CERN Accelerating science

Article
Report number	arXiv:2111.05659
Title	Quantum gravity phenomenology at the dawn of the multi-messenger era—A review
Related title	Quantum gravity phenomenology at the dawn of the multi-messenger era—A review
Author(s)	Addazi, A. (SCU, Chengdu ; Frascati) ; Alvarez-Muniz, J. (Santiago de Compostela U., IGFAE) ; Alves Batista, R. (Madrid, IFT) ; Amelino-Camelia, G. (Naples U. ; INFN, Naples) ; Antonelli, V. (Milan U. ; INFN, Milan) ; Arzano, M. (Naples U. ; INFN, Naples) ; Asorey, M. (Zaragoza U.) ; Atteia, J.-L. (IRAP, Toulouse) ; Bahamonde, S. (Tartu, Inst. Phys. ; Tokyo Inst. Tech.) ; Bajardi, F. (Naples U.) ; Ballesteros, A. (Burgos U.) ; Baret, B. (APC, Paris) ; Barreiros, D.M. (Lisbon, IST) ; Basilakos, S. (Athens Academy ; Athens Observ.) ; Benisty, D. (Cambridge U., DAMTP ; Stockholm U., OKC ; Nordita ; Cambridge U., KICC) ; Birnholtz, O. (Bar Ilan U.) ; Blanco-Pillado, J.J. (IKERBASQUE, Bilbao ; Basque U., Bilbao) ; Blas, D. (Barcelona, IFAE) ; Bolmont, J. (Paris U., VI-VII) ; Boncioli, D. (INFN, Aquila ; L'Aquila U. ; Gran Sasso) ; Bosso, P. (Lethbridge U.) ; Calcagni, G. (Madrid, Inst. Estructura Materia) ; Capozziello, S. (Naples U. ; SSM, Naples ; INFN, Naples) ; Carmona, J.M. (Zaragoza U.) ; Cerci, S. (Adiyaman U.) ; Chernyakova, M. (Dublin City U. ; Dublin Inst. Adv. Stud., Astron. Astrophys.) ; Clesse, S. (Brussels U.) ; Coelho, J.A.B. (APC, Paris) ; Colak, S.M. (Barcelona, IFAE) ; Cortes, J.L. (Zaragoza U.) ; Das, S. (Lethbridge U.) ; D'Esposito, V. (Naples U.) ; Demirci, M. (Karadeniz U.) ; Di Luca, M.G. (SSM, Naples) ; di Matteo, A. (INFN, Turin) ; Dimitrijevic, D. (Nis U.) ; Djordjevic, G. (Nis U.) ; Dominis Prester, D. (Rijeka U.) ; Eichhorn, A. (Southern Denmark U., CP3-Origins) ; Ellis, J. (King's Coll. London ; NICPB, Tallinn ; CERN) ; Escamilla-Rivera, C. (Mexico U., ICN) ; Fabiano, G. (Naples U. ; INFN, Naples) ; Franchino-Viñas, S.A. (La Plata U.) ; Frassino, A.M. (ICC, Barcelona U.) ; Frattulillo, D. (Naples U. ; INFN, Naples) ; Funk, S. (Erlangen - Nuremberg U., ECAP) ; Fuster, A. (Eindhoven, Tech. U.) ; Gamboa, J. (Santiago de Chile U.) ; Gent, A. (Georgia Tech., Atlanta) ; Gergely, L.Á. (Szeged U.) ; Giammarchi, M. (INFN, Milan) ; Giesel, K. (Erlangen - Nuremberg U.) ; Glicenstein, J.-F. (IRFU, Saclay) ; Gracia-Bondía, J. (Zaragoza U. ; Costa Rica U.) ; Gracia-Ruiz, R. (Erlangen - Nuremberg U., ECAP) ; Gubitosi, G. (Naples U. ; INFN, Naples) ; Guendelman, E.I. (Ben Gurion U. of Negev ; FIGGS, Frankfurt ; Frankfurt U., FIAS ; Unlisted, BS) ; Gutierrez-Sagredo, I. (Burgos U.) ; Haegel, L. (APC, Paris) ; Heefer, S. (Eindhoven, Tech. U.) ; Held, A. (Jena U., TPI ; Princeton U. ; Sofiya, Inst. Nucl. Res. ; Imperial Coll., London) ; Herranz, F.J. (Burgos U.) ; Hinderer, T. (Utrecht U.) ; Illana, J.I. (Granada U., Theor. Phys. Astrophys.) ; Ioannisian, A. (Yerevan Phys. Inst.) ; Jetzer, P. (Zurich U.) ; Joaquim, F.R. (Lisbon, IST) ; Kampert, K.-H. (Wuppertal U.) ; Karasu Uysal, A. (Karatay U.) ; Katori, T. (King's Coll. London) ; Kazarian, N. (Yerevan Phys. Inst.) ; Kerszberg, D. (Barcelona, IFAE) ; Kowalski-Glikman, J. (Wroclaw U. ; Dubna, JINR ; NCBJ, Warsaw) ; Kuroyanagi, S. (Madrid, IFT ; Nagoya U.) ; Lämmerzahl, C. (Bremen U., ZARM) ; Levi Said, J. (U. Malta ; Malta U.) ; Liberati, S. (SISSA, Trieste ; INFN, Trieste ; IFPU, Trieste) ; Lim, E. (King's Coll. London) ; Lobo, I.P. (Lavras Federal U.) ; López-Moya, M. (HIAST ; Madrid U.) ; Luciano, G.G. (Salerno U. ; INFN, Salerno) ; Manganaro, M. (Rijeka U.) ; Marcianò, A. (Fudan U. ; Frascati) ; Martín-Moruno, P. (Madrid U.) ; Martinez, Manel (Barcelona, IFAE) ; Martinez, Mario (Barcelona, IFAE ; ICREA, Barcelona) ; Martínez-Huerta, H. (Autonoma