Abstract
The exploration of the universe has recently entered a new era thanks to the multi-messenger paradigm, characterized by a continuous increase in the quantity and quality of experimental data that is obtained by the detection of the various cosmic messengers (photons, neutrinos, cosmic rays and gravitational waves) from numerous origins. They give us information about their sources in the universe and the properties of the intergalactic medium. Moreover, multi-messenger astronomy opens up the possibility to search for phenomenological signatures of quantum gravity. On the one hand, the most energetic events allow us to test our physical theories at energy regimes which are not directly accessible in accelerators; on the other hand, tiny effects in the propagation of very high energy particles could be amplified by cosmological distances. After decades of merely theoretical investigations, the possibility of obtaining phenomenological indications of Planck-scale effects is a revolutionary step in the quest for a quantum theory of gravity, but it requires cooperation between different communities of physicists (both theoretical and experimental). This review, prepared within the COST Action CA18108 "Quantum gravity phenomenology in the multi-messenger approach", is aimed at promoting this cooperation by giving a state-of-the art account of the interdisciplinary expertise that is needed in the effective search of quantum gravity footprints in the production, propagation and detection of cosmic messengers. (C) 2022 The Authors. Published by Elsevier B.V.
| Originalsprog | Engelsk |
|---|---|
| Artikelnummer | 103948 |
| Tidsskrift | Progress in Particle and Nuclear Physics |
| Vol/bind | 125 |
| Antal sider | 119 |
| ISSN | 0146-6410 |
| DOI | |
| Status | Udgivet - 2 jul. 2022 |
Citationsformater
- APA
- Standard
- Harvard
- Vancouver
- Author
- BIBTEX
- RIS
Quantum gravity phenomenology at the dawn of the multi-messenger era-A review. / Addazi, A.; Alvarez-Muniz, J.; Alves Batista, R.; Amelino-Camelia, G.; Antonelli, L.A.; Arzano, M.; Asorey, M.; Atteia, J-L; Bahamonde, S.; Bajardi, F.; Ballesteros, A.; Baret, B.; Barreiros, D. M.; Basilakos, S.; Benisty, D.; Birnholtz, O.; Blanco-Pillado, J. J.; Blas, D.; Bolmont, J.; Boncioli, D.; Bosso, P.; Calcagni, G.; Capozziello, S.; Carmona, J. M.; Cerci, S.; Chernyakova, M.; Clesse, S.; Coelho, J. A. B.; Colak, S. M.; Cortes, J. L.; Das, S.; D'Esposito; Demirci, M.; Di Luca, M. G.; di Matteo, A.; Dimitrijevic, D.; Djordjevic, G.; Prester, D. Dominis; Eichhorn, A.; Ellis, J.; Escamilla-Rivera, C.; Fabiano, G.; Franchino-Vinas, S. A.; Frassino, A. M.; Frattulillo, D.; Funk, S.; Fuster, A.; Gamboa, J.; Gent, A.; Gergely, L. A.; Giammarchi, M.; Giesel, K.; Glicenstein, J-F; Gracia-Bondia, J.; Gracia-Ruiz, R.; Gubitosi, G.; Guendelman, E.; Gutierrez-Sagredo; Haegel, L.; Heefer, S.; Held, A.; Herranz, F. J.; Hinderer, T.; Illana, J. I.; Ioannisian, A.; Jetzer, P.; Joaquim, F. R.; Kampert, K-H; Uysal, A. Karasu; Katori, T.; Kazarian, N.; Kerszberg, D.; Kowalski-Glikman, J.; Kuroyanagi, S.; Lammerzahl, C.; Said, J. Levi; Liberati, S.; Lim, E.; Lobo, I. P.; Lopez-Moya, M.; Luciano, G. G.; Manganaro, M.; Marciano, A.; Martin-Moruno, P.; Martinez, Manel; Martinez, Mario; Martinez-Huerta, H.; Martinez-Mirave, P.; Masip, M.; Mattingly, D.; Mavromatos, N.; Mazumdar, A.; Mendez, F.; Mercati, F.; Micanovic, S.; Mielczarek, J.; Miller, A. L.; Milosevic, M.; Minic, D.; Miramonti, L.; Mitsou, V. A.; Moniz, P.; Mukherjee, S.; Nardini, G.; Navas, S.; Niechciol, M.; Nielsen, A. B.; Obers, N. A.; Oikonomou, F.; Oriti, D.; Paganini, C. F.; Palomares-Ruiz, S.; Pasechnik, R.; Pasic, Srdjan; de los Heros, C. Perez; Pfeifer, C.; Pieroni, M.; Piran, T.; Platania, A.; Rastgoo, S.; Relancio, J. J.; Reyes, M. A.; Ricciardone, A.; Risse, M.; Rodriguez Frias, M. D.; Rosati, G.; Rubiera-Garcia, D.; Sahlmann, H.; Sakellariadou, M.; Salamida, F.; Saridakis, E. N.; Satunin, P.; Schiffer, M.; Schussler, F.; Sigl, G.; Sitarek, J.; Sola Peracaula, J.; Sopuerta, C. F.; Sotiriou, T. P.; Spurio, M.; Staicova, D.; Stergioulas, N.; Stoica, S.; Striskovic, J.; Stuttard, T.; Cerci, D. Sunar; Tavakoli, Y.; Ternes, C. A.; Terzic, T.; Thiemann, T.; Tinyakov, P.; Torri, M. D. C.; Tortola, M.; Trimarelli, C.; Trzesniewski, T.; Tureanu, A.; Urban, F. R.; Vagenas, E. C.; Vernieri, D.; Vitagliano, V.; Wallet, J-C; Zornoza, J. D.
