A Cosmological unicorn solution to Finsler gravity

Research output: Contribution to journalArticleResearchpeer review

Authors

  • Sjors Heefer
  • Christian Pfeifer
  • Antonio Reggio
  • Andrea Fuster

External Research Organisations

  • Eindhoven University of Technology (TU/e)
  • University of Bremen
View graph of relations

Details

Original languageEnglish
Article number064051
JournalPhysical Review D
Volume108
Issue number6
Publication statusPublished - 15 Sept 2023
Externally publishedYes

Abstract

We present a new family of exact vacuum solutions to Pfeifer and Wohlfarth's field equation in Finsler gravity, consisting of Finsler metrics that are Landsbergian but not Berwaldian, also known as unicorns due to their rarity. Interestingly, we find that these solutions have a physically viable light cone structure, even though in some cases the signature is not Lorentzian but positive definite. We furthermore find a promising analogy between our solutions and classical Friedmann-Lemaître-Robertson-Walker cosmology. One of our solutions, in particular, has cosmological symmetry, i.e., it is spatially homogeneous and isotropic, and it is additionally conformally flat, with the conformal factor depending only on the timelike coordinate. We show that this conformal factor can be interpreted as the scale factor, we compute it as a function of cosmological time, and we show that it corresponds to a linearly expanding (or contracting) Finsler universe.

ASJC Scopus subject areas

Cite this

A Cosmological unicorn solution to Finsler gravity. / Heefer, Sjors; Pfeifer, Christian; Reggio, Antonio et al.
In: Physical Review D, Vol. 108, No. 6, 064051, 15.09.2023.

Research output: Contribution to journalArticleResearchpeer review

Heefer, S, Pfeifer, C, Reggio, A & Fuster, A 2023, 'A Cosmological unicorn solution to Finsler gravity', Physical Review D, vol. 108, no. 6, 064051. https://doi.org/10.1103/PhysRevD.108.064051
Heefer, S., Pfeifer, C., Reggio, A., & Fuster, A. (2023). A Cosmological unicorn solution to Finsler gravity. Physical Review D, 108(6), Article 064051. https://doi.org/10.1103/PhysRevD.108.064051
Heefer S, Pfeifer C, Reggio A, Fuster A. A Cosmological unicorn solution to Finsler gravity. Physical Review D. 2023 Sept 15;108(6):064051. doi: 10.1103/PhysRevD.108.064051
Heefer, Sjors ; Pfeifer, Christian ; Reggio, Antonio et al. / A Cosmological unicorn solution to Finsler gravity. In: Physical Review D. 2023 ; Vol. 108, No. 6.
Download
@article{3ea9466c81554866a13840fcdd239ef5,
title = "A Cosmological unicorn solution to Finsler gravity",
abstract = "We present a new family of exact vacuum solutions to Pfeifer and Wohlfarth's field equation in Finsler gravity, consisting of Finsler metrics that are Landsbergian but not Berwaldian, also known as unicorns due to their rarity. Interestingly, we find that these solutions have a physically viable light cone structure, even though in some cases the signature is not Lorentzian but positive definite. We furthermore find a promising analogy between our solutions and classical Friedmann-Lema{\^i}tre-Robertson-Walker cosmology. One of our solutions, in particular, has cosmological symmetry, i.e., it is spatially homogeneous and isotropic, and it is additionally conformally flat, with the conformal factor depending only on the timelike coordinate. We show that this conformal factor can be interpreted as the scale factor, we compute it as a function of cosmological time, and we show that it corresponds to a linearly expanding (or contracting) Finsler universe.",
author = "Sjors Heefer and Christian Pfeifer and Antonio Reggio and Andrea Fuster",
note = "Funding information: C. P. was funded by the cluster of excellence Quantum Frontiers funded by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) under Germany{\textquoteright}s Excellence Strategy EXC-2123 QuantumFrontiers 390837967. The authors would like to acknowledge networking support by the COST Action CA18108.",
year = "2023",
month = sep,
day = "15",
doi = "10.1103/PhysRevD.108.064051",
language = "English",
volume = "108",
journal = "Physical Review D",
issn = "2470-0010",
publisher = "American Institute of Physics",
number = "6",

}

Download

TY - JOUR

T1 - A Cosmological unicorn solution to Finsler gravity

AU - Heefer, Sjors

AU - Pfeifer, Christian

AU - Reggio, Antonio

AU - Fuster, Andrea

N1 - Funding information: C. P. was funded by the cluster of excellence Quantum Frontiers funded by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) under Germany’s Excellence Strategy EXC-2123 QuantumFrontiers 390837967. The authors would like to acknowledge networking support by the COST Action CA18108.

PY - 2023/9/15

Y1 - 2023/9/15

N2 - We present a new family of exact vacuum solutions to Pfeifer and Wohlfarth's field equation in Finsler gravity, consisting of Finsler metrics that are Landsbergian but not Berwaldian, also known as unicorns due to their rarity. Interestingly, we find that these solutions have a physically viable light cone structure, even though in some cases the signature is not Lorentzian but positive definite. We furthermore find a promising analogy between our solutions and classical Friedmann-Lemaître-Robertson-Walker cosmology. One of our solutions, in particular, has cosmological symmetry, i.e., it is spatially homogeneous and isotropic, and it is additionally conformally flat, with the conformal factor depending only on the timelike coordinate. We show that this conformal factor can be interpreted as the scale factor, we compute it as a function of cosmological time, and we show that it corresponds to a linearly expanding (or contracting) Finsler universe.

AB - We present a new family of exact vacuum solutions to Pfeifer and Wohlfarth's field equation in Finsler gravity, consisting of Finsler metrics that are Landsbergian but not Berwaldian, also known as unicorns due to their rarity. Interestingly, we find that these solutions have a physically viable light cone structure, even though in some cases the signature is not Lorentzian but positive definite. We furthermore find a promising analogy between our solutions and classical Friedmann-Lemaître-Robertson-Walker cosmology. One of our solutions, in particular, has cosmological symmetry, i.e., it is spatially homogeneous and isotropic, and it is additionally conformally flat, with the conformal factor depending only on the timelike coordinate. We show that this conformal factor can be interpreted as the scale factor, we compute it as a function of cosmological time, and we show that it corresponds to a linearly expanding (or contracting) Finsler universe.

UR - http://www.scopus.com/inward/record.url?scp=85175019185&partnerID=8YFLogxK

U2 - 10.1103/PhysRevD.108.064051

DO - 10.1103/PhysRevD.108.064051

M3 - Article

AN - SCOPUS:85175019185

VL - 108

JO - Physical Review D

JF - Physical Review D

SN - 2470-0010

IS - 6

M1 - 064051

ER -