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Detection of early-universe gravitational-wave signatures and fundamental physics.
Caldwell, Robert; Cui, Yanou; Guo, Huai-Ke; Mandic, Vuk; Mariotti, Alberto; No, Jose Miguel; Ramsey-Musolf, Michael J; Sakellariadou, Mairi; Sinha, Kuver; Wang, Lian-Tao; White, Graham; Zhao, Yue; An, Haipeng; Bian, Ligong; Caprini, Chiara; Clesse, Sebastien; Cline, James M; Cusin, Giulia; Fornal, Bartosz; Jinno, Ryusuke; Laurent, Benoit; Levi, Noam; Lyu, Kun-Feng; Martinez, Mario; Miller, Andrew L; Redigolo, Diego; Scarlata, Claudia; Sevrin, Alexander; Haghi, Barmak Shams Es; Shu, Jing; Siemens, Xavier; Steer, Danièle A; Sundrum, Raman; Tamarit, Carlos; Weir, David J; Xie, Ke-Pan; Yang, Feng-Wei; Zhou, Siyi.
Afiliação
  • Caldwell R; Department of Physics and Astronomy, Dartmouth College, Hanover, NH 03755 USA.
  • Cui Y; Department of Physics and Astronomy, University of California, Riverside, CA 92521 USA.
  • Guo HK; Department of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112 USA.
  • Mandic V; School of Physics and Astronomy, University of Minnesota, Minneapolis, MN 55455 USA.
  • Mariotti A; Theoretische Natuurkunde and IIHE/ELEM, Vrije Universiteit Brussel, and International Solvay Institutes, Pleinlaan 2, 1050 Brussels, Belgium.
  • No JM; Instituto de Física Teórica UAM/CSIC, C/ Nicolás Cabrera 13- 15, Campus de Cantoblanco, 28049 Madrid, Spain.
  • Ramsey-Musolf MJ; Tsung Dao Lee Institute/Shanghai Jiao Tong University, Shanghai, 200120 People's Republic of China.
  • Sakellariadou M; University of Massachusetts, Amherst, MA 01003 USA.
  • Sinha K; Physics Department, King's College London, Strand, London WC2R 2LS UK.
  • Wang LT; Department of Physics and Astronomy, University of Oklahoma, Norman, OK 73019 USA.
  • White G; Department of Physics, University of Chicago, Chicago, IL 60637 USA.
  • Zhao Y; Kavli IPMU (WPI), UTIAS, The University of Tokyo, Kashiwa, Chiba 277-8583 Japan.
  • An H; Department of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112 USA.
  • Bian L; Department of Physics, Tsinghua University, Beijing, 100084 People's Republic of China.
  • Caprini C; Center for High Energy Physics, Tsinghua University, Beijing, 100084 People's Republic of China.
  • Clesse S; Center for High Energy Physics, Peking University, Beijing, 100871 People's Republic of China.
  • Cline JM; Center for High Energy Physics, Peking University, Beijing, 100871 People's Republic of China.
  • Cusin G; Department of Physics and Chongqing Key Laboratory for Strongly Coupled Physics, Chongqing University, Chongqing, 401331 People's Republic of China.
  • Fornal B; Theoretical Physics Department, University of Geneva, 1211 Geneva, Switzerland.
  • Jinno R; CERN, Theoretical Physics Department, 1 Esplanade des Particules, 1211 Genève 23, Switzerland.
  • Laurent B; Service de Physique Théorique (CP225), University of Brussels (ULB), Boulevard du Triomphe, 1050 Brussels, Belgium.
  • Levi N; Department of Physics, McGill University, Montréal, QC H3A2T8 Canada.
  • Lyu KF; Theoretical Physics Department, University of Geneva, 1211 Geneva, Switzerland.
  • Martinez M; Sorbonne Université, CNRS, UMR 7095, Institut d'Astrophysique de Paris, 75014 Paris, France.
  • Miller AL; Department of Chemistry and Physics, Barry University, Miami Shores, FL 33161 USA.
  • Redigolo D; Instituto de Física Teórica UAM/CSIC, C/ Nicolás Cabrera 13- 15, Campus de Cantoblanco, 28049 Madrid, Spain.
  • Scarlata C; Department of Physics, McGill University, Montréal, QC H3A2T8 Canada.
  • Sevrin A; Raymond and Beverly Sackler School of Physics and Astronomy, Tel-Aviv University, Tel-Aviv, 69978 Israel.
  • Haghi BSE; School of Physics and Astronomy, University of Minnesota, Minneapolis, MN 55455 USA.
  • Shu J; Institut de Física d'Altes Energies, Barcelona Institute of Science and Technology and ICREA, 08193 Barcelona, Spain.
  • Siemens X; Université catholique de Louvain, 1348 Louvain-la-Neuve, Belgium.
  • Steer DA; INFN, Sezione di Firenze Via G. Sansone 1, 50019 Sesto Fiorentino, Italy.
  • Sundrum R; School of Physics and Astronomy, University of Minnesota, Minneapolis, MN 55455 USA.
  • Tamarit C; Theoretische Natuurkunde and IIHE/ELEM, Vrije Universiteit Brussel, and International Solvay Institutes, Pleinlaan 2, 1050 Brussels, Belgium.
  • Weir DJ; Department of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112 USA.
  • Xie KP; CAS Key Laboratory of Theoretical Physics, Insitute of Theoretical Physics, Chinese Academy of Sciences, Beijing, 100190 People's Republic of China.
  • Yang FW; School of Physical Sciences, University of Chinese Academy of Sciences, Beijing, 100049 People's Republic of China.
  • Zhou S; School of Fundamental Physics and Mathematical Sciences, Hangzhou Institute for Advanced Study, University of Chinese Academy of Sciences, Hangzhou, 310024 People's Republic of China.
Gen Relativ Gravit ; 54(12): 156, 2022.
Article em En | MEDLINE | ID: mdl-36465478
ABSTRACT
Detection of a gravitational-wave signal of non-astrophysical origin would be a landmark discovery, potentially providing a significant clue to some of our most basic, big-picture scientific questions about the Universe. In this white paper, we survey the leading early-Universe mechanisms that may produce a detectable signal-including inflation, phase transitions, topological defects, as well as primordial black holes-and highlight the connections to fundamental physics. We review the complementarity with collider searches for new physics, and multimessenger probes of the large-scale structure of the Universe.
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Texto completo: 1 Base de dados: MEDLINE Tipo de estudo: Diagnostic_studies Idioma: En Ano de publicação: 2022 Tipo de documento: Article
Texto completo
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XML
PubMed Links
Buscar no Google

Texto completo: 1 Base de dados: MEDLINE Tipo de estudo: Diagnostic_studies Idioma: En Ano de publicação: 2022 Tipo de documento: Article