Hartle–Hawking state (Q958793)
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proposal concerning the state of the Universe prior to the Planck epoch, given by the path integral over all geometries that have a specified induced metric on their boundary
| Language | Label | Description | Also known as |
|---|---|---|---|
| English | Hartle–Hawking state |
proposal concerning the state of the Universe prior to the Planck epoch, given by the path integral over all geometries that have a specified induced metric on their boundary |
Statements
1983
0 references
![{\displaystyle \Psi [(M,h)]\propto \sum _{N}\int _{(\partial N,g\upharpoonright \partial N)=(M,h)}\mathrm {D} g\,\exp \left(-\int _{N}{\mathcal {L}}_{\text{EH}}[g]\right)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/e2aeb09f76b7058c5df8db18c06af9148f56a605)
0 references
Identifiers
Sitelinks
Wikipedia(11 entries)
- arwiki حالة هارتل-هوكينغ
- enwiki Hartle–Hawking state
- eswiki Estado de Hartle-Hawking
- fawiki حالت هارتل–هاوکینگ
- frwiki Modèle de Hartle-Hawking
- itwiki Stato di Hartle-Hawking
- jawiki ハートル＝ホーキングの境界条件
- kowiki 하틀-호킹 상태
- plwiki Model Hartle’a-Hawkinga
- ptwiki Estado de Hartle-Hawking
- trwiki Hartle-Hawking durumu