Item Infomation
Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Tuan Q. Do | - |
| dc.date.accessioned | 2020-10-13T04:29:20Z | - |
| dc.date.available | 2020-10-13T04:29:20Z | - |
| dc.date.issued | 2020 | - |
| dc.identifier.other | arXiv:2007.04867 | - |
| dc.identifier.uri | https://dlib.phenikaa-uni.edu.vn/handle/PNK/589 | - |
| dc.description.abstract | In this paper, we extend our investigation of the validity of the cosmic no-hair conjecture within non-canonical anisotropic inflation. As a result, we are able to figure out an exact Bianchi type I solution to a power-law {\it k}-inflation model in the presence of unusual coupling between scalar and electromagnetic fields as −f2(ϕ)FμνFμν/4. Furthermore, stability analysis based on the dynamical system method indicates that the obtained solution does admit stable and attractive hairs during an inflationary phase and therefore violates the cosmic no-hair conjecture. | vi |
| dc.language.iso | vi | vi |
| dc.subject | General Relativity and Quantum Cosmology | vi |
| dc.subject | Cosmology and Nongalactic Astrophysics | vi |
| dc.title | Stable small spatial hairs in a power-law k-inflation model | vi |
| dc.type | Article | vi |
| Appears in Collections | ||
| Bài báo khoa học | ||
Files in This Item:
