Zobrazeno 1 - 10
of 43
pro vyhledávání: '"Bradley J Kavanagh"'
Publikováno v:
Journal of High Energy Physics, Vol 2019, Iss 4, Pp 1-46 (2019)
Abstract Even if Dark Matter (DM) is neutral under electromagnetism, it can still interact with the Standard Model (SM) via photon exchange from higher-dimensional operators. Here we classify the general effective operators coupling DM to photons, di
Externí odkaz:
https://doaj.org/article/83f2539c64084d5bb1e9375a342a0c7c
Publikováno v:
Journal of High Energy Physics, Vol 2017, Iss 10, Pp 1-24 (2017)
Abstract It was recently pointed out that direct detection signals from at least three different targets may be used to determine whether the Dark Matter (DM) particle is different from its antiparticle. In this work, we examine in detail the feasibi
Externí odkaz:
https://doaj.org/article/e048038ce01e46fb9e76b264a42568e7
Publikováno v:
Physics Letters B, Vol 771, Iss , Pp 339-348 (2017)
We study vector portal dark matter models where the mediator couples only to leptons. In spite of the lack of tree-level couplings to colored states, radiative effects generate interactions with quark fields that could give rise to a signal in curren
Externí odkaz:
https://doaj.org/article/e8e562d968eb441ab27e4409a3390378
Publikováno v:
SciPost Physics Core, Vol 3, Iss 2, p 007 (2020)
In this white paper, we discuss the prospects for characterizing and identifying dark matter using gravitational waves, covering a wide range of dark matter candidate types and signals. We argue that present and upcoming gravitational wave probes
Externí odkaz:
https://doaj.org/article/6a7be950be014d12ac5a41928a0456b7
Autor:
Sebastian Baum, Patrick Stengel, Natsue Abe, Javier F. Acevedo, Gabriela R. Araujo, Yoshihiro Asahara, Frank Avignone, Levente Balogh, Laura Baudis, Yilda Boukhtouchen, Joseph Bramante, Pieter Alexander Breur, Lorenzo Caccianiga, Francesco Capozzi, Juan I. Collar, Reza Ebadi, Thomas Edwards, Klaus Eitel, Alexey Elykov, Rodney C. Ewing, Katherine Freese, Audrey Fung, Claudio Galelli, Ulrich A. Glasmacher, Arianna Gleason, Noriko Hasebe, Shigenobu Hirose, Shunsaku Horiuchi, Yasushi Hoshino, Patrick Huber, Yuki Ido, Yohei Igami, Norito Ishikawa, Yoshitaka Itow, Takashi Kamiyama, Takenori Kato, Bradley J. Kavanagh, Yoji Kawamura, Shingo Kazama, Christopher J. Kenney, Ben Kilminster, Yui Kouketsu, Yukiko Kozaka, Noah A. Kurinsky, Matthew Leybourne, Thalles Lucas, William F. McDonough, Mason C. Marshall, Jose Maria Mateos, Anubhav Mathur, Katsuyoshi Michibayashi, Sharlotte Mkhonto, Kohta Murase, Tatsuhiro Naka, Kenji Oguni, Surjeet Rajendran, Hitoshi Sakane, Paola Sala, Kate Scholberg, Ingrida Semenec, Takuya Shiraishi, Joshua Spitz, Kai Sun, Katsuhiko Suzuki, Erwin H. Tanin, Aaron Vincent, Nikita Vladimirov, Ronald L. Walsworth, Hiroko Watanabe
Minerals are solid state nuclear track detectors - nuclear recoils in a mineral leave latent damage to the crystal structure. Depending on the mineral and its temperature, the damage features are retained in the material from minutes (in low-melting
