Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
Radial acceleration relation and dissipative dark matter. / Chashchina, Olga; Foot, Robert; Silagadze, Zurab.
в: Physical Review D, Том 95, № 2, 023009, 30.01.2017.Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
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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