TY - JOUR
T1 - Qualitative dynamics of interacting vacuum cosmologies
AU - Kaeonikhom, Chakkrit
AU - Rangdee, Phongsaphat
AU - Assadullahi, Hooshyar
AU - Gumjudpai, Burin
AU - Schewtschenko, Jascha A.
AU - Wands, David
N1 - 20 pages, 8 figures; version accepted for publication
PY - 2020/12/7
Y1 - 2020/12/7
N2 - We present a phase-space analysis of the qualitative dynamics cosmologies where dark matter exchanges energy with the vacuum component. We find fixed points corresponding to power-law solutions where the different components remain a constant fraction of the total energy density and given an existence condition for any fixed points with nonvanishing energy transfer. For some interaction models we find novel fixed points in the presence of a third noninteracting fluid with constant equation of state, such as radiation, where the interacting vacuum+matter tracks the evolution of the third fluid, analogous to tracker solutions previously found for self-interacting scalar fields. We illustrate the phase-plane behavior, determining the equation of state and stability of the fixed points in the case of a simple linear interaction model, for interacting vacuum and dark matter, including the presence of noninteracting radiation. We give approximate solutions for the equation of state in matter- or vacuum-dominated solutions in the case of small interaction parameters.
AB - We present a phase-space analysis of the qualitative dynamics cosmologies where dark matter exchanges energy with the vacuum component. We find fixed points corresponding to power-law solutions where the different components remain a constant fraction of the total energy density and given an existence condition for any fixed points with nonvanishing energy transfer. For some interaction models we find novel fixed points in the presence of a third noninteracting fluid with constant equation of state, such as radiation, where the interacting vacuum+matter tracks the evolution of the third fluid, analogous to tracker solutions previously found for self-interacting scalar fields. We illustrate the phase-plane behavior, determining the equation of state and stability of the fixed points in the case of a simple linear interaction model, for interacting vacuum and dark matter, including the presence of noninteracting radiation. We give approximate solutions for the equation of state in matter- or vacuum-dominated solutions in the case of small interaction parameters.
KW - cosmology
KW - dark energy
KW - RCUK
KW - STFC
KW - ST/S000550/1
UR - https://arxiv.org/abs/2007.12181
U2 - 10.1103/PhysRevD.102.123519
DO - 10.1103/PhysRevD.102.123519
M3 - Article
SN - 2470-0029
VL - 102
JO - Physical Review D - Particles, Fields, Gravitation and Cosmology
JF - Physical Review D - Particles, Fields, Gravitation and Cosmology
IS - 12
M1 - 123519
ER -