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::39661f426cd2f86bd735040b6a3d8100
Autor:
K. G. Arun, Enis Belgacem, Robert Benkel, Laura Bernard, Emanuele Berti, Gianfranco Bertone, Marc Besancon, Diego Blas, Christian G. Böhmer, Richard Brito, Gianluca Calcagni, Alejandro Cardenas-Avendaño, Katy Clough, Marco Crisostomi, Valerio De Luca, Daniela Doneva, Stephanie Escoffier, José María Ezquiaga, Pedro G. Ferreira, Pierre Fleury, Stefano Foffa, Gabriele Franciolini, Noemi Frusciante, Juan García-Bellido, Carlos Herdeiro, Thomas Hertog, Tanja Hinderer, Philippe Jetzer, Lucas Lombriser, Elisa Maggio, Michele Maggiore, Michele Mancarella, Andrea Maselli, Sourabh Nampalliwar, David Nichols, Maria Okounkova, Paolo Pani, Vasileios Paschalidis, Alvise Raccanelli, Lisa Randall, Sébastien Renaux-Petel, Antonio Riotto, Milton Ruiz, Alexander Saffer, Mairi Sakellariadou, Ippocratis D. Saltas, B. S. Sathyaprakash, Lijing Shao, Carlos F. Sopuerta, Thomas P. Sotiriou, Nikolaos Stergioulas, Nicola Tamanini, Filippo Vernizzi, Helvi Witek, Kinwah Wu, Kent Yagi, Stoytcho Yazadjiev, Nicolás Yunes, Miguel Zilhão, Niayesh Afshordi, Marie-Christine Angonin, Vishal Baibhav, Enrico Barausse, Tiago Barreiro, Nicola Bartolo, Nicola Bellomo, Ido Ben-Dayan, Eric A. Bergshoeff, Sebastiano Bernuzzi, Daniele Bertacca, Swetha Bhagwat, Béatrice Bonga, Lior M. Burko, Geoffrey Compére, Giulia Cusin, Antonio da Silva, Saurya Das, Claudia de Rham, Kyriakos Destounis, Ema Dimastrogiovanni, Francisco Duque, Richard Easther, Hontas Farmer, Matteo Fasiello, Stanislav Fisenko, Kwinten Fransen, Jörg Frauendiener, Jonathan Gair, László Árpád Gergely, Davide Gerosa, Leonardo Gualtieri, Wen-Biao Han, Aurelien Hees, Thomas Helfer, Jörg Hennig, Alexander C. Jenkins, Eric Kajfasz, Nemanja Kaloper, Vladimír Karas, Bradley J. Kavanagh, Sergei A. Klioner, Savvas M. Koushiappas, Macarena Lagos, Christophe Le Poncin-Lafitte, Francisco S. N. Lobo, Charalampos Markakis, Prado Martín-Moruno, C. J. A. P. Martins, Sabino Matarrese, Daniel R. Mayerson, José P. Mimoso, Johannes Noller, Nelson J. Nunes, Roberto Oliveri, Giorgio Orlando, George Pappas, Igor Pikovski, Luigi Pilo, Jiří Podolský, Geraint Pratten, Tomislav Prokopec, Hong Qi, Saeed Rastgoo, Angelo Ricciardone, Rocco Rollo, Diego Rubiera-Garcia, Olga Sergijenko, Stuart Shapiro, Deirdre Shoemaker, Alessandro Spallicci, Oleksandr Stashko, Leo C. Stein, Gianmassimo Tasinato, Andrew J. Tolley, Elias C. Vagenas, Stefan Vandoren, Daniele Vernieri, Rodrigo Vicente, Toby Wiseman, Valery I. Zhdanov, Miguel Zumalacárregui
Publikováno v:
Living Reviews in Relativity, 25(1), 1. Albert Einstein Institut
Living Reviews in Relativity
Living Rev.Rel.
Living Rev.Rel., 2022, 25 (1), pp.4. ⟨10.1007/s41114-022-00036-9⟩
E-Prints Complutense. Archivo Institucional de la UCM
instname
Arun, K. G. Ruiz Meneses, Milton Javier 2022 New horizons for fundamental physics with LISA Living Reviews In Relativity 25 4
Living Reviews in Relativity, 25, 1-148
Living Reviews in Relativity, 25(1):4. Albert Einstein Institut
Living Reviews in Relativity, 25, 1, pp. 1-148
Living Reviews in Relativity
Living Rev.Rel.
