Gravitational Waves from a Core g Mode in Supernovae as Probes of the High-Density Equation of State.
- DOI
- 10.1103/physrevlett.131.191201
- Published
- 2023 Nov 10
- Container
- Physical review letters
- Publisher
- Not recorded
- Open access
- unknown
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BibTeX
@article{allodium:10.1103/physrevlett.131.191201,
title = {Gravitational Waves from a Core g Mode in Supernovae as Probes of the High-Density Equation of State.},
author = {Jakobus P and Müller B and Heger A and Zha S and Powell J and Motornenko A and Steinheimer J and Stöcker H},
year = {2023},
journal = {Physical review letters},
doi = {10.1103/physrevlett.131.191201},
url = {https://doi.org/10.1103/physrevlett.131.191201}
}RIS
TY - JOUR TI - Gravitational Waves from a Core g Mode in Supernovae as Probes of the High-Density Equation of State. AU - Jakobus P AU - Müller B AU - Heger A AU - Zha S AU - Powell J AU - Motornenko A AU - Steinheimer J AU - Stöcker H PY - 2023 JO - Physical review letters DO - 10.1103/physrevlett.131.191201 UR - https://doi.org/10.1103/physrevlett.131.191201 ER -
APA
P, J., B, M., A, H., S, Z., J, P., A, M., J, S., & H, S. (2023). Gravitational Waves from a Core g Mode in Supernovae as Probes of the High-Density Equation of State.. Physical review letters. https://doi.org/10.1103/physrevlett.131.191201
Source records
- pubmed · retrieved 2026-09-26T06:48:43.648Z