Gotowe bibliografie tematyczne / Carrollian holography

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Gotowa bibliografia na temat „Carrollian holography”

Autor: Grafiati

Data publikacji: 23 listopada 2024

Data aktualizacji: 31 lipca 2025

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Artykuły w czasopismach na temat "Carrollian holography"

Nguyen, Kevin, and Peter West. "Carrollian Conformal Fields and Flat Holography." Universe 9, no. 9 (2023): 385. http://dx.doi.org/10.3390/universe9090385.

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The null conformal boundary I of Minkowski spacetime M plays a special role in scattering theory, as it is the locus where massless particle states are most naturally defined. We construct quantum fields on I, which create these massless states from the vacuum and transform covariantly under Poincaré symmetries. Because the latter symmetries act as Carrollian conformal isometries of I, these quantum fields are Carrollian conformal fields. This group theoretic construction is intrinsic to I by contrast to existing treatments in the literature. However, we also show that the standard relativisti

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Have, Emil, Kevin Nguyen, Stefan Prohazka, and Jakob Salzer. "Massive carrollian fields at timelike infinity." Journal of High Energy Physics 2024, no. 7 (2024). http://dx.doi.org/10.1007/jhep07(2024)054.

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Abstract Motivated by flat space holography, we demonstrate that massive spin-s fields in Minkowski space near timelike infinity are massive carrollian fields on the carrollian counterpart of anti-de Sitter space called Ti. Its isometries form the Poincaré group, and we construct the carrollian spin-s fields using the method of induced representations. We provide a dictionary between massive carrollian fields on Ti and massive fields in Minkowski space, as well as to fields in the conformal primary basis used in celestial holography. We show that the symmetries of the carrollian structure natu

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Mason, Lionel, Romain Ruzziconi, and Akshay Yelleshpur Srikant. "Carrollian amplitudes and celestial symmetries." Journal of High Energy Physics 2024, no. 5 (2024). http://dx.doi.org/10.1007/jhep05(2024)012.

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Abstract Carrollian holography aims to express gravity in four-dimensional asymptotically flat spacetime in terms of a dual three-dimensional Carrollian CFT living at null infinity. Carrollian amplitudes are massless scattering amplitudes written in terms of asymptotic or null data at $$ \mathcal{I} $$ I . These position space amplitudes at $$ \mathcal{I} $$ I are to be re-interpreted as correlation functions in the putative dual Carrollian CFT. We derive basic results concerning tree-level Carrollian amplitudes yielding dynamical constraints on the holographic dual. We obtain surprisingly com

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Saha, Amartya. "w1+∞ and Carrollian holography." Journal of High Energy Physics 2024, no. 5 (2024). http://dx.doi.org/10.1007/jhep05(2024)145.

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Abstract In a 1 + 2D Carrollian conformal field theory, the Ward identities of the two local fields $$ {S}_0^{+} $$ S 0 + and $$ {S}_1^{+} $$ S 1 + , entirely built out of the Carrollian conformal stress-tensor, contain respectively up to the leading and the subleading positive helicity soft graviton theorems in the 1 + 3D asymptotically flat space-time. This work investigates how the subsubleading soft graviton theorem can be encoded into the Ward identity of a Carrollian conformal field $$ {S}_2^{+} $$ S 2 + . The operator product expansion (OPE) $$ {S}_2^{+}{S}_2^{+} $$ S 2 + S 2 + is const

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Bagchi, Arjun, Prateksh Dhivakar, and Sudipta Dutta. "AdS Witten diagrams to Carrollian correlators." Journal of High Energy Physics 2023, no. 4 (2023). http://dx.doi.org/10.1007/jhep04(2023)135.

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Abstract Carrollian Conformal Field Theories (CFTs) have been proposed as co-dimension one holographic duals to asymptotically flat spacetimes as opposed to Celestial CFTs which are co-dimension two. In this paper, drawing inspiration from Celestial holography, we show by a suitable generalisation of the flat space limit of AdS that keeps track of the previously disregarded null direction, one can reproduce Carrollian CFT correlation functions from AdS Witten diagrams. In particular, considering Witten diagrams in AdS4, we reproduce two and three-point correlation functions for three dimension

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Bagchi, Arjun, Prateksh Dhivakar, and Sudipta Dutta. "Holography in flat spacetimes: the case for Carroll." Journal of High Energy Physics 2024, no. 8 (2024). http://dx.doi.org/10.1007/jhep08(2024)144.

