1
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Leane RK, Linden T. First Analysis of Jupiter in Gamma Rays and a New Search for Dark Matter. PHYSICAL REVIEW LETTERS 2023; 131:071001. [PMID: 37656854 DOI: 10.1103/physrevlett.131.071001] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 05/24/2021] [Revised: 04/12/2023] [Accepted: 06/23/2023] [Indexed: 09/03/2023]
Abstract
We present the first dedicated γ-ray analysis of Jupiter, using 12 years of data from the Fermi Telescope. We find no robust evidence of γ-ray emission, and set upper limits of ∼10^{-9} GeV cm^{-2} s^{-1} on the Jovian γ-ray flux. We point out that Jupiter is an advantageous dark matter (DM) target due to its large surface area (compared with other solar system planets), and cool core temperature (compared with the Sun). These properties allow Jupiter to both capture and retain lighter DM, providing a complementary probe of sub-GeV DM. We therefore identify and perform a new search for DM-sourced γ-rays in Jupiter, where DM annihilates to long-lived particles, which can escape the Jovian surface and decay into γ rays. We consequently constrain DM-proton scattering cross sections as low as about 10^{-40} cm^{2}, showing Jupiter is up to 10 orders of magnitude more sensitive than direct detection. This sensitivity is reached under the assumption that the mediator decay length is sufficient to escape Jupiter, and the equilibrium between DM capture and annihilation; sensitivities can be lower depending on the DM model. Our work motivates follow-up studies with upcoming MeV telescopes such as AMEGO and e-ASTROGAM.
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Affiliation(s)
- Rebecca K Leane
- SLAC National Accelerator Laboratory, Stanford University, Stanford, California 94035, USA
| | - Tim Linden
- Stockholm University and The Oskar Klein Centre for Cosmoparticle Physics, Alba Nova, 10691 Stockholm, Sweden
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2
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Cappiello CV. Analytic Approach to Light Dark Matter Propagation. PHYSICAL REVIEW LETTERS 2023; 130:221001. [PMID: 37327432 DOI: 10.1103/physrevlett.130.221001] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 02/01/2023] [Revised: 04/28/2023] [Accepted: 05/11/2023] [Indexed: 06/18/2023]
Abstract
If dark matter interacts too strongly with nuclei, it could be slowed to undetectable speeds in Earth's crust or atmosphere before reaching a detector. For sub-GeV dark matter, approximations appropriate for heavier dark matter fail, necessitating the use of computationally expensive simulations. We present a new, analytic approximation for modeling attenuation of light dark matter in Earth. We show that our approach agrees well with Monte Carlo results, and can be much faster at large cross sections. We use this method to reanalyze constraints on subdominant dark matter.
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Affiliation(s)
- Christopher V Cappiello
- Department of Physics, Engineering Physics, and Astronomy, Queen's University, Kingston, Ontario, K7N 3N6, Canada; Arthur B. McDonald Canadian Astroparticle Physics Research Institute, Kingston, Ontario, K7L 3N6, Canada; and Perimeter Institute for Theoretical Physics, Waterloo, Ontario, N2L 2Y5, Canada
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3
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Frumkin R, Kuflik E, Lavie I, Silverwater T. Roadmap to Thermal Dark Matter beyond the Weakly Interacting Dark Matter Unitarity Bound. PHYSICAL REVIEW LETTERS 2023; 130:171001. [PMID: 37172246 DOI: 10.1103/physrevlett.130.171001] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 10/26/2022] [Revised: 01/30/2023] [Accepted: 03/31/2023] [Indexed: 05/14/2023]
Abstract
We study the general properties of the freeze-out of a thermal relic. We give analytic estimates of the relic abundance for an arbitrary freeze-out process, showing when instantaneous freeze-out is appropriate and how it can be corrected when freeze-out is slow. This is used to generalize the relationship between the dark matter mass and coupling that matches the observed abundance. The result encompasses well-studied particular examples, such as weakly interacting massive particles (WIMPs), strongly interacting massive particles, coannihilation, coscattering, inverse decays, and forbidden channels, and generalizes beyond them. In turn, this gives an approximate perturbative unitarity bound on the dark matter mass for an arbitrary thermal freeze-out process. We show that going beyond the maximal masses allowed for freeze-out via dark matter self-annihilations [WIMP-like, m_{DM}≫O(100 TeV)] predicts that there are nearly degenerate states with the dark matter and that the dark matter is generically metastable.
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Affiliation(s)
- Ronny Frumkin
- Racah Institute of Physics, Hebrew University of Jerusalem, Jerusalem 91904, Israel
| | - Eric Kuflik
- Racah Institute of Physics, Hebrew University of Jerusalem, Jerusalem 91904, Israel
| | - Itay Lavie
- Racah Institute of Physics, Hebrew University of Jerusalem, Jerusalem 91904, Israel
| | - Tal Silverwater
- Racah Institute of Physics, Hebrew University of Jerusalem, Jerusalem 91904, Israel
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4
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Bringmann T, Depta PF, Hufnagel M, Ruderman JT, Schmidt-Hoberg K. Dark Matter from Exponential Growth. PHYSICAL REVIEW LETTERS 2021; 127:191802. [PMID: 34797149 DOI: 10.1103/physrevlett.127.191802] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 06/25/2021] [Revised: 08/20/2021] [Accepted: 09/14/2021] [Indexed: 06/13/2023]
Abstract
We propose a novel mechanism for the production of dark matter (DM) from a thermal bath based on the idea that DM particles χ can transform heat bath particles ψ: χψ→χχ. For a small initial abundance of χ, this leads to an exponential growth of the DM number density in close analogy to other familiar exponential growth processes in nature. We demonstrate that this mechanism complements freeze-in and freeze-out production in a generic way, opening new parameter space to explain the observed DM abundance, and we discuss observational prospects for such scenarios.
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Affiliation(s)
- Torsten Bringmann
- Department of Physics, University of Oslo, Box 1048, N-0316 Oslo, Norway
| | - Paul Frederik Depta
- Deutsches Elektronen-Synchrotron DESY, Notkestraße 85, D-22607 Hamburg, Germany
| | - Marco Hufnagel
- Service de Physique Théorique, Université Libre de Bruxelles, Boulevard du Triomphe, CP225, B-1050 Brussels, Belgium
| | - Joshua T Ruderman
- Deutsches Elektronen-Synchrotron DESY, Notkestraße 85, D-22607 Hamburg, Germany
- Center for Cosmology and Particle Physics, Department of Physics, New York University, New York, New York 10003, USA
- Kavli Institute for Theoretical Physics, University of California, Santa Barbara, California 93106, USA
- School of Physics and Astronomy, Tel-Aviv University, Tel-Aviv 69978, Israel
| | - Kai Schmidt-Hoberg
- Deutsches Elektronen-Synchrotron DESY, Notkestraße 85, D-22607 Hamburg, Germany
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Xing CY, Zhu SH. Dark Matter Freeze-Out via Catalyzed Annihilation. PHYSICAL REVIEW LETTERS 2021; 127:061101. [PMID: 34420347 DOI: 10.1103/physrevlett.127.061101] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 02/20/2021] [Revised: 05/31/2021] [Accepted: 07/12/2021] [Indexed: 06/13/2023]
Abstract
We present a new paradigm of dark matter freeze-out, where the annihilation of dark matter particles is catalyzed. We discuss in detail the regime in which the depletion of dark matter proceeds via 2χ→2A^{'} and 3A^{'}→2χ processes, where χ and A^{'} denote dark matter and the catalyst, respectively. In this regime, the dark matter number density is depleted polynomially rather than exponentially (Boltzmann suppression) as in classical weakly interacting massive particles and strongly interacting massive particles. The paradigm applies for a secluded weakly interacting dark sector with dark matter in the MeV-TeV mass range. The catalyzed annihilation paradigm is compatible with cosmic microwave background and big bang nucleosynthesis constraints, with enhanced indirect detection signals.
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Affiliation(s)
- Chuan-Yang Xing
- Department of Physics and State Key Laboratory of Nuclear Physics and Technology, Peking University, Beijing 100871, China
| | - Shou-Hua Zhu
- Department of Physics and State Key Laboratory of Nuclear Physics and Technology, Peking University, Beijing 100871, China
- Collaborative Innovation Center of Quantum Matter, Beijing, 100871, China
- Center for High Energy Physics, Peking University, Beijing 100871, China
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6
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Leane RK, Smirnov J. Exoplanets as Sub-GeV Dark Matter Detectors. PHYSICAL REVIEW LETTERS 2021; 126:161101. [PMID: 33961477 DOI: 10.1103/physrevlett.126.161101] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 10/08/2020] [Revised: 11/28/2020] [Accepted: 03/15/2021] [Indexed: 06/12/2023]
Abstract
We present exoplanets as new targets to discover dark matter (DM). Throughout the Milky Way, DM can scatter, become captured, deposit annihilation energy, and increase the heat flow within exoplanets. We estimate upcoming infrared telescope sensitivity to this scenario, finding actionable discovery or exclusion searches. We find that DM with masses above about an MeV can be probed with exoplanets, with DM-proton and DM-electron scattering cross sections down to about 10^{-37} cm^{2}, stronger than existing limits by up to six orders of magnitude. Supporting evidence of a DM origin can be identified through DM-induced exoplanet heating correlated with galactic position, and hence DM density. This provides new motivation to measure the temperature of the billions of brown dwarfs, rogue planets, and gas giants peppered throughout our Galaxy.
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Affiliation(s)
- Rebecca K Leane
- Center for Theoretical Physics, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
- SLAC National Accelerator Laboratory, Stanford University, Stanford, California 94039, USA
| | - Juri Smirnov
- Center for Cosmology and AstroParticle Physics (CCAPP), The Ohio State University, Columbus, Ohio 43210, USA
- Department of Physics, The Ohio State University, Columbus, Ohio 43210, USA
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7
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Kramer ED, Kuflik E, Levi N, Outmezguine NJ, Ruderman JT. Heavy Thermal Dark Matter from a New Collision Mechanism. PHYSICAL REVIEW LETTERS 2021; 126:081802. [PMID: 33709734 DOI: 10.1103/physrevlett.126.081802] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 05/13/2020] [Revised: 12/02/2020] [Accepted: 02/02/2021] [Indexed: 06/12/2023]
Abstract
We propose a new thermal freeze-out mechanism that results in dark matter masses exceeding the unitarity bound by many orders of magnitude, without violating perturbative unitarity or modifying the standard cosmology. The process determining the relic abundance is χζ^{†}→ζζ, where χ is the dark matter candidate. For m_{ζ}<m_{χ}<3m_{ζ}, χ is cosmologically long-lived and scatters against the exponentially more abundant ζ. Therefore, such a process allows for exponentially heavier dark matter for the same interaction strength as a particle undergoing ordinary 2→2 freeze-out, or equivalently, exponentially weaker interactions for the same mass. We demonstrate this mechanism in a leptophilic dark matter model, which allows for dark matter masses up to 10^{9} GeV.
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Affiliation(s)
- Eric David Kramer
- Racah Institute of Physics, Hebrew University of Jerusalem, Jerusalem 91904, Israel
| | - Eric Kuflik
- Racah Institute of Physics, Hebrew University of Jerusalem, Jerusalem 91904, Israel
| | - Noam Levi
- School of Physics and Astronomy, Tel-Aviv University, Tel-Aviv 69978, Israel
| | | | - Joshua T Ruderman
- Center for Cosmology and Particle Physics, Department of Physics, New York University, New York, New York 10003, USA
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Shakeri S, Hajkarim F, Xue SS. Shedding new light on sterile neutrinos from XENON1T experiment. JOURNAL OF HIGH ENERGY PHYSICS : JHEP 2020; 2020:194. [PMID: 33424225 PMCID: PMC7779899 DOI: 10.1007/jhep12(2020)194] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Figures] [Subscribe] [Scholar Register] [Received: 08/23/2020] [Accepted: 11/15/2020] [Indexed: 06/12/2023]
Abstract
The XENON1T collaboration recently reported the excess of events from recoil electrons, possibly giving an insight into new area beyond the Standard Model (SM) of particle physics. We try to explain this excess by considering effective interactions between the sterile neutrinos and the SM particles. In this paper, we present an effective model based on one-particle-irreducible interaction vertices at low energies that are induced from the SM gauge symmetric four-fermion operators at high energies. The effective interaction strength is constrained by the SM precision measurements, astrophysical and cosmological observations. We introduce a novel effective electromagnetic interaction between sterile neutrinos and SM neutrinos, which can successfully explain the XENON1T event rate through inelastic scattering of the sterile neutrino dark matter from Xenon electrons. We find that sterile neutrinos with masses around 90 keV and specific effective coupling can fit well with the XENON1T data where the best fit points preserving DM constraints and possibly describe the anomalies in other experiments.
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Affiliation(s)
- Soroush Shakeri
- Department of Physics, Isfahan University of Technology, Isfahan, 84156-83111 Iran
- ICRANet-Isfahan, Isfahan University of Technology, Isfahan, 84156-83111 Iran
| | - Fazlollah Hajkarim
- Institut für Theoretische Physik, Goethe Universität, Max von Laue Straße 1, D-60438 Frankfurt am Main, Germany
- Dipartimento di Fisica e Astronomia, Università degli Studi di Padova, Via Marzolo 8, 35131 Padova, Italy
| | - She-Sheng Xue
- ICRANet, Piazzale della Repubblica 10, 65122 Pescara, Italy
- ICRA, Physics Department, La Sapienza University of Rome, P.le Aldo Moro 5, I-00185 Rome, Italy
- INFN, Sezione di Perugia, Via A. Pascoli, 06123 Perugia, Italy
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9
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Kannike K, Raidal M, Veermäe H, Strumia A, Teresi D. Dark matter and the XENON1T electron recoil excess. Int J Clin Exp Med 2020. [DOI: 10.1103/physrevd.102.095002] [Citation(s) in RCA: 39] [Impact Index Per Article: 9.8] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
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10
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Bramante J, Song N. Electric But Not Eclectic: Thermal Relic Dark Matter for the XENON1T Excess. PHYSICAL REVIEW LETTERS 2020; 125:161805. [PMID: 33124868 DOI: 10.1103/physrevlett.125.161805] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 06/30/2020] [Revised: 08/13/2020] [Accepted: 09/21/2020] [Indexed: 06/11/2023]
Abstract
The identity of dark matter is being sought with increasingly sensitive and voluminous underground detectors. Recently the XENON1T Collaboration reported excess electronic recoil events, with most of these having recoil energies around 1-30 keV. We show that a straightforward model of inelastic dark matter produced via early Universe thermal freeze-out annihilation can account for the XENON1T excess. Remarkably, this dark matter model consists of a few simple elements: sub-GeV mass Dirac fermion dark matter coupled to a lighter dark photon kinetically mixed with the standard model photon. A scalar field charged under the dark U(1) gauge symmetry can provide a mass for the dark photon and splits the Dirac fermion component state masses by a few keV, which survive in equal abundance and interact inelastically with electrons and nuclei.
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Affiliation(s)
- Joseph Bramante
- The McDonald Institute and Department of Physics, Engineering Physics, and Astronomy, Queen's University, Kingston, Ontario, K7L 2S8, Canada and Perimeter Institute for Theoretical Physics, Waterloo, Ontario, N2L 2Y5, Canada
| | - Ningqiang Song
- The McDonald Institute and Department of Physics, Engineering Physics, and Astronomy, Queen's University, Kingston, Ontario, K7L 2S8, Canada and Perimeter Institute for Theoretical Physics, Waterloo, Ontario, N2L 2Y5, Canada
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11
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Fornal B, Sandick P, Shu J, Su M, Zhao Y. Boosted Dark Matter Interpretation of the XENON1T Excess. PHYSICAL REVIEW LETTERS 2020; 125:161804. [PMID: 33124870 DOI: 10.1103/physrevlett.125.161804] [Citation(s) in RCA: 7] [Impact Index Per Article: 1.8] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 06/26/2020] [Accepted: 09/09/2020] [Indexed: 06/11/2023]
Abstract
We propose boosted dark matter (BDM) as a possible explanation for the excess of keV electron recoil events observed by XENON1T. BDM particles have velocities much larger than those typical of virialized dark matter, and, as such, BDM-electron scattering can naturally produce keV electron recoils. We show that the required BDM-electron scattering cross sections can be easily realized in a simple model with a heavy vector mediator. Though these cross sections are too large for BDM to escape from the Sun, the BDM flux can originate from the Galactic Center or from halo dark matter annihilations. Furthermore, a daily modulation of the BDM signal will be present, which could not only be used to differentiate it from various backgrounds but would also provide important directional information for the BDM flux.
