Abstract
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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Acknowledgments
We would like to thank Johanna Erdmenger, Suvendu Giri, Andreas Karch, Dominik Neuenfeld, Daniel Panizo and Thomas Van Riet for useful discussions and communications. We would also like to thank Dominik Neuenfeld for comments on an earlier version of the manuscript.
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Banerjee, S., Danielsson, U. & Zemsch, M. The dark bubbleography. J. High Energ. Phys. 2024, 102 (2024). https://doi.org/10.1007/JHEP02(2024)102
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DOI: https://doi.org/10.1007/JHEP02(2024)102