activity
19932026
most citedNeutron Star Structure and the Neutron Radius of 208Pb

871 citations · 11k across the 151 of their papers we have counts for

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Showing astro-ph.SRShow all

20 papers · 1 filter

astro-ph.SR2022★ 2 cited

Ignition of carbon burning from nuclear fission in compact stars

C. J. Horowitz

Type-Ia supernovae (SN Ia) are powerful stellar explosions that provide important distance indicators in cosmology. Recently, we proposed a new SN Ia mechanism that involves a nucl…

astro-ph.SR2021★ 1 cited

Nuclear fission reaction simulations in compact stars

Alex Deibel, M. E. Caplan, C. J. Horowitz

Type-Ia supernovae (SN Ia) are powerful stellar explosions that provide important distance indicators in cosmology. Recently, we proposed a new SN Ia mechanism that involves a nucl…

astro-ph.SR2021★ 22 cited

Cooling Delays from Iron Sedimentation and Iron Inner Cores in White Dwarfs

M. E. Caplan, I. F. Freeman, C. J. Horowitz +2

Do white dwarfs have inner cores made of iron? Neutron rich nuclei like Fe experience a net gravitational force and sediment toward the core. Using new phase diagrams and mo…

astro-ph.SR2021

Nuclear fission chain reaction in cooling white dwarf stars

C. J. Horowitz, M. E. Caplan

The first solids that form as a white dwarf (WD) starts to crystallize are expected to be greatly enriched in actinides. Previously [PRL 126, 1311010] we found that these solids mi…

astro-ph.SR2021★ 16 cited

Actinide crystallization and fission reactions in cooling white dwarf stars

C. J. Horowitz, M. E. Caplan

The first solids that form as a cooling white dwarf (WD) starts to crystallize are expected to be greatly enriched in actinides. This is because the melting points of WD matter sca…

astro-ph.SR2020★ 28 cited

Nuclear and dark matter heating in massive white dwarf stars

C. J. Horowitz

Recently, Cheng et al. identified a number of massive white dwarfs (WD) that appear to have an additional heat source providing a luminosity near for multi…