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Radial acceleration relation and dissipative dark matter. / Chashchina, Olga; Foot, Robert; Silagadze, Zurab.

In: Physical Review D, Vol. 95, No. 2, 023009, 30.01.2017.

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

Harvard

Chashchina, O, Foot, R & Silagadze, Z 2017, 'Radial acceleration relation and dissipative dark matter', Physical Review D, vol. 95, no. 2, 023009. https://doi.org/10.1103/PhysRevD.95.023009

APA

Chashchina, O., Foot, R., & Silagadze, Z. (2017). Radial acceleration relation and dissipative dark matter. Physical Review D, 95(2), [023009]. https://doi.org/10.1103/PhysRevD.95.023009

Vancouver

Chashchina O, Foot R, Silagadze Z. Radial acceleration relation and dissipative dark matter. Physical Review D. 2017 Jan 30;95(2):023009. doi: 10.1103/PhysRevD.95.023009

Author

Chashchina, Olga ; Foot, Robert ; Silagadze, Zurab. / Radial acceleration relation and dissipative dark matter. In: Physical Review D. 2017 ; Vol. 95, No. 2.

BibTeX

@article{6b4591e488e246d59afbd1ac781f5313,
title = "Radial acceleration relation and dissipative dark matter",
abstract = "Observations indicate that ordinary matter, the baryons, influence the structural properties of dark matter on galactic scales. One such indication is the radial acceleration relation, which is a tight correlation between the measured gravitational acceleration and that expected from the baryons. We show here that the dark matter density profile that has been motivated by dissipative dark matter models, including mirror dark matter, can reproduce this radial acceleration relation.",
keywords = "SPIRAL GALAXIES, ROTATION CURVES, SURFACE BRIGHTNESS, DISC GALAXIES, MASS MODELS, STELLAR, HALOES",
author = "Olga Chashchina and Robert Foot and Zurab Silagadze",
year = "2017",
month = jan,
day = "30",
doi = "10.1103/PhysRevD.95.023009",
language = "English",
volume = "95",
journal = "Physical Review D",
issn = "2470-0010",
publisher = "AMER PHYSICAL SOC",
number = "2",

}

RIS

TY - JOUR

T1 - Radial acceleration relation and dissipative dark matter

AU - Chashchina, Olga

AU - Foot, Robert

AU - Silagadze, Zurab

PY - 2017/1/30

Y1 - 2017/1/30

N2 - Observations indicate that ordinary matter, the baryons, influence the structural properties of dark matter on galactic scales. One such indication is the radial acceleration relation, which is a tight correlation between the measured gravitational acceleration and that expected from the baryons. We show here that the dark matter density profile that has been motivated by dissipative dark matter models, including mirror dark matter, can reproduce this radial acceleration relation.

AB - Observations indicate that ordinary matter, the baryons, influence the structural properties of dark matter on galactic scales. One such indication is the radial acceleration relation, which is a tight correlation between the measured gravitational acceleration and that expected from the baryons. We show here that the dark matter density profile that has been motivated by dissipative dark matter models, including mirror dark matter, can reproduce this radial acceleration relation.

KW - SPIRAL GALAXIES

KW - ROTATION CURVES

KW - SURFACE BRIGHTNESS

KW - DISC GALAXIES

KW - MASS MODELS

KW - STELLAR

KW - HALOES

UR - http://www.scopus.com/inward/record.url?scp=85021693647&partnerID=8YFLogxK

U2 - 10.1103/PhysRevD.95.023009

DO - 10.1103/PhysRevD.95.023009

M3 - Article

AN - SCOPUS:85021693647

VL - 95

JO - Physical Review D

JF - Physical Review D

SN - 2470-0010

IS - 2

M1 - 023009

ER -

ID: 10097925