Quantum gravity phenomenology at the dawn of the multi-messenger era—A review

Addazi, Andrea; Álvarez-Muñiz, J.; Batista, Rafael Alves; Amelino‐Camelia, Giovanni; Antonelli, Vito; Arzano, Michele; Asorey, M.; Atteia, J. L.; Bahamonde, Sebastián; Bajardi, F; Ballesteros, Ángel; Baret, B.; Barreiros, D. M.; Basilakos, Spyros; Benisty, David; Birnholtz, O.; Blanco-Pillado, José J.; Blas, Diego; Bolmont, J.; Boncioli, D.; Bosso, Pasquale; Calcagni, Gianluca; Capozziello, Salvatore; Carmona, J. M.; Çerçi, S.; Chernyakov, M.; Clesse, S.; Coelho, J. A. B.; Colak, S. M.; Cortés, José Luis; Das, Saurya; D’Esposito, Vittorio; Demirci, Mehmet; Luca, M. G. Di; Matteo, Armando di; Dimitrijević, Dragoljub D.; Djordjević, Goran S.; Prester, D. Dominis; Eichhorn, Astrid; Ellis, John; Escamilla-Rivera, Celia; Fabiano, G.; Franchino-Viñas, S. A.; Frassino, Antonia Micol; Frattulillo, D.; Funk, S.; Fuster, Alan; Gamboa, J.; Gent, A.; Gergely, L.; Giammarchi, M.; Giesel, Kristina; Glicenstein, J. F.; Gracia‐Bondía, José M.; Gracia-Ruiz, R.; Gubitosi, Giulia; Guendelman, Eduardo; Gutiérrez-Sagredo, Iván; Haegel, L.; Heefer, Sjors; Held, Aaron; Herranz, Francisco J.; Hinderer, Tanja; Illana, J. I.; Ioannisian, Ara; Jetzer, Philippe; Joaquim, F. R.; Kampert, K. H.; Uysal, A. Karasu; Katori, T.; Kazarian, Narine; Kerszberg, Daniel; Kowalski-Glikman, Jerzy; Kuroyanagi, Sachiko; Lämmerzahl, Cláus; Said, Jackson Levi; Liberati, Stefano; Lim, Eugene A.; Lobo, Iarley P.; López-Moya, Marcos; Luciano, Giuseppe Gaetano; Manganaro, M.; Marcianò, Antonino; Martín–Moruno, Prado; Martı́nez, M.; Martínez, M.; Martínez-Huerta, H.; Martínez-Miravé, Pablo; Masip, M.; Mattingly, David; Mavromatos, Nick E.; Mazumdar, Anupam; Méndez, F.; Mercati, Flavio; Mićanović, Saša; Mielczarek, Jakub; Miller, A.; Milošević, Milan; Minić, Djordje; Miramonti, L.; Mitsou, V. A.; Moniz, P. R. L. V.; Mukherjee, Soma; Nardini, Germano; Navas, S.; Niechciol, Marcus; Nielsen, A. B.; Obers, Niels A.; Oikonomou, Foteini; Oriti, Daniele; Paganini, Claudio F.; Palomares‐Ruiz, Sergio; Pasechnik, Roman; Pasic, Vedad; Heros, C. Pérez de los; Pfeifer, Christian; Pieroni, Mauro; Piran, Tsvi; Platania, Alessia; Rastgoo, Saeed; Relancio, J. J.; Reyes, M. A.; Ricciardone, Angelo; Risse, M.; Frías, M. D. Rodríguez; Rosati, Giacomo; Rubiera-García, Diego; Sahlmann, Hanno; Sakellariadou, Mairi; Salamida, F.; Saridakis, Emmanuel N.; Satunin, Petr; Schiffer, Marc; Schüßler, F.; Sigl, Guenter; Sitarek, J.; Peracaula, Joan Solà; Sopuerta, Carlos F.; Sotiriou, Thomas P.; Spurio, M.; Staicova, Denitsa; Stergioulas, Nikolaos; Stoica, S.; Strišković, Jelena; Stuttard, T.; Cerci, D. Sunar; Tavakoli, Yaser; Ternes, C. A.; Terzić, T.; Thiemann, Thomas; Tinyakov, P.; Torri, Marco Danilo Claudio; Tórtola, M.; Trimarelli, Caterina; Trześniewski, Tomasz; Tureanu, Anca; Urban, Federico; Vagenas, Elias C.; Vernieri, Daniele; Vitagliano, Vincenzo; Wallet, Jean-Christophe; Zornoza, J. D.

doi:10.1016/j.ppnp.2022.103948

Cited by 231 publications

(160 citation statements)

References 1,199 publications

Supporting

Mentioning

159

Contrasting

Order By: Relevance

“…At the same time, there are many reasons indicating that one should construct modified gravitational theories. At the theoretical level, gravitational modifications are known to be able to improve the renormalizability issues of general relativity [28,29]. At the phenomenological level, modified gravity can offer an alternative way to explain the two phases of the Universe's accelerated expansion, namely the early-time, inflationary one [30,31], and/or the late-time, dark-energy one [32][33][34].…”

Section: Introductionmentioning

confidence: 99%

Scalar induced gravitational waves from primordial black hole Poisson fluctuations in $f(R)$ gravity

