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Caldwell R, Cui Y, Guo HK, Mandic V, Mariotti A, No JM, Ramsey-Musolf MJ, Sakellariadou M, Sinha K, Wang LT, White G, Zhao Y, An H, Bian L, Caprini C, Clesse S, Cline JM, Cusin G, Fornal B, Jinno R, Laurent B, Levi N, Lyu KF, Martinez M, Miller AL, Redigolo D, Scarlata C, Sevrin A, Haghi BSE, Shu J, Siemens X, Steer DA, Sundrum R, Tamarit C, Weir DJ, Xie KP, Yang FW, Zhou S. Detection of early-universe gravitational-wave signatures and fundamental physics. GENERAL RELATIVITY AND GRAVITATION 2022; 54:156. [PMID: 36465478 PMCID: PMC9712380 DOI: 10.1007/s10714-022-03027-x] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [Grants] [Track Full Text] [Figures] [Subscribe] [Scholar Register] [Received: 04/23/2022] [Accepted: 10/20/2022] [Indexed: 06/17/2023]
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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Affiliation(s)
- Robert Caldwell
- Department of Physics and Astronomy, Dartmouth College, Hanover, NH 03755 USA
| | - Yanou Cui
- Department of Physics and Astronomy, University of California, Riverside, CA 92521 USA
| | - Huai-Ke Guo
- Department of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112 USA
| | - Vuk Mandic
- School of Physics and Astronomy, University of Minnesota, Minneapolis, MN 55455 USA
| | - Alberto Mariotti
- Theoretische Natuurkunde and IIHE/ELEM, Vrije Universiteit Brussel, and International Solvay Institutes, Pleinlaan 2, 1050 Brussels, Belgium
| | - Jose Miguel No
- Instituto de Física Teórica UAM/CSIC, C/ Nicolás Cabrera 13- 15, Campus de Cantoblanco, 28049 Madrid, Spain
| | - Michael J. Ramsey-Musolf
- Tsung Dao Lee Institute/Shanghai Jiao Tong University, Shanghai, 200120 People’s Republic of China
- University of Massachusetts, Amherst, MA 01003 USA
| | | | - Kuver Sinha
- Department of Physics and Astronomy, University of Oklahoma, Norman, OK 73019 USA
| | - Lian-Tao Wang
- Department of Physics, University of Chicago, Chicago, IL 60637 USA
| | - Graham White
- Kavli IPMU (WPI), UTIAS, The University of Tokyo, Kashiwa, Chiba 277-8583 Japan
| | - Yue Zhao
- Department of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112 USA
| | - Haipeng An
- Department of Physics, Tsinghua University, Beijing, 100084 People’s Republic of China
- Center for High Energy Physics, Tsinghua University, Beijing, 100084 People’s Republic of China
- Center for High Energy Physics, Peking University, Beijing, 100871 People’s Republic of China
| | - Ligong Bian
- Center for High Energy Physics, Peking University, Beijing, 100871 People’s Republic of China
- Department of Physics and Chongqing Key Laboratory for Strongly Coupled Physics, Chongqing University, Chongqing, 401331 People’s Republic of China
| | - Chiara Caprini
- Theoretical Physics Department, University of Geneva, 1211 Geneva, Switzerland
- CERN, Theoretical Physics Department, 1 Esplanade des Particules, 1211 Genève 23, Switzerland
| | - Sebastien Clesse
- Service de Physique Théorique (CP225), University of Brussels (ULB), Boulevard du Triomphe, 1050 Brussels, Belgium
| | - James M. Cline
- Department of Physics, McGill University, Montréal, QC H3A2T8 Canada
| | - Giulia Cusin
- Theoretical Physics Department, University of Geneva, 1211 Geneva, Switzerland
- Sorbonne Université, CNRS, UMR 7095, Institut d’Astrophysique de Paris, 75014 Paris, France
| | - Bartosz Fornal
- Department of Chemistry and Physics, Barry University, Miami Shores, FL 33161 USA
| | - Ryusuke Jinno
- Instituto de Física Teórica UAM/CSIC, C/ Nicolás Cabrera 13- 15, Campus de Cantoblanco, 28049 Madrid, Spain
