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].
{ "_oai": { "updated": "2024-06-18T15:33:36Z", "id": "oai:repo.scoap3.org:83442", "sets": [ "JHEP" ] }, "authors": [ { "affiliations": [ { "country": "Germany", "value": "Institut f\u00fcr Theoretische Physik und Astrophysik, Julius-Maximilians-Universit\u00e4t W\u00fcrzburg, Am Hubland, W\u00fcrzburg, 97074, Germany", "organization": "Julius-Maximilians-Universit\u00e4t W\u00fcrzburg" } ], "surname": "Banerjee", "email": "souvik.banerjee@physik.uni-wuerzburg.de", "full_name": "Banerjee, Souvik", "given_names": "Souvik" }, { "affiliations": [ { "country": "Sweden", "value": "Institutionen f\u00f6r fysik och astronomi, Uppsala Universitet, Box 803, Uppsala, SE-751 08, Sweden", "organization": "Uppsala Universitet" } ], "surname": "Danielsson", "email": "ulf.danielsson@physics.uu.se", "full_name": "Danielsson, Ulf", "given_names": "Ulf" }, { "affiliations": [ { "country": "Germany", "value": "Institut f\u00fcr Theoretische Physik und Astrophysik, Julius-Maximilians-Universit\u00e4t W\u00fcrzburg, Am Hubland, W\u00fcrzburg, 97074, Germany", "organization": "Julius-Maximilians-Universit\u00e4t W\u00fcrzburg" } ], "surname": "Zemsch", "email": "maximilian.zemsch@stud-mail.uni-wuerzburg.de", "full_name": "Zemsch, Maximilian", "given_names": "Maximilian" } ], "titles": [ { "source": "Springer", "title": "The dark bubbleography" } ], "dois": [ { "value": "10.1007/JHEP02(2024)102" } ], "publication_info": [ { "page_end": "19", "journal_title": "Journal of High Energy Physics", "material": "article", "journal_volume": "2024", "artid": "JHEP02(2024)102", "year": 2024, "page_start": "1", "journal_issue": "2" } ], "$schema": "http://repo.scoap3.org/schemas/hep.json", "acquisition_source": { "date": "2024-06-18T15:31:47.711731", "source": "Springer", "method": "Springer", "submission_number": "a024d7ea2d8711ef9fecbe60ec5a7b90" }, "page_nr": [ 19 ], "license": [ { "url": "https://creativecommons.org/licenses//by/4.0", "license": "CC-BY-4.0" } ], "copyright": [ { "holder": "The Author(s)", "year": "2024" } ], "control_number": "83442", "record_creation_date": "2024-02-15T21:30:09.991870", "_files": [ { "checksum": "md5:eeca4b386f63a67fe229f3bf5481459f", "filetype": "xml", "bucket": "1457eb0f-ee69-4a10-8e40-04541617c3fd", "version_id": "deb296f0-62e8-41b0-a01a-dac4b0d9e11e", "key": "10.1007/JHEP02(2024)102.xml", "size": 11288 }, { "checksum": "md5:33e9c61b2808b136872988bc5a473e2e", "filetype": "pdf/a", "bucket": "1457eb0f-ee69-4a10-8e40-04541617c3fd", "version_id": "30d9da75-1c62-425c-a342-3455f047665b", "key": "10.1007/JHEP02(2024)102_a.pdf", "size": 351201 } ], "collections": [ { "primary": "Journal of High Energy Physics" } ], "arxiv_eprints": [ { "categories": [ "hep-th" ], "value": "2311.16242" } ], "abstracts": [ { "source": "Springer", "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]." } ], "imprints": [ { "date": "2024-02-15", "publisher": "Springer" } ] }