Revisiting the dynamics of interacting vector-like dark energy

被引:6
作者
Rodriguez-Benites, Carlos [1 ,2 ,3 ]
Gonzalez-Espinoza, Manuel [4 ,5 ]
Otalora, Giovanni [6 ]
Alva-Morales, Manuel [2 ,3 ,7 ]
机构
[1] Univ Nacl Trujillo, Fac Ciencias Fis & Matemat, Dept Acad Fis, Ave Juan Pablo II s-n, Trujillo, Peru
[2] Univ Nacl Trujillo, Fac Ciencias Fis & Matemat, GRACOCC Res Grp, Ave Juan Pablo II s-n, Trujillo, Peru
[3] Univ Nacl Trujillo, Fac Ciencias Fis & Matemat, OASIS Res Grp, Ave Juan Pablo II s-n, Trujillo, Peru
[4] Univ Playa Ancha, Fac Ciencias Nat & Exactas, Dept Matemat Fis & Comp, Lab Comp Fis LCF UPLA, Subida Leopoldo Carvallo 270, Valparaiso, Chile
[5] Univ Playa Ancha, Fac Ciencias Nat & Exactas, Dept Matemat Fis & Comp, Lab Didact Fis, Subida Leopoldo Carvallo 270, Valparaiso, Chile
[6] Univ Tarapaca, Fac Ciencias, Dept Fis, Casilla 7-D, Arica, Chile
[7] Univ Nacl Trujillo, Escuela Profes Fis, Fac Ciencias Fis & Matemat, Ave Juan Pablo II s-n, Trujillo, Peru
来源
EUROPEAN PHYSICAL JOURNAL C | 2024年 / 84卷 / 03期
关键词
COSMOLOGICAL CONSTANT PROBLEM; OBSERVATIONAL H(Z) DATA; LUMINOUS RED GALAXIES; MODIFIED GRAVITY; INFLATION; MODELS; EXPANSION; UNIVERSE; DRIVEN; FIELD;
D O I
10.1140/epjc/s10052-024-12613-z
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We revise the dynamics of interacting vector-like dark energy, a theoretical framework proposed to explain the accelerated expansion of the universe. By investigating the interaction between vector-like dark energy and dark matter, we analyze its effects on the cosmic expansion history and the thermodynamics of the accelerating universe. Our results demonstrate that the presence of interaction significantly influences the evolution of vector-like dark energy, leading to distinct features in its equation of state and energy density. We compare our findings with observational data and highlight the importance of considering interactions in future cosmological studies.
引用
收藏
页数:18
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