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Affiliation(s)
- Bartosz Fornal
- Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah 84112, USA
| | - Pearl Sandick
- Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah 84112, USA
| | - Jing Shu
- CAS Key Laboratory of Theoretical Physics, Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing 100190, China
- School of Physical Sciences, University of Chinese Academy of Sciences, Beijing 100049, China
- CAS Center for Excellence in Particle Physics, Beijing 100049, China
- Center for High Energy Physics, Peking University, Beijing 100871, China
- School of Fundamental Physics and Mathematical Sciences, Hangzhou Institute for Advanced Study, University of Chinese Academy of Sciences, Hangzhou 310024, China
- International Centre for Theoretical Physics Asia-Pacific, Beijing/Hangzhou, China
| | - Meng Su
- Department of Physics, The University of Hong Kong, Hong Kong SAR 999077, China
- Laboratory for Space Research, The University of Hong Kong, Hong Kong SAR 999077, China
| | - Yue Zhao
- Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah 84112, USA
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12
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Cai C, Zhang HH, Cacciapaglia G, Rosenlyst M, Frandsen MT. XENON1T solar axion and the Higgs boson emerging from the dark. Int J Clin Exp Med 2020. [DOI: 10.1103/physrevd.102.075018] [Citation(s) in RCA: 12] [Impact Index Per Article: 3.0] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
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13
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Gao C, Liu J, Wang LT, Wang XP, Xue W, Zhong YM. Reexamining the Solar Axion Explanation for the XENON1T Excess. PHYSICAL REVIEW LETTERS 2020; 125:131806. [PMID: 33034473 DOI: 10.1103/physrevlett.125.131806] [Citation(s) in RCA: 6] [Impact Index Per Article: 1.5] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 07/07/2020] [Accepted: 08/28/2020] [Indexed: 06/11/2023]
Abstract
The XENON1T collaboration has observed an excess in electronic recoil events below 5 keV over the known background, which could originate from beyond-the-standard-model physics. The solar axion is a well-motivated model that has been proposed to explain the excess, though it has tension with astrophysical observations. The axions traveling from the Sun can be absorbed by the electrons in the xenon atoms via the axion-electron coupling. Meanwhile, they can also scatter with the atoms through the inverse Primakoff process via the axion-photon coupling, which emits a photon and mimics the electronic recoil signals. We found that the latter process cannot be neglected. After including the keV photon produced via the inverse Primakoff process in the detection, the tension with the astrophysical constraints can be significantly reduced. We also explore scenarios involving additional new physics to further alleviate the tension with the astrophysical bounds.
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Affiliation(s)
- Christina Gao
- Theoretical Physics Department, Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
| | - Jia Liu
- Enrico Fermi Institute, University of Chicago, Chicago, Illinois 60637, USA
- School of Physics and State Key Laboratory of Nuclear Physics and Technology, Peking University, Beijing 100871, China
| | - Lian-Tao Wang
- Enrico Fermi Institute, University of Chicago, Chicago, Illinois 60637, USA
- Department of Physics, University of Chicago, Chicago, Illinois 60637, USA
| | - Xiao-Ping Wang
- HEP Division, Argonne National Laboratory, 9700 Cass Ave., Argonne, Illinois 60439, USA
- School of Physics, Beihang University, Beijing 100083, China
| | - Wei Xue
- Department of Physics, University of Florida, Gainesville, Florida 32611, USA
| | - Yi-Ming Zhong
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
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