| | - Benoit Laurent
- Department of Physics, McGill University, Montréal, QC H3A2T8 Canada
| | - Noam Levi
- Raymond and Beverly Sackler School of Physics and Astronomy, Tel-Aviv University, Tel-Aviv, 69978 Israel
| | - Kun-Feng Lyu
- School of Physics and Astronomy, University of Minnesota, Minneapolis, MN 55455 USA
| | - Mario Martinez
- Institut de Física d’Altes Energies, Barcelona Institute of Science and Technology and ICREA, 08193 Barcelona, Spain
| | - Andrew L. Miller
- Université catholique de Louvain, 1348 Louvain-la-Neuve, Belgium
| | - Diego Redigolo
- INFN, Sezione di Firenze Via G. Sansone 1, 50019 Sesto Fiorentino, Italy
| | - Claudia Scarlata
- School of Physics and Astronomy, University of Minnesota, Minneapolis, MN 55455 USA
| | - Alexander Sevrin
- Theoretische Natuurkunde and IIHE/ELEM, Vrije Universiteit Brussel, and International Solvay Institutes, Pleinlaan 2, 1050 Brussels, Belgium
| | - Barmak Shams Es Haghi
- Department of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112 USA
| | - Jing Shu
- CAS Key Laboratory of Theoretical Physics, Insitute of Theoretical Physics, Chinese Academy of Sciences, Beijing, 100190 People’s Republic of China
- School of Physical Sciences, University of Chinese Academy of Sciences, Beijing, 100049 People’s Republic of China
- 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
- International Center for Theoretical Physics Asia-Pacific, Beijing, Hanzhou, People’s Republic of China
| | - Xavier Siemens
- Department of Physics, Oregon State University, Corvallis, OR 97331 USA
| | - Danièle A. Steer
- Laboratoire Astroparticule et Cosmologie, CNRS, Université Paris Cité, 75013 Paris, France
| | | | - Carlos Tamarit
- Physik-Department T70, Technische Universität München, James-Franck-Straße, 85748 Garching, Germany
| | - David J. Weir
- Department of Physics and Helsinki Institute of Physics, University of Helsinki, P.O. Box 64, 00014 Helsinki, Finland
| | - Ke-Pan Xie
- Department of Physics and Astronomy, University of Nebraska, Lincoln, NE 68588 USA
| | - Feng-Wei Yang
- Department of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112 USA
| | - Siyi Zhou
- Department of Physics, Kobe University, Kobe, 657-8501 Japan
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Di Y, Wang J, Zhou R, Bian L, Cai RG, Liu J. Magnetic Field and Gravitational Waves from the First-Order Phase Transition. PHYSICAL REVIEW LETTERS 2021; 126:251102. [PMID: 34241495 DOI: 10.1103/physrevlett.126.251102] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 02/06/2021] [Accepted: 05/27/2021] [Indexed: 06/13/2023]
Abstract
We perform the three-dimensional lattice simulation of the magnetic field and gravitational wave productions from bubble collisions during the first-order electroweak phase transition. Except for the gravitational wave, the power-law spectrum of the magnetic field strength is numerically calculated for the first time, which is of a broken power-law spectrum: B_{ξ}∝f^{0.91} for the low-frequency region of f<f_{⋆} and B_{ξ}∝f^{-1.65} for the high-frequency region of f>f_{⋆} in the thin-wall limit, with the peak frequency being f_{⋆}∼5 Hz at the phase transition temperature 100 GeV. When the hydrodynamics is taken into account, the generated magnetic field strength can reach B_{ξ}∼10^{-7} G at a correlation length ξ∼10^{-7} pc, which may seed the large scale magnetic fields. Our study shows that the measurements of cosmic magnetic field strength and gravitational waves are complementary to probe new physics admitting electroweak phase transition.
