Addressing the missing matter problem in galaxies through a new fundamental gravitational radius
Само за регистроване кориснике
2017
Чланак у часопису (Објављена верзија)
Метаподаци
Приказ свих података о документуАпстракт
We demonstrate that the existence of a Noether symmetry in f theories of gravity gives rise to a further gravitational radius, besides tile standard Schwarzschild one, determining the dynamics at galactic scales. By this feature, it is possible to explain the baryonic Fully-Fisher relation and the rotation curve of gas-rich galaxies without the dark matter hypothesis.
Кључне речи:
modified gravity / rotation curves of galaxiesИзвор:
Journal of Cosmology and Astroparticle Physics, 2017, 6Финансирање / пројекти:
- Гравитација и структура космоса на великим скалама (RS-MESTD-Basic Research (BR or ON)-176003)
- INFN (iniziative specifiche TEONGRAV), INFN (QGSKY)
- Bilateral Cooperation [451-03-01231/2015-09/1]
- COST Actions [MP1304, CA15117]
DOI: 10.1088/1475-7516/2017/06/044
ISSN: 1475-7516
WoS: 000408310600014
Scopus: 2-s2.0-85021652997
Институција/група
VinčaTY - JOUR AU - Capozziello, Salvatore AU - Jovanović, Predrag AU - Borka Jovanović, Vesna AU - Borka, Duško PY - 2017 UR - https://vinar.vin.bg.ac.rs/handle/123456789/1696 AB - We demonstrate that the existence of a Noether symmetry in f theories of gravity gives rise to a further gravitational radius, besides tile standard Schwarzschild one, determining the dynamics at galactic scales. By this feature, it is possible to explain the baryonic Fully-Fisher relation and the rotation curve of gas-rich galaxies without the dark matter hypothesis. T2 - Journal of Cosmology and Astroparticle Physics T1 - Addressing the missing matter problem in galaxies through a new fundamental gravitational radius IS - 6 DO - 10.1088/1475-7516/2017/06/044 ER -
@article{ author = "Capozziello, Salvatore and Jovanović, Predrag and Borka Jovanović, Vesna and Borka, Duško", year = "2017", abstract = "We demonstrate that the existence of a Noether symmetry in f theories of gravity gives rise to a further gravitational radius, besides tile standard Schwarzschild one, determining the dynamics at galactic scales. By this feature, it is possible to explain the baryonic Fully-Fisher relation and the rotation curve of gas-rich galaxies without the dark matter hypothesis.", journal = "Journal of Cosmology and Astroparticle Physics", title = "Addressing the missing matter problem in galaxies through a new fundamental gravitational radius", number = "6", doi = "10.1088/1475-7516/2017/06/044" }
Capozziello, S., Jovanović, P., Borka Jovanović, V.,& Borka, D.. (2017). Addressing the missing matter problem in galaxies through a new fundamental gravitational radius. in Journal of Cosmology and Astroparticle Physics(6). https://doi.org/10.1088/1475-7516/2017/06/044
Capozziello S, Jovanović P, Borka Jovanović V, Borka D. Addressing the missing matter problem in galaxies through a new fundamental gravitational radius. in Journal of Cosmology and Astroparticle Physics. 2017;(6). doi:10.1088/1475-7516/2017/06/044 .
Capozziello, Salvatore, Jovanović, Predrag, Borka Jovanović, Vesna, Borka, Duško, "Addressing the missing matter problem in galaxies through a new fundamental gravitational radius" in Journal of Cosmology and Astroparticle Physics, no. 6 (2017), https://doi.org/10.1088/1475-7516/2017/06/044 . .