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CERN Document Server 8 записей найдено  Поиск длился 1.36 секунд. 
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Cold-atom analogues of vacuum decay / Jenkins, Alexander (speaker) (University College London)
2024 - 2006. Eucapt Conferences; 4th EuCAPT Annual Symposium External links: Talk details; Event details In : 4th EuCAPT Annual Symposium
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Improving access to radiotherapy in LMICs through a collaborative initiative to reduce technology downtime / Ige, Taofeeq A (Natl. Hospital Abuja, Nigeria ; Lancaster U.) ; Jenkins, Alexander (Lancaster U. ; Oxford U.) ; Dosanjh, Manjit (Lancaster U. ; Oxford U. ; Internatl. Cancer Expert Corps, Washington) ; O’Brien, Donna (Internatl. Cancer Expert Corps, Washington) ; Pistenmaa, David (Lancaster U. ; Internatl. Cancer Expert Corps, Washington) ; Coleman, C Norman (Internatl. Cancer Expert Corps, Washington)
This chapter covers approaches that aim to increase access to radiotherapy care in Africa by reducing machine downtime. It includes a survey design covering this issue across Africa..
2022 - 10 p. - Published in : 10.1088/978-0-7503-3075-6ch21
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Science with the Einstein Telescope: a comparison of different designs / Branchesi, Marica (GSSI, Aquila ; Gran Sasso) ; Maggiore, Michele (Geneva U., Dept. Theor. Phys. ; Geneva U.) ; Alonso, David (Oxford U.) ; Badger, Charles (King's Coll. London) ; Banerjee, Biswajit (GSSI, Aquila ; Gran Sasso) ; Beirnaert, Freija (Gent U.) ; Belgacem, Enis (Geneva U.) ; Bhagwat, Swetha (Rome U. ; Birmingham U.) ; Boileau, Guillaume (U. Antwerp (main) ; ARTEMIS, Nice) ; Borhanian, Ssohrab (Jena U., TPI) et al.
The Einstein Telescope (ET), the European project for a third-generation gravitational-wave detector, has a reference configuration based on a triangular shape consisting of three nested detectors with 10 km arms, where in each arm there is a `xylophone' configuration made of an interferometer tuned toward high frequencies, and an interferometer tuned toward low frequencies and working at cryogenic temperature. Here, we examine the scientific perspectives under possible variations of this reference design. [...]
arXiv:2303.15923; ET-0084A-23.- 2023-07-28 - 197 p. - Published in : JCAP 2307 (2023) 068 Fulltext: document - PDF; 2303.15923 - PDF;
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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
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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;
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CLASS_GWB: robust modeling of the astrophysical gravitational wave background anisotropies / Bellomo, Nicola (Texas U. ; U. Barcelona (main)) ; Bertacca, Daniele (U. Padua (main) ; INFN, Padua ; Padua Observ.) ; Jenkins, Alexander C. (King's Coll. London) ; Matarrese, Sabino (U. Padua (main) ; INFN, Padua ; Padua Observ. ; GSSI, Aquila) ; Raccanelli, Alvise (U. Padua (main) ; INFN, Padua ; CERN) ; Regimbau, Tania (Annecy, LAPP) ; Ricciardone, Angelo (U. Padua (main) ; INFN, Padua) ; Sakellariadou, Mairi (King's Coll. London)
Gravitational radiation offers a unique possibility to study the large-scale structure of the Universe, gravitational wave sources and propagation in a completely novel way. Given that gravitational wave maps contain a wealth of astrophysical and cosmological information, interpreting this signal requires a non-trivial multidisciplinary approach. [...]
arXiv:2110.15059; KCL-PH-TH-2021-70.- 2022-06-27 - 58 p. - Published in : JCAP 2206 (2022) 030 Fulltext: PDF;
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Nonlinear gravitational-wave memory from cusps and kinks on cosmic strings / Jenkins, Alexander C. (King's Coll. London) ; Sakellariadou, Mairi (King's Coll. London ; CERN)
The nonlinear memory effect is a fascinating prediction of general relativity (GR), in which oscillatory gravitational-wave (GW) signals are generically accompanied by a monotonically-increasing strain which persists in the detector long after the signal has passed. This effect presents a unique opportunity to test GR in the dynamical and nonlinear regime. [...]
arXiv:2102.12487; KCL-PH-TH/2021-04; CERN-TH-2021-016.- 2021-07-22 - 29 p. - Published in : Class. Quantum Gravity 38 (2021) 165004 Fulltext: document - HTM; 2102.12487 - PDF; Fulltext from publisher: PDF;
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Projection effects on the observed angular spectrum of the astrophysical stochastic gravitational wave background / Bertacca, Daniele (U. Padua, Dept. Phys. Astron. ; INFN, Padua ; Padua Observ.) ; Ricciardone, Angelo (INFN, Padua) ; Bellomo, Nicola (ICC, Barcelona U.) ; Jenkins, Alexander C. (King's Coll. London) ; Matarrese, Sabino (U. Padua, Dept. Phys. Astron. ; INFN, Padua ; Padua Observ. ; GSSI, Aquila) ; Raccanelli, Alvise (CERN) ; Regimbau, Tania (Annecy, LAPP) ; Sakellariadou, Mairi (King's Coll. London)
The detection and characterization of the Stochastic Gravitational Wave Background (SGWB) is one of the main goals of Gravitational Wave (GW) experiments. The observed SGWB will be the combination of GWs from cosmological (as predicted by many models describing the physics of the early Universe) and astrophysical origins, which will arise from the superposition of GWs from unresolved sources whose signal is too faint to be detected. [...]
arXiv:1909.11627; CERN-TH-2019-153; KCL-PH-TH 2019-73.- 2020-05-12 - 15 p. - Published in : Phys. Rev. D 101 (2020) 103513 Fulltext: PDF; Fulltext from Publisher: PDF; Fulltext from publisher: PDF;
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