Skip to main content

Neutrinos from Pair Instability Supernovae

  • Conference paper
  • First Online:
Nuclei in the Cosmos XV

Part of the book series: Springer Proceedings in Physics ((SPPHY,volume 219))

  • 783 Accesses

Abstract

We present the first ever calculations of the neutrino signal from pair-instability supernovae (PISNe) using two hydrodynamical simulations which bracket the mass range of the stars which explode via this mechanism. We take into account both the time and energy dependence of the emission and the flavor oscillations, as well as investigating the equation-of-state dependence. We then process the computed neutrino fluxes at Earth through four different neutrino detectors. We show how the neutrino signal from PISNe possesses unique features that distinguish it from other supernovae, how the detectors we consider are capable of observing neutrinos from PISNe at the standard distance of 10 kpc, and how the proposed HyperKamiokande detector can even reach the Large Magellanic Cloud and the several very high mass stars known to exist there.

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

Access this chapter

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 EPUB and 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
Hardcover Book
USD 109.99
Price excludes VAT (USA)
  • Durable hardcover 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

References

  1. A. Kozyreva, M. Gilmer, R. Hirschi et al., MNRAS 464, 2854 (2017). https://doi.org/10.1093/mnras/stw2562

    Article  ADS  Google Scholar 

  2. M.S. Gilmer, A. Kozyreva, R. Hirschi et al., ApJ 846, 100 (2017). https://doi.org/10.3847/1538-4357/aa8461

    Article  ADS  Google Scholar 

  3. N. Itoh, H. Hayashi, A. Nishikawa, Y. Kohyama, ApJ Supp. 102, 411 (1996). https://doi.org/10.1086/192264

    Article  ADS  Google Scholar 

  4. A.W. Steiner, M. Hempel, T. Fischer, ApJ 774, 17 (2013). https://doi.org/10.1088/0004-637X/774/1/17

    Article  ADS  Google Scholar 

  5. W.P. Wright, G. Nagaraj, J.P. Kneller et al., Phys. Rev. D 94(2), 025026 (2016). https://doi.org/10.1103/PhysRevD.94.025026

    Article  ADS  Google Scholar 

  6. W.P. Wright, J.P. Kneller, S.T. Ohlmann et al., Phys. Rev. D 95(4), 043006 (2017). https://doi.org/10.1103/PhysRevD.95.043006

    Article  ADS  Google Scholar 

  7. A. Mirizzi, I. Tamborra, H.T. Janka et al., Nuovo Cimento Rivista Serie, vol. 39, p. 1 (2016). https://doi.org/10.1393/ncr/i2016-10120-8

Download references

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to James P. Kneller .

Editor information

Editors and Affiliations

Rights and permissions

Reprints and permissions

Copyright information

© 2019 Springer Nature Switzerland AG

About this paper

Check for updates. Verify currency and authenticity via CrossMark

Cite this paper

Kneller, J.P., Fröhlich, C., Gilmer, M.S., Wright, W.P. (2019). Neutrinos from Pair Instability Supernovae. In: Formicola, A., Junker, M., Gialanella, L., Imbriani, G. (eds) Nuclei in the Cosmos XV. Springer Proceedings in Physics, vol 219. Springer, Cham. https://doi.org/10.1007/978-3-030-13876-9_25

Download citation

Publish with us

Policies and ethics