Istituto Nazionale di Fisica Nucleare (INFN)

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Istituto Nazionale di Fisica Nucleare (INFN)

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Velocity distribution of elliptical galaxies in the framework of Non-local Gravity model

Borka, Duško; Borka Jovanović, Vesna; Capozziello, Salvatore; Jovanović, Predrag

(2022)

TY  - JOUR
AU  - Borka, Duško
AU  - Borka Jovanović, Vesna
AU  - Capozziello, Salvatore
AU  - Jovanović, Predrag
PY  - 2022
UR  - https://vinar.vin.bg.ac.rs/handle/123456789/10420
AB  - We investigate the velocity distribution of elliptical galaxies in the framework of Non-local Gravity. According to this approach, it is possible to recover the fundamental plane of elliptical galaxies without the dark matter hypothesis. Specifically, we compare theoretical predictions for circular velocity in Non-local Gravity context with the corresponding values coming from a large sample of observed elliptical galaxies. We adopt the surface brightness, effective radius and velocity dispersion as structural parameters for the fundamental plane. As final result, it is possible to show that non-local gravity effects can reproduce the stellar dynamics in elliptical galaxies and fit consistently observational data.
T2  - Advances in Space Research
T1  - Velocity distribution of elliptical galaxies in the framework of Non-local Gravity model
VL  - 71
IS  - 2
SP  - 1235
EP  - 1244
DO  - 10.1016/j.asr.2022.08.060
ER  - 
@article{
author = "Borka, Duško and Borka Jovanović, Vesna and Capozziello, Salvatore and Jovanović, Predrag",
year = "2022",
abstract = "We investigate the velocity distribution of elliptical galaxies in the framework of Non-local Gravity. According to this approach, it is possible to recover the fundamental plane of elliptical galaxies without the dark matter hypothesis. Specifically, we compare theoretical predictions for circular velocity in Non-local Gravity context with the corresponding values coming from a large sample of observed elliptical galaxies. We adopt the surface brightness, effective radius and velocity dispersion as structural parameters for the fundamental plane. As final result, it is possible to show that non-local gravity effects can reproduce the stellar dynamics in elliptical galaxies and fit consistently observational data.",
journal = "Advances in Space Research",
title = "Velocity distribution of elliptical galaxies in the framework of Non-local Gravity model",
volume = "71",
number = "2",
pages = "1235-1244",
doi = "10.1016/j.asr.2022.08.060"
}
Borka, D., Borka Jovanović, V., Capozziello, S.,& Jovanović, P.. (2022). Velocity distribution of elliptical galaxies in the framework of Non-local Gravity model. in Advances in Space Research, 71(2), 1235-1244.
https://doi.org/10.1016/j.asr.2022.08.060
Borka D, Borka Jovanović V, Capozziello S, Jovanović P. Velocity distribution of elliptical galaxies in the framework of Non-local Gravity model. in Advances in Space Research. 2022;71(2):1235-1244.
doi:10.1016/j.asr.2022.08.060 .
Borka, Duško, Borka Jovanović, Vesna, Capozziello, Salvatore, Jovanović, Predrag, "Velocity distribution of elliptical galaxies in the framework of Non-local Gravity model" in Advances in Space Research, 71, no. 2 (2022):1235-1244,
https://doi.org/10.1016/j.asr.2022.08.060 . .
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