Pervasiveness of the breakdown of self-interacting vector field theories
dc.contributor.authorid | 0000-0001-8856-3067 | |
dc.contributor.authorid | 0000-0003-3075-1457 | |
dc.contributor.department | Department of Physics | |
dc.contributor.department | Department of Physics | |
dc.contributor.kuauthor | Coates, Andrew | |
dc.contributor.kuauthor | Ramazanoğlu, Fethi Mübin | |
dc.contributor.kuprofile | Researcher | |
dc.contributor.kuprofile | Faculty Member | |
dc.contributor.schoolcollegeinstitute | College of Sciences | |
dc.contributor.schoolcollegeinstitute | College of Sciences | |
dc.contributor.yokid | N/A | |
dc.contributor.yokid | 254225 | |
dc.date.accessioned | 2025-01-19T10:30:05Z | |
dc.date.issued | 2023 | |
dc.description.abstract | Various groups recently argued that self-interacting vector field theories lack a well-defined time evolution when the field grows to large amplitudes, which has drastic consequences for models in gravity and high energy theory. Such field amplitudes can be a result of an external driving mechanism, or occur intrinsically, due to large values of the field and its derivatives in the initial data. This brings a natural question: Is small amplitude initial data guaranteed to evolve indefinitely in these theories in the absence of an outside driving term? We answer this question in the negative, demonstrating that arbitrarily low amplitude initial data can still lead to the breakdown of the theory. Namely, ingoing spherically symmetric wave packets in more than one spatial dimensions grow as an inverse power of the radius, and their amplitudes can generically reach high enough values where time evolution ceases to exist. This simple example further establishes the pervasiveness of the pathology of self-interacting vector field theories. | |
dc.description.indexedby | WoS | |
dc.description.indexedby | Scopus | |
dc.description.issue | 10 | |
dc.description.openaccess | Green Submitted | |
dc.description.publisherscope | International | |
dc.description.sponsors | We thank Will East for many valuable discussions and stimulating questions. F. M. R acknowledges support from TUB I TAK Project No. 122F097. | |
dc.description.volume | 107 | |
dc.identifier.doi | 10.1103/PhysRevD.107.104036 | |
dc.identifier.eissn | 2470-0029 | |
dc.identifier.issn | 2470-0010 | |
dc.identifier.quartile | Q1 | |
dc.identifier.scopus | 2-s2.0-85159702679 | |
dc.identifier.uri | https://doi.org/10.1103/PhysRevD.107.104036 | |
dc.identifier.uri | https://hdl.handle.net/20.500.14288/25966 | |
dc.identifier.wos | 995756000007 | |
dc.language | en | |
dc.publisher | American Physical Society | |
dc.relation.grantno | [122F097] | |
dc.source | Physical Review D | |
dc.subject | Astronomy and astrophysics | |
dc.subject | Physics, particles and fields | |
dc.title | Pervasiveness of the breakdown of self-interacting vector field theories | |
dc.type | Journal Article |
Files
Original bundle
1 - 1 of 1