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Neutrino-“pasta” scattering: The opacity of nonuniform neutron-rich matter
Open accessAbstract
Neutron-rich matter at subnuclear densities may involve complex structures displaying a variety of shapes, such as spherical, slablike, and∕or rodlike shapes. These phases of the nuclear pasta are expected to exist in the crust of neutron stars and in core-collapse supernovae. The dynamics of core-collapse supernovae is very sensitive to the interactions between neutrinos and nucleons∕nuclei. Indeed, neutrino excitation of the low-energy modes of the pasta may allow for a significant energy transfer to the nuclear medium, thereby reviving the stalled supernovae shock. The linear response of the nuclear pasta to neutrinos is modeled via a simple semiclassical simulation. The transport mean free path for $\ensuremath{\mu}$ and $\ensuremath{\tau}$ neutrinos (and antineutrinos) is expressed in terms of the static structure factor of the pasta, which is evaluated using Metropolis Monte Carlo simulations.
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Cited by
Complexity in Strongly Correlated Electronic Systems
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A statistical model for a complete supernova equation of state
Hempel, M., & Schaffner-Bielich, J. (2010) · Nuclear Physics A · doi:10.1016/j.nuclphysa.2010.02.010 · Cited by 638
Metadata
- Authors
- Horowitz, C. J., Pérez-García, M. A., & Piekarewicz, J.
- Venue
- Physical Review C
- Publisher
- American Physical Society (APS)
- Published
- 2004-04-27
- Volume
- 69
- Issue
- 4
- ISSN
- 0556-2813 (ISSN-L)
- 1089-490X
- OpenAlex
- W1990059845
- Cited by
- 259
- References
- 15
- FWCI
- 6.77
- Type
- journal article
- Language
- en
- Open access
- green
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