Living Rev.Rel., 2022, 25 (1), pp.4. ⟨10.1007/s41114-022-00036-9⟩
E-Prints Complutense. Archivo Institucional de la UCM
instname
Arun, K. G. Ruiz Meneses, Milton Javier 2022 New horizons for fundamental physics with LISA Living Reviews In Relativity 25 4
Living Reviews in Relativity, 25, 1-148
Living Reviews in Relativity, 25(1):4. Albert Einstein Institut
Living Reviews in Relativity, 25, 1, pp. 1-148
K. G. Arun et al.
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. I
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. I
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6ee753d4ce141fae6dca78bfdba343d8
https://orca.cardiff.ac.uk/id/eprint/150937/1/41114_2022_Article_36.pdf
https://orca.cardiff.ac.uk/id/eprint/150937/1/41114_2022_Article_36.pdf
Publikováno v:
Physical Review D, 105(4):043009. American Institute of Physics
Digital.CSIC. Repositorio Institucional del CSIC
instname
Digital.CSIC. Repositorio Institucional del CSIC
instname
Large dark matter overdensities can form around black holes of astrophysical and primordial origin as they form and grow. This “dark dress” inevitably affects the dynamical evolution of binary systems and induces a dephasing in the gravitational
Autor:
Matteo Martinelli, Francesca Scarcella, Natalie B. Hogg, Bradley J. Kavanagh, Daniele Gaggero, Pierre Fleury
Publikováno v:
JCAP
JCAP, 2022, 08 (08), pp.006. ⟨10.1088/1475-7516/2022/08/006⟩
JCAP, 2022, 08 (08), pp.006. ⟨10.1088/1475-7516/2022/08/006⟩
Primordial black holes (PBHs) are compact objects proposed to have formed in the early Universe from the collapse of small-scale over-densities. Their existence may be detected from the observation of gravitational waves (GWs) emitted by PBH mergers,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5e0331a7ff59358cb72537a57003a9f5
Autor:
Beatriz Aja, Sergio Arguedas Cuendis, Ivan Arregui, Eduardo Artal, R. Belén Barreiro, Francisco J. Casas, Marina C. de Ory, Alejandro Díaz-Morcillo, Luisa de la Fuente, Juan Daniel Gallego, Jose María García-Barceló, Benito Gimeno, Alicia Gomez, Daniel Granados, Bradley J. Kavanagh, Miguel A.G. Laso, Txema Lopetegi, Antonio José Lozano-Guerrero, Maria T. Magaz, Jesús Martín-Pintado, Enrique Martínez-González, Jordi Miralda-Escudé, Juan Monzó-Cabrera, Francisco Najarro de la Parra, Jose R. Navarro-Madrid, Ana B. Nuñez Chico, Juan Pablo Pascual, Jorge Pelegrin, Carlos Peña Garay, David Rodriguez, Juan M. Socuéllamos, Fernando Teberio, Jorge Teniente, Patricio Vielva, Iván Vila, Rocío Vilar, Enrique Villa
We propose a novel experiment, the Canfranc Axion Detection Experiment (CADEx), to probe dark matter axions with masses in the range 330–460 μeV, within the W-band (80–110 GHz), an unexplored parameter space in the well-motivated dark matter win
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2d7177d995e6d08e6b79d88c8738dbc3
https://hdl.handle.net/2454/45319
https://hdl.handle.net/2454/45319
Publikováno v:
Physical Review Letters
Digital.CSIC. Repositorio Institucional del CSIC
instname
Digital.CSIC. Repositorio Institucional del CSIC
instname
In many cosmologies dark matter clusters on subkiloparsec scales and forms compact subhalos, in which the majority of Galactic dark matter could reside. Null results in direct detection experiments since their advent four decades ago could then be th