Skip to main content Accessibility help
×
Hostname: page-component-cd9895bd7-gxg78 Total loading time: 0 Render date: 2024-12-22T06:44:29.779Z Has data issue: false hasContentIssue false

23 - Large scale convection and the convective supernova mechanism

Published online by Cambridge University Press:  11 August 2009

S. A. Colgate
Affiliation:
MS 227, Los Alamos Nat. Lab, P.O. Box 1663, Los Alamos, NM 87545; [email protected]
M. E. Herant
Affiliation:
Boston University BME, 44 Cummington St., Boston, MA 02215.
Peter Höflich
Affiliation:
University of Texas, Austin
Pawan Kumar
Affiliation:
University of Texas, Austin
J. Craig Wheeler
Affiliation:
University of Texas, Austin
Get access

Summary

Abstract

It is a weird and unlikely circumstance that a collapse supernova (Type II) should explode. The peculiar mechanism that facilitates this explosion is the formation and preservation of large scale structures in a high entropy atmosphere residing on the surface of a nearly formed neutron star. The high entropy atmosphere is maintained by two sources: the gravitational energy of initial formation of the neutron star, released by diffusion and transport of neutrinos and secondly and possibly dominantly by the gravitational energy released at the suface by additional low entropy matter falling through to the neutron star surface. The preservation of this entropy contrast between up and down flows requires thermal isolation between the low entropy down flows and the high entropy up flows. This entropy contrast allows an efficient Carnot cycle to operate and thus allows the efficient conversion of thermal energy to mechanical, which in turn drives the explosion. The P-V diagram of various up and down going mass elements in the calculations demonstrates the existence of the cycle and its efficiency. Greater thermal isolation should occur in 3-D as opposed to 2-D calculations because of the difference in relative thickness or surface to mass ratio for the same mass flow in 2 and 3-D. This may explain the observed stronger explosion in 3-D calculations.

Prolog

This paper is written in honor of a long and lasting friendship between Craig Wheeler and the first author for more than half his current life.

Type
Chapter
Information
Cosmic Explosions in Three Dimensions
Asymmetries in Supernovae and Gamma-Ray Bursts
, pp. 199 - 208
Publisher: Cambridge University Press
Print publication year: 2004

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Bethe, H. A., 1990, Rev. of Mod. Phys., 62, 801CrossRef
Bethe, H. A., & Wilson, J. R. 1985 Ap J, 295, 14CrossRef
Colgate, S. A., Herant, M, and Benz, W. 1993, Physics Reports, 227, 157CrossRef
Colgate, S. A. & Fryer, C. L., 1994, Physics Reports, 256, 5CrossRef
Colgate, S. A. & Petschek, A. G. 1993, Advances in Cryogenic Engineering, CEC/ICMC39 Albuquerque, NM,
Fryer, C. L. & Warren, M. S., 2002 Ap. J. (Letters. 541, 1033 Mon. Not. R. astr. Soc., 196, 731–745CrossRef
Herant, M., Benz, W., Hix, W. R., Fryer, C., and Colgate, S. A., 1994, ApJ, 435, 339CrossRef
Herant, M., Benz, W., and Colgate, S. A. 1992, ApJ 395, 642CrossRef
Herant, M, Colgate, S. A., and Benz, W. 1996 LAScience
Rampp, M. & Janka, H.-Th 2002a, Ap. J. (Letters), 432, L119)
Rampp, M. & Janka, H.-Th 2002b, Astr. Ap., 396, 361

Save book to Kindle

To save this book to your Kindle, first ensure [email protected] is added to your Approved Personal Document E-mail List under your Personal Document Settings on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part of your Kindle email address below. Find out more about saving to your Kindle.

Note you can select to save to either the @free.kindle.com or @kindle.com variations. ‘@free.kindle.com’ emails are free but can only be saved to your device when it is connected to wi-fi. ‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.

Find out more about the Kindle Personal Document Service.

Available formats
×

Save book to Dropbox

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Dropbox.

Available formats
×

Save book to Google Drive

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Google Drive.

Available formats
×