Convection, type II supernovae, and the early evolution of neutron stars

Adam Burrows; James M. Lattimer

doi:10.1016/0370-1573(88)90035-X

Convection, type II supernovae, and the early evolution of neutron stars

Adam Burrows, James M. Lattimer

Research output: Contribution to journal › Article › peer-review

47 Scopus citations

Abstract

We discuss some of the issues attending the study of the early evolution of neutron stars. In particular, the effect of convection during the protoneutron star stage is investigated. We conclude that convection not only affects a young neutron star's first seconds in interesting ways, but also that it makes the long-term mechanism for Type II supernova explosions more viable and energetic.

Original language	English (US)
Pages (from-to)	51-62
Number of pages	12
Journal	Physics Reports
Volume	163
Issue number	1-3
DOIs	https://doi.org/10.1016/0370-1573(88)90035-X
State	Published - Jun 1988
Externally published	Yes

All Science Journal Classification (ASJC) codes

General Physics and Astronomy

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10.1016/0370-1573(88)90035-X

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title = "Convection, type II supernovae, and the early evolution of neutron stars",

abstract = "We discuss some of the issues attending the study of the early evolution of neutron stars. In particular, the effect of convection during the protoneutron star stage is investigated. We conclude that convection not only affects a young neutron star's first seconds in interesting ways, but also that it makes the long-term mechanism for Type II supernova explosions more viable and energetic.",

author = "Adam Burrows and Lattimer, {James M.}",

note = "Funding Information: The authors would like to acknowledge the support of the Alfred P. Sloan Foundation. In addition, JML thanks the Dudley Foundation for a generous stipend. This work was supported in part by USDOE grant DE-AC02-80ER10719.",

year = "1988",

month = jun,

doi = "10.1016/0370-1573(88)90035-X",

language = "English (US)",

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pages = "51--62",

journal = "Physics Reports",

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T1 - Convection, type II supernovae, and the early evolution of neutron stars

AU - Burrows, Adam

AU - Lattimer, James M.

N1 - Funding Information: The authors would like to acknowledge the support of the Alfred P. Sloan Foundation. In addition, JML thanks the Dudley Foundation for a generous stipend. This work was supported in part by USDOE grant DE-AC02-80ER10719.

PY - 1988/6

Y1 - 1988/6

N2 - We discuss some of the issues attending the study of the early evolution of neutron stars. In particular, the effect of convection during the protoneutron star stage is investigated. We conclude that convection not only affects a young neutron star's first seconds in interesting ways, but also that it makes the long-term mechanism for Type II supernova explosions more viable and energetic.

AB - We discuss some of the issues attending the study of the early evolution of neutron stars. In particular, the effect of convection during the protoneutron star stage is investigated. We conclude that convection not only affects a young neutron star's first seconds in interesting ways, but also that it makes the long-term mechanism for Type II supernova explosions more viable and energetic.

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U2 - 10.1016/0370-1573(88)90035-X

DO - 10.1016/0370-1573(88)90035-X

M3 - Article

AN - SCOPUS:0012087341

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VL - 163

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EP - 62

JO - Physics Reports

JF - Physics Reports

IS - 1-3

ER -

Convection, type II supernovae, and the early evolution of neutron stars

Abstract

All Science Journal Classification (ASJC) codes

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