GrailQuest & HERMES: Hunting for gravitational wave electromagnetic counterparts and probing space-time quantum foam
- Burderi L.
- Di Salvo T.
- Sanna A.
- Fiore F.
- Riggio A.
- Gambino A. F.
- Amarilli F.
- Amati L.
- Ambrosino F.
- Amelino-Camelia G.
- Anitra A.
- Barbera M.
- Bechini M.
- Bellutti P.
- Bertacin R.
- Bertuccio G.
- Campana R.
- Cao J.
- Capozziello S.
- Ceraudo F.
- Chen T.
- Cinelli M.
- Citossi M.
- Clerici A.
- Colagrossi A.
- Costa E.
- Curzel S.
- De Laurentis M.
- Della Casa G.
- Demenev E.
- Del Santo M.
- Della Valle M.
- Dilillo G.
- Efremov P.
- Evangelista Y.
- Feroci M.
- Feruglio C.
- Ferrandi F.
- Fiorini M.
- Fiorito M.
- Frontera F.
- Fuschino F.
- Gacnik D.
- Galgoczi G.
- Gao N.
- Gandola M.
- Ghirlanda G.
- Gomboc A.
- Grassi M.
- Guidorzi C.
- Guzman A.
- Iaria R.
- Karlica M.
- Kostic U.
- Labanti C.
- La Rosa G.
- Lo Cicero U.
- Lopez Fernandez B.
- Lunghi P.
- Malcovati P.
- Maselli A.
- Manca A.
- Mele F.
- Milankovich D.
- Monge A.
- Morgante G.
- Nava L.
- Negri B.
- Nogara P.
- Ohno M.
- Ottolina D.
- Pasquale A.
- Pal A.
- Perri M.
- Piccinin M.
- Piazzolla R.
- Pirrotta S.
- Pliego-Caballero S.
- Prinetto J.
- Pucacco G.
- Puccetti S.
- Rapisarda M.
- Rashevskaya I.
- Rashevski A.
- Ripa J.
- Russo F.
- Papitto A.
- Piranomonte S.
- Santangelo A.
- Scala F.
- Sciarrone G.
- Selcan D.
- Silvestrini S.
- Sottile G.
- Rapisarda M.
- Rotovnik T.
- Tenzer C.
- Troisi I.
- Vacchi A.
- Virgilli E.
- Werner N.
- Wang L.
- Xu Y.
- Zampa G.
- Zampa N.
- Zane S.
- Zanotti G.
DOIAbstract
GrailQuest (Gamma-ray Astronomy International Laboratory for Quantum Exploration of Space-Time) is an ambitious astrophysical mission concept that uses a fleet of small satellites whose main objective is to search for a dispersion law for light propagation in vacuo. Within Quantum Gravity theories, different models for space-time quantization predict relative discrepancies of the speed of photons w.r.t. the speed of light that depend on the ratio of the photon energy to the Planck energy. This ratio is as small as 10-23 for photons in the γ- ray band (100 keV). Therefore, to detect this effect, light must propagate over enormous distances and the experiment must have extraordinary sensitivity. Gamma-Ray Bursts, occurring at cosmological dis...
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