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Affiliation(s)
- Yuefeng Di
- Department of Physics, Chongqing University, Chongqing 401331, China
| | - Jialong Wang
- Department of Physics, Chongqing University, Chongqing 401331, China
| | - Ruiyu Zhou
- Department of Physics, Chongqing University, Chongqing 401331, China
| | - Ligong Bian
- Department of Physics, Chongqing University, Chongqing 401331, China
| | - Rong-Gen Cai
- CAS Key Laboratory of Theoretical Physics, Institute of Theoretical Physics, Chinese Academy of Sciences, P.O. Box 2735, Beijing 100190, China, School of Physical Sciences, University of Chinese Academy of Sciences, No. 19A Yuquan Road, Beijing 100049, China, and School of Fundamental Physics and Mathematical Sciences, Hangzhou Institute for Advanced Study, University of Chinese Academy of Sciences, Hangzhou 310024, China
| | - Jing Liu
- School of Fundamental Physics and Mathematical Sciences, Hangzhou Institute for Advanced Study, University of Chinese Academy of Sciences, Hangzhou 310024, China and School of Physical Sciences, University of Chinese Academy of Sciences, Beijing 100049, China
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Abstract
Gravitational waves (GWs) produced by sound waves in the primordial plasma during a strong first-order phase transition in the early Universe are going to be a main target of the upcoming Laser Interferometer Space Antenna (LISA) experiment. In this short note, I draw a global picture of LISA’s expected sensitivity to this type of GW signal, based on the concept of peak-integrated sensitivity curves (PISCs) recently introduced in two previous papers. In particular, I use LISA’s PISC to perform a systematic comparison of several thousands of benchmark points in ten different particle physics models in a compact fashion. The presented analysis (i) retains the complete information on the optimal signal-to-noise ratio, (ii) allows for different power-law indices describing the spectral shape of the signal, (iii) accounts for galactic confusion noise from compact binaries, and (iv) exhibits the dependence of the expected sensitivity on the collected amount of data. An important outcome of this analysis is that, for the considered set of models, galactic confusion noise typically reduces the number of observable scenarios by roughly a factor of two, more or less independent of the observing time. The numerical results presented in this paper are also available in the online repository Zenodo.
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Abstract
Symmetries at finite temperature are of great importance to understand dynamics of spontaneous symmetry breaking phenomena, especially phase transitions in early Universe. Some symmetries such as the electroweak symmetry can be restored in hot environment. However, it is a nontrivial question that the phase transition occurs via first or second order, or even smooth crossover, which strongly depends on underlying physics. If it is first order, gravitational waves can be generated, providing a detectable signal of this epoch. Moreover, the baryon asymmetry of the Universe can also arise under some conditions. In this article, the electroweak phase transition is reviewed, focusing particularly on the case of the first-order phase transition. Much attention is paid to multi-step phase transitions in which additional symmetry breaking such as a spontaneous Z 2 breaking plays a pivotal role in broadening the possibility of the first-order electroweak phase transition. On the technical side, we review thermal resummation that mitigates a bad infrared behavior related to the symmetry restoration. In addition, gauge and scheme dependences of perturbative calculations are also briefly discussed.