Papanikolaou¹,

Tzerefos²,

Basilakos³

et al. 2021

Preprint

View full text Add to dashboard Cite

The gravitational potential of a gas of initially randomly distributed primordial black holes (PBH) can induce a stochastic gravitational-wave background through second-order gravitational effects. This gravitational-wave background can be abundantly generated in a cosmic era of domination of ultralight primordial black holes, with masses m PBH < 10 9 g, which evaporate before Big Bang Nucleosynthesis. Hence, the condition to avoid overproduction of gravitational waves at PBH evaporation time, can act as a novel method to extract constraints on cosmological models and gravitational theories. We consider f (R) gravity as the underlying gravitational theory and we study its effect at the level of the gravitational potential of Poisson distributed primordial black holes. After the general analysis we focus on Starobinsky R 2 gravity model and we extract strong constraints on the involved mass parameter, denoted as M , as a function of the initial primordial black hole abundance, Ω PBH,f and the black hole mass, m PBH . In particular, one finds that in general 5 × 10 −14 M min M Pl 10 −5 , and only in the extreme possible regime where Ω PBH,f > 10 −3 we get that 10 −5 M min M Pl 10 −1 .

show abstract

Section: Introductionmentioning

confidence: 99%

Scalar induced gravitational waves from primordial black hole Poisson fluctuations in $f(R)$ gravity

Papanikolaou¹,

Tzerefos²,

Basilakos³

et al. 2021

Preprint

View full text Add to dashboard Cite

show abstract

“…In fact, for those models for which a nontrivial structure regarding time is present, such as the κ-Minkowski model, the Moyal twist of quantum mechanics is ill-defined, since in it only the vector fields of the space components appear. Given the relevance of models with time noncommutativity in the literature, especially when phenomenology is involved [9,46], it would be interesting to investigate whether other methods leading to double quantization can be defined, which are compatible with a time noncommutativity.…”

Section: Discussionmentioning

confidence: 99%

“…In order to construct the double quantization of the phase space associated to the space noncommutativity (36), we can proceed as for the λ-Minkwoski case and express the noncommutative space coordinates as a function of the canonical phase-space ones, given in Eq. (9). A particularly simple solution is…”

Section: Symmetries Of the Doubly-quantized Phase Spacementioning

confidence: 99%

“…If spacetime noncommutativity is to be ascribed to quantum gravitational effects, then it would be natural to link this scale to the Planck length l P ≡ G/c 3 . While this is a reasonable assumption, in principle the two noncommutativity constants, and λ, are not necessarily related [7,8] (see also [9,Sec. 2.3] and references therein), and one could consider the two quantization procedures independently.…”

Section: Introductionmentioning

confidence: 99%

See 1 more Smart Citation

Double Quantization

Gubitosi,

Lizzi,

Relancio

et al. 2021

Preprint

View full text Add to dashboard Cite

In a quantum gravity theory, it is expected that the classical notion of spacetime disappears, leading to a quantum structure with new properties. A possible way to take into account these quantum effects is through a noncommutativity of spacetime coordinates. In the literature, there is not a clear way to describe at the same time a noncommutativity of spacetime and the phasespace noncommutativity of quantum mechanics. In this paper we address this issue by constructing a Drinfel'd twist in phase space which deals with both quantizations. This method can be applied to a noncommutativity which involves only space, leaving time aside. We apply our construction to the so-called λ-Minkwoski and R 3 λ noncommutative spaces.

show abstract

“…The aim of this paper is the explicit construction of the noncommutative space of light-like geodesics associated to the κ-deformation. Indeed, the study of the propagation of photons on a quantum spacetime is one of the main theoretical problems in quantum gravity phenomenology (see [39,40]) and we hope that this new model could shed some light in this context. Moreover, we will show that the construction of this new noncommutative space is possible only if the light-like (or null-plane) κ-deformation of the Poincaré algebra [41][42][43] is considered.…”

Section: Introductionmentioning

confidence: 99%

The noncommutative space of light-like worldlines

Ballesteros,

Gutierrez-Sagredo,

Herranz

2022

Preprint

View full text Add to dashboard Cite

The noncommutative space of light-like worldlines that is covariant under the light-like (or null-plane) κ-deformation of the (3+1) Poincaré group is fully constructed as the quantization of the corresponding Poisson homogeneous space of null geodesics. This new noncommutative space of geodesics is five-dimensional, and turns out to be defined as a quadratic algebra that can be mapped to a non-central extension of the direct sum of two Heisenberg-Weyl algebras whose noncommutative parameter is just the Planck scale parameter κ −1 . Moreover, it is shown that the usual time-like κ-deformation of the Poincaré group does not allow the construction of the Poisson homogeneous space of light-like worldlines. Therefore, the most natural choice in order to model the propagation of massless particles on a quantum Minkowski spacetime seems to be provided by the light-like κ-deformation.

show abstract

Quantum gravity phenomenology at the dawn of the multi-messenger era—A review

Cited by 231 publications

References 1,199 publications

Scalar induced gravitational waves from primordial black hole Poisson fluctuations in $f(R)$ gravity

Scalar induced gravitational waves from primordial black hole Poisson fluctuations in $f(R)$ gravity

Double Quantization

The noncommutative space of light-like worldlines

Contact Info

Product

Resources

About