The dark bubbleography

Souvik Banerjee (Institut für Theoretische Physik und Astrophysik, Julius-Maximilians-Universität Würzburg, Am Hubland, Würzburg, 97074, Germany) ; Ulf Danielsson (Institutionen för fysik och astronomi, Uppsala Universitet, Box 803, Uppsala, SE-751 08, Sweden) ; Maximilian Zemsch (Institut für Theoretische Physik und Astrophysik, Julius-Maximilians-Universität Würzburg, Am Hubland, Würzburg, 97074, Germany)

We present the holographic construction of the dark bubble model of dark energy and highlight the pivotal role played by the non-normalizable modes. Following the route of holographic renormalization, we show that the non-normalizable modes are essential for having a vanishing mass for the induced graviton in any braneworld model. We then apply this idea in the computation of the propagator on the wall of the dark bubble introduced in [1].

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      "value": "We present the holographic construction of the dark bubble model of dark energy and highlight the pivotal role played by the non-normalizable modes. Following the route of holographic renormalization, we show that the non-normalizable modes are essential for having a vanishing mass for the induced graviton in any braneworld model. We then apply this idea in the computation of the propagator on the wall of the dark bubble introduced in [1]."
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Published on:
15 February 2024
Publisher:
Springer
Published in:
Journal of High Energy Physics , Volume 2024 (2024)
Issue 2
Pages 1-19
DOI:
https://doi.org/10.1007/JHEP02(2024)102
arXiv:
2311.16242
Copyrights:
The Author(s)
Licence:
CC-BY-4.0

Fulltext files: