Paleodetectors for Galactic supernova neutrinos
Abstract
Paleodetectors are a proposed experimental technique in which one would search for traces of recoiling nuclei in ancient minerals. Natural minerals on Earth are as old as $$\mathcal{O}$$(1) Gyr and, in many minerals, the damage tracks left by recoiling nuclei are also preserved for timescales long compared to 1 Gyr once created. Thus, even reading out relatively small target samples of order 100 g, paleodetectors would allow one to search for very rare events thanks to the large exposure, ϵ ~ 100 g Gyr = 105 t yr. Here, we explore the potential of paleodetectors to measure nuclear recoils induced by neutrinos from Galactic core collapse supernovae. We find that they would not only allow for a direct measurement of the average core collapse supernova rate in the Milky Way, but would also contain information about the time dependence of the local supernova rate over the past ~1 Gyr. Since the supernova rate is thought to be directly proportional to the star formation rate, such a measurement would provide a determination of the local star formation history. We investigate the sensitivity of paleodetectors to both a smooth time evolution and an enhancement of the core collapse supernova rate on relatively short timescales, as would be expected for a starburst period in the local group.
- Authors:
- Publication Date:
- Research Org.:
- Univ. of Michigan, Ann Arbor, MI (United States)
- Sponsoring Org.:
- Swedish Research Council (VR); USDOE Office of Science (SC); The Dutch Research Council (NWO)
- OSTI Identifier:
- 1618389
- Alternate Identifier(s):
- OSTI ID: 1801768
- Grant/Contract Number:
- SC007859; SC0007859; 638-2013-8993
- Resource Type:
- Published Article
- Journal Name:
- Physical Review D
- Additional Journal Information:
- Journal Name: Physical Review D Journal Volume: 101 Journal Issue: 10; Journal ID: ISSN 2470-0010
- Publisher:
- American Physical Society
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; Astronomy & Astrophysics; Physics
Citation Formats
Baum, Sebastian, Edwards, Thomas D. P., Kavanagh, Bradley J., Stengel, Patrick, Drukier, Andrzej K., Freese, Katherine, Górski, Maciej, and Weniger, Christoph. Paleodetectors for Galactic supernova neutrinos. United States: N. p., 2020.
Web. doi:10.1103/PhysRevD.101.103017.
Baum, Sebastian, Edwards, Thomas D. P., Kavanagh, Bradley J., Stengel, Patrick, Drukier, Andrzej K., Freese, Katherine, Górski, Maciej, & Weniger, Christoph. Paleodetectors for Galactic supernova neutrinos. United States. https://doi.org/10.1103/PhysRevD.101.103017
Baum, Sebastian, Edwards, Thomas D. P., Kavanagh, Bradley J., Stengel, Patrick, Drukier, Andrzej K., Freese, Katherine, Górski, Maciej, and Weniger, Christoph. Wed .
"Paleodetectors for Galactic supernova neutrinos". United States. https://doi.org/10.1103/PhysRevD.101.103017.
@article{osti_1618389,
title = {Paleodetectors for Galactic supernova neutrinos},
author = {Baum, Sebastian and Edwards, Thomas D. P. and Kavanagh, Bradley J. and Stengel, Patrick and Drukier, Andrzej K. and Freese, Katherine and Górski, Maciej and Weniger, Christoph},
abstractNote = {Paleodetectors are a proposed experimental technique in which one would search for traces of recoiling nuclei in ancient minerals. Natural minerals on Earth are as old as $\mathcal{O}$(1) Gyr and, in many minerals, the damage tracks left by recoiling nuclei are also preserved for timescales long compared to 1 Gyr once created. Thus, even reading out relatively small target samples of order 100 g, paleodetectors would allow one to search for very rare events thanks to the large exposure, ϵ ~ 100 g Gyr = 105 t yr. Here, we explore the potential of paleodetectors to measure nuclear recoils induced by neutrinos from Galactic core collapse supernovae. We find that they would not only allow for a direct measurement of the average core collapse supernova rate in the Milky Way, but would also contain information about the time dependence of the local supernova rate over the past ~1 Gyr. Since the supernova rate is thought to be directly proportional to the star formation rate, such a measurement would provide a determination of the local star formation history. We investigate the sensitivity of paleodetectors to both a smooth time evolution and an enhancement of the core collapse supernova rate on relatively short timescales, as would be expected for a starburst period in the local group.},
doi = {10.1103/PhysRevD.101.103017},
journal = {Physical Review D},
number = 10,
volume = 101,
place = {United States},
year = {Wed May 13 00:00:00 EDT 2020},
month = {Wed May 13 00:00:00 EDT 2020}
}
https://doi.org/10.1103/PhysRevD.101.103017
Web of Science
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Time-resolved 2-million-year-old supernova activity discovered in Earth’s microfossil record
journal, August 2016
- Ludwig, Peter; Bishop, Shawn; Egli, Ramon
- Proceedings of the National Academy of Sciences, Vol. 113, Issue 33