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Finsler spacetime in light of Segal's principle. / Dhasmana, S.; Silagadze, Z. K.

In: Modern Physics Letters A, Vol. 35, No. 6, 2050019, 28.02.2020.

Research output: Contribution to journal › Article › peer-review

Harvard

Dhasmana, S & Silagadze, ZK 2020, 'Finsler spacetime in light of Segal's principle', Modern Physics Letters A, vol. 35, no. 6, 2050019. https://doi.org/10.1142/S0217732320500194

APA

Dhasmana, S., & Silagadze, Z. K. (2020). Finsler spacetime in light of Segal's principle. Modern Physics Letters A, 35(6), [2050019]. https://doi.org/10.1142/S0217732320500194

Vancouver

Dhasmana S, Silagadze ZK. Finsler spacetime in light of Segal's principle. Modern Physics Letters A. 2020 Feb 28;35(6):2050019. doi: 10.1142/S0217732320500194

Author

Dhasmana, S. ; Silagadze, Z. K. / Finsler spacetime in light of Segal's principle. In: Modern Physics Letters A. 2020 ; Vol. 35, No. 6.

BibTeX

@article{f490a177c12c4b0eb66c19fa8e708456,
title = "Finsler spacetime in light of Segal's principle",
abstract = "ISIM(2) symmetry group of Cohen and Glashow's very special relativity is unstable with respect to small deformations of its underlying algebraic structure, and according to Segal's principle cannot be a true symmetry of nature. However, like special relativity, which is a very good description of nature, thanks to the smallness of the cosmological constant, which characterizes the deformation of the Poincar{\'e} group, the very special relativity can also be a very good approximation, thanks to the smallness of the dimensionless parameter characterizing the deformation of ISIM(2).",
keywords = "anisotropic spacetime, Finsler geometry, Segal's principle, Very special relativity, LORENTZ, DEFORMATIONS, RELATIVITY",
author = "S. Dhasmana and Silagadze, {Z. K.}",
year = "2020",
month = feb,
day = "28",
doi = "10.1142/S0217732320500194",
language = "English",
volume = "35",
journal = "Modern Physics Letters A",
issn = "0217-7323",
publisher = "World Scientific Publishing Co. Pte Ltd",
number = "6",

}

RIS

TY - JOUR

T1 - Finsler spacetime in light of Segal's principle

AU - Dhasmana, S.

AU - Silagadze, Z. K.

PY - 2020/2/28

Y1 - 2020/2/28

N2 - ISIM(2) symmetry group of Cohen and Glashow's very special relativity is unstable with respect to small deformations of its underlying algebraic structure, and according to Segal's principle cannot be a true symmetry of nature. However, like special relativity, which is a very good description of nature, thanks to the smallness of the cosmological constant, which characterizes the deformation of the Poincaré group, the very special relativity can also be a very good approximation, thanks to the smallness of the dimensionless parameter characterizing the deformation of ISIM(2).

AB - ISIM(2) symmetry group of Cohen and Glashow's very special relativity is unstable with respect to small deformations of its underlying algebraic structure, and according to Segal's principle cannot be a true symmetry of nature. However, like special relativity, which is a very good description of nature, thanks to the smallness of the cosmological constant, which characterizes the deformation of the Poincaré group, the very special relativity can also be a very good approximation, thanks to the smallness of the dimensionless parameter characterizing the deformation of ISIM(2).

KW - anisotropic spacetime

KW - Finsler geometry

KW - Segal's principle

KW - Very special relativity

KW - LORENTZ

KW - DEFORMATIONS

KW - RELATIVITY

UR - http://www.scopus.com/inward/record.url?scp=85074204932&partnerID=8YFLogxK

U2 - 10.1142/S0217732320500194

DO - 10.1142/S0217732320500194

M3 - Article

AN - SCOPUS:85074204932

VL - 35

JO - Modern Physics Letters A

JF - Modern Physics Letters A

SN - 0217-7323

IS - 6

M1 - 2050019

ER -

ID: 22035823