Boundary terms in cosmology
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arXiv
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| Autores principales: | , , |
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| Formato: | Preprint |
| Publicado: |
2025
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| _version_ | 1866915322105167872 |
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| author | Cuevas, Ángel Chagoya, Javier Ortiz, C. |
| author_facet | Cuevas, Ángel Chagoya, Javier Ortiz, C. |
| contents | In the derivation of the Einstein field equations via Hamilton's principle, the inclusion of a boundary term is essential to render the variational problem well-posed, as it addresses variations that do not vanish at the boundary of the spacetime manifold. Typically, this term is chosen as the Gibbons-Hawking-York boundary term. In this work, we propose an alternative treatment of the boundary term within a cosmological framework by employing the Lagrange multiplier method. This approach enforces the vanishing of the boundary term throughout the evolution of the Universe, leading to the prediction of a fluid component that decays as the sixth power of the scale factor. This type of fluid has been studied in the context of the early universe under the name of stiff matter, and it can be related to a scalar field known as kination. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2505_23679 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Boundary terms in cosmology Cuevas, Ángel Chagoya, Javier Ortiz, C. General Relativity and Quantum Cosmology High Energy Physics - Theory Mathematical Physics In the derivation of the Einstein field equations via Hamilton's principle, the inclusion of a boundary term is essential to render the variational problem well-posed, as it addresses variations that do not vanish at the boundary of the spacetime manifold. Typically, this term is chosen as the Gibbons-Hawking-York boundary term. In this work, we propose an alternative treatment of the boundary term within a cosmological framework by employing the Lagrange multiplier method. This approach enforces the vanishing of the boundary term throughout the evolution of the Universe, leading to the prediction of a fluid component that decays as the sixth power of the scale factor. This type of fluid has been studied in the context of the early universe under the name of stiff matter, and it can be related to a scalar field known as kination. |
| title | Boundary terms in cosmology |
| topic | General Relativity and Quantum Cosmology High Energy Physics - Theory Mathematical Physics |
| url | https://arxiv.org/abs/2505.23679 |