I: Progress in Particle and Nuclear Physics, Bind 125, 103948, 02.07.2022.Publikation: Bidrag til tidsskrift › Review › Forskning › peer review
}
TY - JOUR
T1 - Quantum gravity phenomenology at the dawn of the multi-messenger era-A review
AU - Addazi, A.
AU - Alvarez-Muniz, J.
AU - Alves Batista, R.
AU - Amelino-Camelia, G.
AU - Antonelli, L.A.
AU - Arzano, M.
AU - Asorey, M.
AU - Atteia, J-L
AU - Bahamonde, S.
AU - Bajardi, F.
AU - Ballesteros, A.
AU - Baret, B.
AU - Barreiros, D. M.
AU - Basilakos, S.
AU - Benisty, D.
AU - Birnholtz, O.
AU - Blanco-Pillado, J. J.
AU - Blas, D.
AU - Bolmont, J.
AU - Boncioli, D.
AU - Bosso, P.
AU - Calcagni, G.
AU - Capozziello, S.
AU - Carmona, J. M.
AU - Cerci, S.
AU - Chernyakova, M.
AU - Clesse, S.
AU - Coelho, J. A. B.
AU - Colak, S. M.
AU - Cortes, J. L.
AU - Das, S.
AU - D'Esposito, null
AU - Demirci, M.
AU - Di Luca, M. G.
AU - di Matteo, A.
AU - Dimitrijevic, D.
AU - Djordjevic, G.
AU - Prester, D. Dominis
AU - Eichhorn, A.
AU - Ellis, J.
AU - Escamilla-Rivera, C.
AU - Fabiano, G.
AU - Franchino-Vinas, S. A.
AU - Frassino, A. M.
AU - Frattulillo, D.
AU - Funk, S.
AU - Fuster, A.
AU - Gamboa, J.
AU - Gent, A.
AU - Gergely, L. A.
AU - Giammarchi, M.
AU - Giesel, K.
AU - Glicenstein, J-F
AU - Gracia-Bondia, J.
AU - Gracia-Ruiz, R.
AU - Gubitosi, G.
AU - Guendelman, E.
AU - Gutierrez-Sagredo, null
AU - Haegel, L.
AU - Heefer, S.
AU - Held, A.
AU - Herranz, F. J.
AU - Hinderer, T.
AU - Illana, J. I.
AU - Ioannisian, A.
AU - Jetzer, P.
AU - Joaquim, F. R.
AU - Kampert, K-H
AU - Uysal, A. Karasu
AU - Katori, T.
AU - Kazarian, N.
AU - Kerszberg, D.
AU - Kowalski-Glikman, J.
AU - Kuroyanagi, S.
AU - Lammerzahl, C.
AU - Said, J. Levi
AU - Liberati, S.
AU - Lim, E.
AU - Lobo, I. P.
AU - Lopez-Moya, M.
AU - Luciano, G. G.
AU - Manganaro, M.
AU - Marciano, A.
AU - Martin-Moruno, P.
AU - Martinez, Manel
AU - Martinez, Mario
AU - Martinez-Huerta, H.
AU - Martinez-Mirave, P.
AU - Masip, M.
AU - Mattingly, D.
AU - Mavromatos, N.
AU - Mazumdar, A.
AU - Mendez, F.
AU - Mercati, F.
AU - Micanovic, S.
AU - Mielczarek, J.
AU - Miller, A. L.
AU - Milosevic, M.
AU - Minic, D.
AU - Miramonti, L.
AU - Mitsou, V. A.
AU - Moniz, P.
AU - Mukherjee, S.
AU - Nardini, G.
AU - Navas, S.
AU - Niechciol, M.
AU - Nielsen, A. B.
AU - Obers, N. A.
AU - Oikonomou, F.
AU - Oriti, D.
AU - Paganini, C. F.
AU - Palomares-Ruiz, S.
AU - Pasechnik, R.
AU - Pasic, Srdjan
AU - de los Heros, C. Perez
AU - Pfeifer, C.
AU - Pieroni, M.
AU - Piran, T.
AU - Platania, A.
AU - Rastgoo, S.
