic field.
We study a possible mechanism for astrophysical jet production from a neutron
star composed by a partially bosonized npe-gas. We obtain that the expulsion of
a stable stream of matter might be triggered by the quantum magnetic collapse
of one or various components of the gas, while its collimation is due to the
formation of a strong self-generated magnetic field.
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