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Krauss ME, Opferkuch T, Staub F. The ultraviolet landscape of two-Higgs doublet models. THE EUROPEAN PHYSICAL JOURNAL. C, PARTICLES AND FIELDS 2018; 78:1020. [PMID: 30872961 PMCID: PMC6383873 DOI: 10.1140/epjc/s10052-018-6489-2] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Figures] [Subscribe] [Scholar Register] [Received: 08/01/2018] [Accepted: 11/30/2018] [Indexed: 06/09/2023]
Abstract
We study the predictions of generic ultraviolet completions of two-Higgs doublet models. We assume that at the matching scale between the two-Higgs doublet model and an ultraviolet complete theory - which can be anywhere between the TeV and the Planck scale - arbitrary but perturbative values for the quartic couplings are present. We evaluate the couplings down from the matching scale to the weak scale and study the predictions for the scalar mass spectrum. In particular, we show the importance of radiative corrections which are essential for both an accurate Higgs mass calculation as well as determining the stability of the electroweak vacuum. We study the relation between the mass splitting of the heavy Higgs states and the size of the quartic couplings at the matching scale, finding that only a small class of models exhibit sizeable mass splittings between the heavy scalars at the weak scale. Moreover, we find a clear correlation between the maximal size of the couplings and the considered matching scale.
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Affiliation(s)
- Manuel E. Krauss
- Bethe Center for Theoretical Physics and Physikalisches Institut derUniversität Bonn, Nußallee 12, 53115 Bonn, Germany
| | - Toby Opferkuch
- PRISMA Cluster of Excellence and Mainz Institute for Theoretical Physics, Johannes Gutenberg-Universität Mainz, 55099 Mainz, Germany
| | - Florian Staub
- Institute for Theoretical Physics (ITP), Karlsruhe Institute of Technology, Engesserstraße 7, 76128 Karlsruhe, Germany
- Institute for Nuclear Physics (IKP), Karlsruhe Institute of Technology, Hermann-von-Helmholtz-Platz 1, 76344 Eggenstein-Leopoldshafen, Germany
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Andersen JO, Gorda T, Helset A, Niemi L, Tenkanen TVI, Tranberg A, Vuorinen A, Weir DJ. Nonperturbative Analysis of the Electroweak Phase Transition in the Two Higgs Doublet Model. PHYSICAL REVIEW LETTERS 2018; 121:191802. [PMID: 30468614 DOI: 10.1103/physrevlett.121.191802] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 01/15/2018] [Revised: 09/21/2018] [Indexed: 06/09/2023]
Abstract
We perform a nonperturbative study of the electroweak phase transition (EWPT) in the two Higgs doublet model (2HDM) by deriving a dimensionally reduced high-temperature effective theory for the model, and matching to known results for the phase diagram of the effective theory. We find regions of the parameter space where the theory exhibits a first-order phase transition. In particular, our findings are consistent with previous perturbative results suggesting that the primary signature of a first-order EWPT in the 2HDM is m_{A_{0}}>m_{H_{0}}+m_{Z}.
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Affiliation(s)
- Jens O Andersen
- Department of Physics, Faculty of Natural Sciences, Norwegian University of Science and Technology, Høgskoleringen 5, N-7491 Trondheim, Norway
| | - Tyler Gorda
- Department of Physics and Helsinki Institute of Physics, P.O. Box 64, FI-00014 University of Helsinki, Finland
- Department of Physics, University of Virginia, 382 McCormick Road, Charlottesville, Virginia 22904-4714, USA
| | - Andreas Helset
- Department of Physics, Faculty of Natural Sciences, Norwegian University of Science and Technology, Høgskoleringen 5, N-7491 Trondheim, Norway
- Niels Bohr Institute, University of Copenhagen, Blegdamsvej 17, 2100 Copenhagen
| | - Lauri Niemi
- Department of Physics and Helsinki Institute of Physics, P.O. Box 64, FI-00014 University of Helsinki, Finland
| | - Tuomas V I Tenkanen
- Department of Physics and Helsinki Institute of Physics, P.O. Box 64, FI-00014 University of Helsinki, Finland
| | - Anders Tranberg
- Department of Mathematics and Physics, University of Stavanger, 4036 Stavanger, Norway
| | - Aleksi Vuorinen
- Department of Physics and Helsinki Institute of Physics, P.O. Box 64, FI-00014 University of Helsinki, Finland
| | - David J Weir
- Department of Physics and Helsinki Institute of Physics, P.O. Box 64, FI-00014 University of Helsinki, Finland
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