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1.
Terrestrial Very-Long-Baseline Atom Interferometry: Workshop Summary Terrestrial Very-Long-Baseline Atom Interferometry Workshop (TVLBAI 2023)   13 - 14 Mar 2023  - CERN, Geneva, Switzerland  / Abend, Sven (Leibniz U., Hannover); Allard, Baptiste (LCAR, Toulouse); Alonso, Iván (Balearic Islands U.); Antoniadis, John (Crete U.); Araújo, Henrique (Imperial Coll., London); Arduini, Gianluigi (CERN); Arnold, Aidan S. (SUPA, UK ; Strathclyde U.); Aßmann, Tobias (Ulm U.); Augst, Nadja (DLR, Neustrelitz); Badurina, Leonardo (King's Coll. London ; Caltech) et al.
This document presents a summary of the 2023 Terrestrial Very-Long-Baseline Atom Interferometry Workshop hosted by CERN. The workshop brought together experts from around the world to discuss the exciting developments in large-scale atom interferometer (AI) prototypes and their potential for detecting ultralight dark matter and gravitational waves. [...]
2023 - 99 p. arXiv:2310.08183 - Published in : 10.1116/5.0185291
10.1116/5.0185291
2.
FRB 121102 Casts New Light on the Photon Mass / Bonetti, Luca (Orleans U. ; LPC2E, Orleans) ; Ellis, John (King's Coll. London ; CERN) ; Mavromatos, Nikolaos E. (King's Coll. London ; CERN) ; Sakharov, Alexander S. (New York U. ; Manhattan Coll., Riverdale ; CERN) ; Sarkisyan-Grinbaum, Edward K. (CERN ; Texas U., Arlington) ; Spallicci, Alessandro D. A. M. (Orleans U. ; LPC2E, Orleans)
The photon mass, $m_\gamma$, can in principle be constrained using measurements of the dispersion measures (DMs) of fast radio bursts (FRBs), once the FRB redshifts are known. The DM of the repeating FRB 121102 is known to $< 1$\%, a host galaxy has now been identified with high confidence,and its redshift, $z$, has now been determined with high accuracy: $z = 0.19273(8)$. [...]
arXiv:1701.03097; KCL-PH-TH-2017-01; CERN-TH-2017-007.- 2017-05-10 - 4 p. - Published in : Phys. Lett. B 768 (2017) 326-329 Article from SCOAP3: PDF; Fulltext: PDF;
3.
Photon Mass Limits from Fast Radio Bursts / Bonetti, Luca (Orleans U. ; LPCE, Orleans) ; Ellis, John (King's Coll. London ; CERN) ; Mavromatos, Nikolaos E. (King's Coll. London ; CERN) ; Sakharov, Alexander S. (New York U. ; Manhattan Coll., Riverdale ; CERN) ; Sarkisyan-Grinbaum, Edward K.G. (CERN ; Texas U., Arlington) ; Spallicci, Alessandro D.A.M. (Orleans U. ; LPCE, Orleans)
The frequency-dependent time delays in fast radio bursts (FRBs) can be used to constrain the photon mass, if the FRB redshifts are known, but the similarity between the frequency dependences of dispersion due to plasma effects and a photon mass complicates the derivation of a limit on $m_\gamma$. The redshift of FRB 150418 has been measured to $\sim 2$% and its dispersion measure (DM) is known to $\sim 0.1$%, but the strength of the constraint on $m_\gamma$ is limited by uncertainties in the modelling of the host galaxy and the Milky Way, as well as possible inhomogeneities in the intergalactic medium (IGM). [...]
arXiv:1602.09135; KCL-PH-TH-2016-08; LCTS-2016-06; CERN-TH-2016-044; KCL-PH-TH-2016-08; LCTS-2016-06; CERN-TH-2016-044.- Geneva : CERN, 2016-06-10 - 5 p. - Published in : Phys. Lett. B 757 (2016) 548-552 Article from SCOAP3: PDF; Elsevier Open Access article: PDF; Fulltext: PDF; External link: Preprint

See also: similar author names
6 Spallicci, A
10 Spallicci, A D
2 Spallicci, A.
7 Spallicci, Alessandro
12 Spallicci, Alessandro D A M
1 Spallicci, Alessandro D. A. M.
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