Skip to main content
SpringerLink
Log in

Multigroup Simulation of Protoneutron Star Cooling

  • Conference paper
Supernovae

Part of the book series: Santa Cruz Summer Workshops in Astronomy and Astrophysics ((SANTA CRUZ))

Abstract

As well known, the data of the neutrino burst from SN1987A observed by KAMI-OKANDE-II and 1MB show good agreement with the theoretical model of protoneutron star cooling developed by mainly BURROWS and LATTIMER[1]. Although they used the energy-integrated scheme for neutrino transfer, it is not very insufficient because of the small statistics of the data as for SN1987A. But situations would be changed when the neutrino burst from the next Galactic supernova is detected by the future experiment such as SUPERKAMIOKANDE. Since several thousands of events will be detected, we can analyze the neutrino spectrum. That means multi-group simulation of the protoneutron star cooling is required to get useful information about equation of state of high density matter, supernova mechanism, neutrino interaction and so on. This is one of the main reasons why we are doing multigroup simulation of the protoneutron star cooling.

This is a preview of subscription content, log in via an institution to check access.

Access this chapter

Log in via an institution
Chapter
USD 29.95
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
eBook
USD 84.99
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book
USD 109.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Purchases are for personal use only

Institutional subscriptions

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

  1. A. Burrows and J. M. Lattimer, Ap. J. 307, 178 (1986).

    Article  ADS  Google Scholar 

  2. S. W. Bruenn, Ap. J. Suppl. 58, 771 (1985).

    Article  ADS  Google Scholar 

  3. J. R. Wilson and R. W. Mayle, preprint (1988), and private communications.

    Google Scholar 

  4. R. W. Mayle, J. R. Wilson and D. N. Schramm, Ap. J. 318, 288 (1987).

    Article  ADS  Google Scholar 

  5. A. Burrows, Ap. J. 334, 891 (1988).

    Article  ADS  Google Scholar 

Download references

Authors
  1. Hideyuki Suzuki
    View author publications

    You can also search for this author in PubMed Google Scholar

  2. Katsuhiko Sato
    View author publications

    You can also search for this author in PubMed Google Scholar

Editor information

Editors and Affiliations

  1. Lick Observatory, University of California, 95064, Santa Cruz, CA, USA

    S. E. Woosley

Rights and permissions

Reprints and permissions

Copyright information

© 1991 Springer-Verlag New York, Inc.

About this paper

Cite this paper

Suzuki, H., Sato, K. (1991). Multigroup Simulation of Protoneutron Star Cooling. In: Woosley, S.E. (eds) Supernovae. Santa Cruz Summer Workshops in Astronomy and Astrophysics. Springer, New York, NY. https://doi.org/10.1007/978-1-4612-2988-9_45

Download citation

  • DOI: https://doi.org/10.1007/978-1-4612-2988-9_45

  • Publisher Name: Springer, New York, NY

  • Print ISBN: 978-1-4612-7748-4

  • Online ISBN: 978-1-4612-2988-9

  • eBook Packages: Springer Book Archive

Publish with us

Policies and ethics

Search

Navigation