Kinetic coupled tachyon: A dynamical system analysis

被引:1
作者
Pace, Francesco [1 ,2 ,3 ]
Rozas-Fernandez, Alberto [4 ]
Turker, Ozgen Tunc [5 ]
机构
[1] Univ Torino, Dipartimento Fis, Via P Giuria 1, I-10125 Turin, Italy
[2] INFN, Sez Torino, Via P Giuria 1, I-10125 Turin, Italy
[3] INAF Ist Nazl Astrofis, Osservatorio Astrofis Torino, Str Osservatorio 20, I-10025 Pino Torinese, Italy
[4] Univ Lisbon, Inst Astrofis & Ciencias Espaco, OAL, PT-1349018 Lisbon, Portugal
[5] Univ Fed Espirito Santo, PPGCosmo, Ave Fernando Ferrari 514, BR-29075910 Vitoria, ES, Brazil
来源
PHYSICS OF THE DARK UNIVERSE | 2025年 / 47卷
关键词
Cosmology; Scalar field; Coupled tachyon; Dark energy; Phase-space analysis; COSMOLOGICAL CONSTANT; SCALAR FIELD; DARK-MATTER; ENERGY;
D O I
10.1016/j.dark.2024.101786
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present and examine a kinetically coupled tachyon dark energy model, where a tachyon scalar field cp interacts with the matter sector. More specifically, we deduce this cosmological setting from a generalised interacting dark energy model that allows for the kinetic term of the scalar field to couple to the matter species a priori in the action. A thorough dynamical system analysis and its cosmological implications unveil the appearance of a scaling solution which is also an attractor of the system, thanks to a novel critical point, with a period of accelerated expansion thereafter. This new solution, not present in the uncoupled case, has the enticing consequence of alleviating the coincidence problem.
引用
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页数:11
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