CERN Accelerating science

CERN Document Server 11 record trovati  1 - 10successivo  salta al record: La ricerca ha impiegato 0.56 secondi. 
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.
Tests of General Relativity with GWTC-3 / LIGO Scientific Collaboration
The ever-increasing number of detections of gravitational waves (GWs) from compact binaries by the Advanced LIGO and Advanced Virgo detectors allows us to perform ever-more sensitive tests of general relativity (GR) in the dynamical and strong-field regime of gravity. [...]
arXiv:2112.06861 ; LIGO-P2100275.
- 41 p.
Fulltext
3.
Search for Subsolar-Mass Binaries in the First Half of Advanced LIGO’s and Advanced Virgo’s Third Observing Run / LIGO Scientific Collaboration
We report on a search for compact binary coalescences where at least one binary component has a mass between 0.2 $M_\odot$ and 1.0 $M_\odot$ in Advanced LIGO and Advanced Virgo data collected between 1 April 2019 1500 UTC and 1 October 2019 1500 UTC. We extend previous analyses in two main ways: we include data from the Virgo detector and we allow for more unequal mass systems, with mass ratio $q \geq 0.1$. [...]
arXiv:2109.12197; LIGO-P2100163-v8.- 2022-08-05 - 16 p. - Published in : Phys. Rev. Lett. 129 (2022) 061104 Fulltext: PDF;
4.
Cosmology with the Laser Interferometer Space Antenna / LISA Cosmology Working Group Collaboration
The Laser Interferometer Space Antenna (LISA) has two scientific objectives of cosmological focus: to probe the expansion rate of the universe, and to understand stochastic gravitational-wave backgrounds and their implications for early universe and particle physics, from the MeV to the Planck scale. However, the range of potential cosmological applications of gravitational wave observations extends well beyond these two objectives. [...]
arXiv:2204.05434; LISA CosWG-22-03; FERMILAB-PUB-22-349-SCD.- 2023-08-28 - 176 p. - Published in : Living Rev. Relativ. 26 (2023) 5 Fulltext: jt - PDF; 2204.05434 - PDF; Fulltext from Publisher: PDF; External link: Fermilab Library Server
5.
First joint observation by the underground gravitational-wave detector KAGRA with GEO 600 / KAGRA Collaboration
We report the results of the first joint observation of the KAGRA detector with GEO600. KAGRA is a cryogenic and underground gravitational-wave detector consisting of a laser interferometer with three-kilometer arms, and located in Kamioka, Gifu, Japan. [...]
arXiv:2203.01270; LIGO-P2100286.- 2022-06-14 - 37 p. - Published in : PTEP 2022 (2022) 063F01 Fulltext: 2203.01270 - PDF; document - PDF;
6.
New horizons for fundamental physics with LISA / LISA Collaboration
The Laser Interferometer Space Antenna (LISA) has the potential to reveal wonders about the fundamental theory of nature at play in the extreme gravity regime, where the gravitational interaction is both strong and dynamical. In this white paper, the Fundamental Physics Working Group of the LISA Consortium summarizes the current topics in fundamental physics where LISA observations of GWs can be expected to provide key input. [...]
arXiv:2205.01597.- 2022-06-30 - 116 p. - Published in : Living Rev. Relativ. 25 (2022) 4 Fulltext: 2205.01597 - PDF; document - PDF;
7.
Discussion / Tolley, Andrew (speaker) (Imperial College London)
2021 - 3116. Conferences & Workshops; Positivity and the Bootstrap External links: Talk details; Event details In : Positivity and the Bootstrap
8.
Prospects for Fundamental Physics with LISA / LISA Collaboration
In this paper, which is of programmatic rather than quantitative nature, we aim to further delineate and sharpen the future potential of the LISA mission in the area of fundamental physics. Given the very broad range of topics that might be relevant to LISA, we present here a sample of what we view as particularly promising directions, based in part on the current research interests of the LISA scientific community in the area of fundamental physics. [...]
arXiv:2001.09793.- 2020-08-31 - 22 p. Fulltext: PDF;
9.
Non-Gaussianity as a Probe of the Physics of the Primordial Universe and the Astrophysics of the Low Redshift Universe / Komatsu, E. (Texas U. ; Tokyo U.) ; Afshordi, N. (Perimeter Inst. Theor. Phys.) ; Bartolo, N. (Padua U.) ; Baumann, D. (Harvard U.) ; Bond, J.R. (Toronto U.) ; Buchbinder, E.I. (Perimeter Inst. Theor. Phys.) ; Byrnes, C.T. (Heidelberg U.) ; Chen, Xingang (MIT) ; Chung, D.J.H. (Wisconsin U., Madison) ; Cooray, A. (UC, Irvine) et al.
A new and powerful probe of the origin and evolution of structures in the Universe has emerged and been actively developed over the last decade. [...]
arXiv:0902.4759 ; CERN-PH-TH-2009-103.
- 2009. - 8 p.
Preprint - Full text
10.
Cascading Gravity : Extending the Dvali-Gabadadze-Porrati Model to Higher Dimension / de Rham, Claudia (Perimeter Inst. Theor. Phys. ; McMaster U.) ; Dvali, Gia (CERN ; New York U., CCPP) ; Hofmann, Stefan (Perimeter Inst. Theor. Phys. ; Nordita) ; Khoury, Justin (Perimeter Inst. Theor. Phys.) ; Pujolas, Oriol (New York U., CCPP) ; Redi, Michele (New York U., CCPP ; EPFL-ISIC, Lausanne) ; Tolley, Andrew J. (Perimeter Inst. Theor. Phys.)
We present a higher codimension generalization of the DGP scenario which, unlike previous attempts, is free of ghost instabilities. The 4D propagator is made regular by embedding our visible 3-brane within a 4-brane, each with their own induced gravity terms, in a flat 6D bulk. [...]
arXiv:0711.2072.- 2008 - 4 p. - Published in : Phys. Rev. Lett. 100 (2008) 251603 APS Published version, local copy: PDF; Fulltext: PDF; External link: Fulltext

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