de Nuevo Leon U.) ; Martínez-Miravé, P. (Valencia U., IFIC) ; Masip, M. (Granada U., Theor. Phys. Astrophys.) ; Mattingly, D. (Durham U.) ; Mavromatos, N. (Natl. Tech. U., Athens ; King's Coll. London) ; Mazumdar, A. (U. Groningen, VSI) ; Méndez, F. (Santiago de Chile U.) ; Mercati, F. (Burgos U.) ; Micanovic, S. (Rijeka U.) ; Mielczarek, J. (Jagiellonian U.) ; Miller, A.L. (Leuven U.) ; Milosevic, M. (Nis U.) ; Minic, D. (Virginia Tech.) ; Miramonti, L. (Milan U. ; INFN, Milan) ; Mitsou, V.A. (Valencia U., IFIC) ; Moniz, P. (Beira Interior U., Covilha) ; Mukherjee, S. (Perimeter Inst. Theor. Phys.) ; Nardini, G. (Stavanger U.) ; Navas, S. (Granada U., Theor. Phys. Astrophys.) ; Niechciol, M. (Siegen U.) ; Nielsen, A.B. (Stavanger U.) ; Obers, N.A. (DARK Cosmology Ctr. ; Nordita ; Stockholm U.) ; Oikonomou, F. (Norwegian U. Sci. Tech.) ; Oriti, D. (Munich U., ASC) ; Paganini, C.F. (Regensburg U. ; Potsdam, Max Planck Inst.) ; Palomares-Ruiz, S. (Valencia U., IFIC) ; Pasechnik, R. (Lund U., Dept. Theor. Phys.) ; Pasic, V. (Tuzla U.) ; Pérez de los Heros, C. (Uppsala U.) ; Pfeifer, C. (Bremen U., ZARM) ; Pieroni, M.P. (Sofiya, Inst. Nucl. Res. ; Imperial Coll., London) ; Piran, T. (Hebrew U.) ; Platania, A. (Perimeter Inst. Theor. Phys.) ; Rastgoo, S. (York U., Canada) ; Relancio, J.J. (Naples U. ; INFN, Naples ; Zaragoza U.) ; Reyes, M.A. (Zaragoza U.) ; Ricciardone, A. (Padua U. ; Padua U., Astron. Dept. ; INFN, Padua) ; Risse, M. (Siegen U.) ; Rodriguez Frias, M.D. (Alcala de Henares U.) ; Rosati, G. (Wroclaw U. ; Dubna, JINR) ; Rubiera-Garcia, D. (Madrid U.) ; Sahlmann, H. (Erlangen - Nuremberg U.) ; Sakellariadou, M. (King's Coll. London) ; Salamida, F. (INFN, Aquila ; L'Aquila U. ; Gran Sasso) ; Saridakis, E.N. (Athens Observ. ; Hefei, CUST) ; Satunin, P. (Moscow, INR) ; Schiffer, M. (Perimeter Inst. Theor. Phys.) ; Schüssler, F. (IRFU, Saclay) ; Sigl, G. (Hamburg U., Inst. Theor. Phys. II) ; Sitarek, J. (Lodz U. ; Tokyo U., ICRR) ; Solà Peracaula, J. (ICC, Barcelona U.) ; Sopuerta, C.F. (ICE, Bellaterra ; CSIC, Catalunya ; Barcelona, IEEC) ; Sotiriou, T.P. (U. Nottingham) ; Spurio, M. (Bologna U.) ; Staicova, D. (Sofiya, Inst. Nucl. Res.) ; Stergioulas, N. (Aristotle U., Thessaloniki) ; Stoica, S. (Bucharest, IFIN-HH) ; Strišković, J. (Boskovic Inst., Zagreb) ; Stuttard, T. (DARK Cosmology Ctr.) ; Sunar Cerci, D. (Adiyaman U.) ; Tavakoli, Y. (Gilan U., Rasht ; IPM, Tehran) ; Ternes, C.A. (INFN, Turin) ; Terzić, T. (Rijeka U.) ; Thiemann, T. (Erlangen - Nuremberg U.) ; Tinyakov, P. (Brussels U.) ; Torri, M.D.C. (Naples U. ; Milan U. ; INFN, Milan) ; Tórtola, M. (Valencia U., IFIC) ; Trimarelli, C. (INFN, Aquila ; L'Aquila U. ; Gran Sasso) ; Trześniewski, T. (Jagiellonian U.) ; Tureanu, A. (Helsinki U.) ; Urban, F.R. (Prague, Inst. Phys.) ; Vagenas, E.C. (Kuwait U.) ; Vernieri, D. (Naples U. ; INFN, Naples) ; Vitagliano, V. (Genoa U. ; Hull U.) ; Wallet, J.-C. (IJCLab, Orsay) ; Zornoza, J.D. (Valencia U., IFIC)
Publication	2022-07
Imprint	2021-11-10
Number of pages	119
Note	This review was written by participants of the COST Action CA18108. Further information on the review can be found at https://qg-mm.unizar.es/review/, updated to published version
In:	Prog. Part. Nucl. Phys. 125 (2022) pp.103948
DOI	10.1016/j.ppnp.2022.103948 (publication) 10.1016/j.ppnp.2022.103948 (publication)
Subject category	hep-th ; Particle Physics - Theory ; gr-qc ; General Relativity and Cosmology ; astro-ph.HE ; Astrophysics and Astronomy ; hep-ph ; Particle Physics - Phenomenology
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 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.
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