AU - Relancio, J. J.
AU - Reyes, M. A.
AU - Ricciardone, A.
AU - Risse, M.
AU - Rodriguez Frias, M. D.
AU - Rosati, G.
AU - Rubiera-Garcia, D.
AU - Sahlmann, H.
AU - Sakellariadou, M.
AU - Salamida, F.
AU - Saridakis, E. N.
AU - Satunin, P.
AU - Schiffer, M.
AU - Schussler, F.
AU - Sigl, G.
AU - Sitarek, J.
AU - Sola Peracaula, J.
AU - Sopuerta, C. F.
AU - Sotiriou, T. P.
AU - Spurio, M.
AU - Staicova, D.
AU - Stergioulas, N.
AU - Stoica, S.
AU - Striskovic, J.
AU - Stuttard, T.
AU - Cerci, D. Sunar
AU - Tavakoli, Y.
AU - Ternes, C. A.
AU - Terzic, T.
AU - Thiemann, T.
AU - Tinyakov, P.
AU - Torri, M. D. C.
AU - Tortola, M.
AU - Trimarelli, C.
AU - Trzesniewski, T.
AU - Tureanu, A.
AU - Urban, F. R.
AU - Vagenas, E. C.
AU - Vernieri, D.
AU - Vitagliano, V.
AU - Wallet, J-C
AU - Zornoza, J. D.
PY - 2022/7/2
Y1 - 2022/7/2
N2 - The exploration of the universe has recently entered a new era thanks to the multi-messenger paradigm, characterized by a continuous increase in the quantity and quality of experimental data that is obtained by the detection of the various cosmic messengers (photons, neutrinos, cosmic rays and gravitational waves) from numerous origins. They give us information about their sources in the universe and the properties of the intergalactic medium. Moreover, multi-messenger astronomy opens up the possibility to search for phenomenological signatures of quantum gravity. On the one hand, the most energetic events allow us to test our physical theories at energy regimes which are not directly accessible in accelerators; on the other hand, tiny effects in the propagation of very high energy particles could be amplified by cosmological distances. After decades of merely theoretical investigations, the possibility of obtaining phenomenological indications of Planck-scale effects is a revolutionary step in the quest for a quantum theory of gravity, but it requires cooperation between different communities of physicists (both theoretical and experimental). This review, prepared within the COST Action CA18108 "Quantum gravity phenomenology in the multi-messenger approach", is aimed at promoting this cooperation by giving a state-of-the art account of the interdisciplinary expertise that is needed in the effective search of quantum gravity footprints in the production, propagation and detection of cosmic messengers. (C) 2022 The Authors. Published by Elsevier B.V.
AB - The exploration of the universe has recently entered a new era thanks to the multi-messenger paradigm, characterized by a continuous increase in the quantity and quality of experimental data that is obtained by the detection of the various cosmic messengers (photons, neutrinos, cosmic rays and gravitational waves) from numerous origins. They give us information about their sources in the universe and the properties of the intergalactic medium. Moreover, multi-messenger astronomy opens up the possibility to search for phenomenological signatures of quantum gravity. On the one hand, the most energetic events allow us to test our physical theories at energy regimes which are not directly accessible in accelerators; on the other hand, tiny effects in the propagation of very high energy particles could be amplified by cosmological distances. After decades of merely theoretical investigations, the possibility of obtaining phenomenological indications of Planck-scale effects is a revolutionary step in the quest for a quantum theory of gravity, but it requires cooperation between different communities of physicists (both theoretical and experimental). This review, prepared within the COST Action CA18108 "Quantum gravity phenomenology in the multi-messenger approach", is aimed at promoting this cooperation by giving a state-of-the art account of the interdisciplinary expertise that is needed in the effective search of quantum gravity footprints in the production, propagation and detection of cosmic messengers. (C) 2022 The Authors. Published by Elsevier B.V.
KW - Lorentz invariance violation and deformation
KW - Gamma-ray astronomy
KW - Cosmic neutrinos
KW - Ultra-high-energy cosmic rays
KW - Gravitational waves
KW - GAMMA-RAY BURST
KW - LORENTZ INVARIANCE VIOLATION
KW - ENERGY COSMIC-RAYS
KW - GENERALIZED UNCERTAINTY PRINCIPLE
KW - EXTRAGALACTIC BACKGROUND LIGHT
KW - DOUBLY-SPECIAL RELATIVITY
KW - COHERENT STATES GCS
KW - PRIMORDIAL BLACK-HOLES
KW - ACTIVE GALACTIC NUCLEI
KW - CAUSAL DYNAMICAL TRIANGULATIONS
U2 - 10.1016/j.ppnp.2022.103948
DO - 10.1016/j.ppnp.2022.103948
M3 - Review
VL - 125
JO - Progress in Particle and Nuclear Physics
JF - Progress in Particle and Nuclear Physics
SN - 0146-6410
M1 - 103948
ER -