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M. E. Caplan

4 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author1
  • middle author2

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE2
  • nucl-th2
ORCID 0009-0006-2122-5606

identity via Semantic Scholar / OpenAlex

most citedDisordered nuclear pasta, magnetic field decay, and crust cooling in neutron stars

208 citations · 362 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.HE2016★ 17 cited

Nuclear pasta and supernova neutrinos at late times

C. J. Horowitz, D. K. Berry, M. E. Caplan +5

Nuclear pasta, with nucleons arranged into tubes, sheets, or other complex shapes, is expected in core collapse supernovae (SNe) at just below nuclear density. We calculate the add…

nucl-th2014★ 70 cited

Pasta Nucleosynthesis: Molecular dynamics simulations of nuclear statistical equilibrium

M. E. Caplan, A. S. Schneider, C. J. Horowitz +1

Background: Exotic non-spherical nuclear pasta shapes are expected in nuclear matter at just below saturation density because of competition between short range nuclear attraction…

astro-ph.HE2014★ 208 cited

Disordered nuclear pasta, magnetic field decay, and crust cooling in neutron stars

C. J. Horowitz, D. K. Berry, C. M. Briggs +3

Nuclear pasta, with non-spherical shapes, is expected near the base of the crust in neutron stars. Large scale molecular dynamics simulations of pasta show long lived topological d…

nucl-th2014★ 67 cited

Nuclear Waffles

A. S. Schneider, D. K. Berry, C. M. Briggs +2

The dense neutron-rich matter found in supernovae and neutron stars is expected to form complex nonuniform phases referred to as nuclear pasta. The pasta shapes depend on density,…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.