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Abstract We compare and contrast the two approaches of holography in asymptotically flat spacetimes, viz. the co-dimension two Celestial approach based on the Mellin transformation and the co-dimension one Carrollian approach based on the modified Mellin and elucidate how some of the problems of the Celestial approach can be rectified by the Carrollian one. Considering flat holography as a limit from AdS/CFT makes a co-dimension one dual more plausible, and our previous construction of Carrollian correlations from AdS Witten diagrams is testimony to this. In this paper, we show how to generali

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Salzer, Jakob. "An embedding space approach to Carrollian CFT correlators for flat space holography." Journal of High Energy Physics 2023, no. 10 (2023). http://dx.doi.org/10.1007/jhep10(2023)084.

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Abstract Carrollian conformal field theories (carrollian CFTs) are natural field theories on null infinity of an asymptotically flat spacetime or, more generally, geometries with conformal carrollian structure. Using a basis transformation, gravitational S-matrix elements can be brought into the form of correlators of a carrollian CFT. Therefore, it has been suggested that carrollian CFTs could provide a co-dimension one dual description to gravity in asymptotically flat spacetimes. In this work, we construct an embedding space formalism for three-dimensional carrollian CFTs and use it to dete

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Donnay, Laura, Adrien Fiorucci, Yannick Herfray, and Romain Ruzziconi. "Carrollian Perspective on Celestial Holography." Physical Review Letters 129, no. 7 (2022). http://dx.doi.org/10.1103/physrevlett.129.071602.

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Ciambelli, Luca, Charles Marteau, Anastasios C. Petkou, P. Marios Petropoulos, and Konstantinos Siampos. "Flat holography and Carrollian fluids." Journal of High Energy Physics 2018, no. 7 (2018). http://dx.doi.org/10.1007/jhep07(2018)165.

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Donnay, Laura, Adrien Fiorucci, Yannick Herfray, and Romain Ruzziconi. "Bridging Carrollian and celestial holography." Physical Review D 107, no. 12 (2023). http://dx.doi.org/10.1103/physrevd.107.126027.

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Rozprawy doktorskie na temat "Carrollian holography"

Rivera, betancour David. "Aspects of Carrollian physics." Electronic Thesis or Diss., Institut polytechnique de Paris, 2023. http://www.theses.fr/2023IPPAX146.

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Nous étudions divers aspects et applications gravitationnelles de la dynamique carrollienne. Les systèmes carrolliens se manifestent lorsque la vitesse de la lumière s’annule. Nous construisons des équations dynamiques générales carrolliennes et galiléennes valables pour des géométries carrolliennes/newtoniennes arbitraires, courbes et dépendantes du temps, l’accent étant mis sur l’hydrodynamique. La présence d'un courant U(1) est aussi prise en compte. Cette démarche suit deux approches : basée sur l'invariance de l'action sous Carroll/Galilée et Weyl, ou par la prise d'une limite de grande/p

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Ciambelli, Luca. "paving the fluid road to flat holography." Thesis, Université Paris-Saclay (ComUE), 2019. http://www.theses.fr/2019SACLX055/document.

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L’objet de cette thèse est l’étude de la correspondance fluide/gravité, réalisation macroscopique de la dualité AdS/CFT, à la limite où la constante cosmologique tend vers zéro (limite plate). La jauge de Fefferman-Graham, habituellement utilisée dans le dictionnaire holographique, est singulière à la limite plate. Ici, en passant par la formulation hydrodynamique de la théorie dubord, nous construisons une jauge, appelée jauge du développement en série dérivatif, où cette limite est bien définie. Sur la géométrie du bord, elle correspond en fait à faire tendre vers zéro la vitesse de la lumiè

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Vilatte, Matthieu. "Adventures in (thermal) Wonderland." Electronic Thesis or Diss., Institut polytechnique de Paris, 2024. https://theses.hal.science/tel-04791687.

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Le travail que nous présentons dans cette thèse est structuré autour de la notion de théorie des champs et de géométrie, qui sont appliquées à la gravité et la thermalisation.En gravité, notre travail donne un éclairage nouveau sur la structure asymptotique du champ gravitationnel dans le contexte des espace-temps asymptotiquement plats, ceci en utilisant l'information codée sur leur bord conforme. Ce dernier est une hypersurface de genre lumière sur laquelle émerge la physique carrollienne au lieu de la physique relativiste. Une structure carrollienne sur une variété est constituée une métriq

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