INDUCED ROTATION IN THREE-DIMENSIONAL SIMULATIONS OF CORE-COLLAPSE SUPERNOVAE: IMPLICATIONS FOR PULSAR SPINS

Journal Article · Sun May 01 04:00:00 EDT 2011 · Astrophysical Journal

DOI:https://doi.org/10.1088/0004-637X/732/1/57· OSTI ID:21574631

Rantsiou, Emmanouela; Burrows, Adam; Nordhaus, Jason ^[1]; Almgren, Ann ^[2]

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1. Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544 (United States)
2. Computational Research Division, Lawrence Berkeley National Lab, Berkeley, CA 94720 (United States)

It has been suggested that the observed rotation periods of radio pulsars might be induced by a non-axisymmetric spiral-mode instability in the turbulent region behind the stalled supernova bounce shock, even if the progenitor core was not initially rotating. In this paper, using the three-dimensional Adaptive Mesh Refinement code CASTRO with a realistic progenitor and equation of state and a simple neutrino heating and cooling scheme, we present a numerical study of the evolution in three dimensions of the rotational profile of a supernova core from collapse, through bounce and shock stagnation, to delayed explosion. By the end of our simulation ({approx}420 ms after core bounce), we do not witness significant spin-up of the proto-neutron star core left behind. However, we do see the development before the explosion of strong differential rotation in the turbulent gain region between the core and stalled shock. Shells in this region acquire high spin rates that reach {approx}150 Hz, but this region contains too little mass and angular momentum to translate, even if left behind, into rapid rotation for the full neutron star. We also find that much of the induced angular momentum is likely to be ejected in the explosion, and moreover that even if the optimal amount of induced angular momentum is retained in the core, the resulting spin period is likely to be quite modest. Nevertheless, induced periods of seconds are possible.

• OSTI ID: 21574631
• Journal Information: Astrophysical Journal, Journal Name: Astrophysical Journal Journal Issue: 1 Vol. 732; ISSN ASJOAB; ISSN 0004-637X
• Country of Publication: United States
• Language: English

Related Subjects

79 ASTRONOMY AND ASTROPHYSICS
ANGULAR MOMENTUM
BINARY STARS
COOLING
COSMIC RADIO SOURCES
ELEMENTARY PARTICLES
EQUATIONS
EQUATIONS OF STATE
ERUPTIVE VARIABLE STARS
EVOLUTION
FERMIONS
FLUID MECHANICS
HEATING
HYDRODYNAMICS
LEPTONS
MASSLESS PARTICLES
MATHEMATICS
MECHANICS
MOTION
NEUTRINOS
NEUTRON STARS
NUMERICAL ANALYSIS
PARTICLE PROPERTIES
PULSARS
ROTATION
SIMULATION
SPIN
STARS
SUPERNOVAE
THREE-DIMENSIONAL CALCULATIONS
VARIABLE STARS