Junction Conditions and Gravitational Collapse in Scalar-Tensor-Vector Gravity
Fuente:
arXiv
Guardado en:
| Autores principales: | , , |
|---|---|
| Formato: | Preprint |
| Publicado: |
2026
|
| Materias: | |
| Acceso en línea: | |
| Etiquetas: |
Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
|
| _version_ | 1866909052811870208 |
|---|---|
| author | Debnath, Debanjan Badal, Anant Bhattacharya, Kaushik |
| author_facet | Debnath, Debanjan Badal, Anant Bhattacharya, Kaushik |
| contents | We formulate the junction conditions for Scalar-Tensor-Vector Gravity (STVG/MOG), proposed by J.~W.~Moffat. Using these conditions, the theory of gravitational collapse is constructed. In the collapsing process, an interior Friedmann-Lemaître-Robertson-Walker (FLRW) spacetime with baryonic matter and dark energy is matched with an exterior static, spherically symmetric Reissner--Nordström (RN)-like spacetime through a shell that carries STVG-charge. Starting from the standard STVG action, we derive the junction conditions across a boundary that relate the values of the various field quantities and their derivatives across the matching surface. Using the matching conditions and the nature of the collapsing shell, it is shown that a gravitational collapse can proceed in the present situation, and one can have RN-like horizon formation in finite proper time. We present two simplified models of gravitational collapse in this article: one ends up as an extremal RN-like black hole, and the other tends to collapse towards a sub-extremal RN-like black hole, as observed by an asymptotic observer at an infinite distance away from the collapsing system. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2605_17615 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | Junction Conditions and Gravitational Collapse in Scalar-Tensor-Vector Gravity Debnath, Debanjan Badal, Anant Bhattacharya, Kaushik General Relativity and Quantum Cosmology We formulate the junction conditions for Scalar-Tensor-Vector Gravity (STVG/MOG), proposed by J.~W.~Moffat. Using these conditions, the theory of gravitational collapse is constructed. In the collapsing process, an interior Friedmann-Lemaître-Robertson-Walker (FLRW) spacetime with baryonic matter and dark energy is matched with an exterior static, spherically symmetric Reissner--Nordström (RN)-like spacetime through a shell that carries STVG-charge. Starting from the standard STVG action, we derive the junction conditions across a boundary that relate the values of the various field quantities and their derivatives across the matching surface. Using the matching conditions and the nature of the collapsing shell, it is shown that a gravitational collapse can proceed in the present situation, and one can have RN-like horizon formation in finite proper time. We present two simplified models of gravitational collapse in this article: one ends up as an extremal RN-like black hole, and the other tends to collapse towards a sub-extremal RN-like black hole, as observed by an asymptotic observer at an infinite distance away from the collapsing system. |
| title | Junction Conditions and Gravitational Collapse in Scalar-Tensor-Vector Gravity |
| topic | General Relativity and Quantum Cosmology |
| url | https://arxiv.org/abs/2605.17615 |