ACOUSTIC WAVE GENERATION IN COLLAPSING MASSIVE STARS WITH CONVECTIVE SHELLS

dc.contributor.authorAbdikamalov, Ernazar
dc.contributor.authorFoglizzo, Thierry
dc.date.accessioned2022-07-05T04:15:46Z
dc.date.available2022-07-05T04:15:46Z
dc.date.issued2020
dc.description.abstractThe convection that takes place in the innermost shells of massive stars plays an important role in the formation of core-collapse supernova explosions. Upon encountering the supernova shock, additional turbulence is generated, amplifying the explosion. In this work, we study how the convective perturbations evolve during the stellar collapse. Our main aim is to establish their physical properties right before they reach the supernova shock. To this end, we solve the linearized hydrodynamics equations perturbed on a stationary background flow. The latter is approximated by the spherical transonic Bondi accretion, while the convective perturbations are modelled as a combination of entropy and vorticity waves. We follow their evolution from large radii, where convective shells are initially located, down to small radii, where they are expected to encounter the accretion shock above the proto-neutron star. Considering typical vorticity perturbations with a Mach number ∼0.1 and entropy perturbations with magnitude ∼0.05kb/baryon, we find that the advection of these perturbations down to the shock generates acoustic waves with a relative amplitude δp/γ p 10 per cent, in agreement with published numerical simulations. The velocity perturbations consist of contributions from acoustic and vorticity waves with values reaching ∼10 per cent of the sound speed ahead of the shock. The perturbation amplitudes decrease with increasing and initial radii of the convective shellsen_US
dc.identifier.citationAbdikamalov, E., & Foglizzo, T. (2020). Acoustic wave generation in collapsing massive stars with convective shells. Monthly Notices of the Royal Astronomical Society, 493(3), 3496–3512. https://doi.org/10.1093/mnras/staa533en_US
dc.identifier.urihttp://nur.nu.edu.kz/handle/123456789/6364
dc.language.isoenen_US
dc.publisherMonthly Notices of the Royal Astronomical Societyen_US
dc.rightsAttribution-NonCommercial-ShareAlike 3.0 United States*
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/3.0/us/*
dc.subjectType of access: Open Accessen_US
dc.subjecthydrodynamicsen_US
dc.subjectInstabilitiesen_US
dc.subjectshock wavesen_US
dc.titleACOUSTIC WAVE GENERATION IN COLLAPSING MASSIVE STARS WITH CONVECTIVE SHELLSen_US
dc.typeArticleen_US
workflow.import.sourcescience

Files

Original bundle
Now showing 1 - 1 of 1
Loading...
Thumbnail Image
Name:
staa533.pdf
Size:
961.56 KB
Format:
Adobe Portable Document Format
Description:
article
License bundle
Now showing 1 - 1 of 1
No Thumbnail Available
Name:
license.txt
Size:
6.28 KB
Format:
Item-specific license agreed upon to submission
Description:

Collections