{"title":"Estimating high-order time derivatives of Kerr orbital functionals","authors":"Lennox S. Keeble, Alejandro Cárdenas-Avendaño","doi":"10.1103/g26m-mz4v","DOIUrl":"https://doi.org/10.1103/g26m-mz4v","url":null,"abstract":"","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"95 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-10-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145311279","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Xiao-Dong Cheng, Zhen-Lu Weng, Ying-Ying Fan, Ru-Min Wang
{"title":"Estimating CP violation in Bc→BK0+BK¯0→Bπ±e∓νe decays","authors":"Xiao-Dong Cheng, Zhen-Lu Weng, Ying-Ying Fan, Ru-Min Wang","doi":"10.1103/r98k-2ctc","DOIUrl":"https://doi.org/10.1103/r98k-2ctc","url":null,"abstract":"In this paper, we investigate the C</a:mi>P</a:mi></a:math> asymmetries <c:math xmlns:c=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><c:msubsup><c:mi mathvariant=\"script\">A</c:mi><c:mrow><c:mi>C</c:mi><c:mi>P</c:mi></c:mrow><c:mrow><c:mi>p</c:mi><c:mi>m</c:mi></c:mrow></c:msubsup></c:math> and <f:math xmlns:f=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><f:msubsup><f:mi mathvariant=\"script\">A</f:mi><f:mrow><f:mi>C</f:mi><f:mi>P</f:mi></f:mrow><f:mrow><f:mi>m</f:mi><f:mi>p</f:mi></f:mrow></f:msubsup></f:math> in <i:math xmlns:i=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><i:msubsup><i:mi>B</i:mi><i:mi>c</i:mi><i:mo>±</i:mo></i:msubsup><i:mo stretchy=\"false\">→</i:mo><i:msup><i:mi>B</i:mi><i:mo>±</i:mo></i:msup><i:msup><i:mi>K</i:mi><i:mn>0</i:mn></i:msup><i:mo>+</i:mo><i:msup><i:mi>B</i:mi><i:mo>±</i:mo></i:msup><i:msup><i:mover accent=\"true\"><i:mi>K</i:mi><i:mo stretchy=\"false\">¯</i:mo></i:mover><i:mn>0</i:mn></i:msup><i:mo stretchy=\"false\">→</i:mo><i:msup><i:mi>B</i:mi><i:mo>±</i:mo></i:msup><i:msup><i:mi>π</i:mi><i:mo>±</i:mo></i:msup><i:msup><i:mi>e</i:mi><i:mo>∓</i:mo></i:msup><i:msub><i:mi>ν</i:mi><i:mi>e</i:mi></i:msub></i:math> and <o:math xmlns:o=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><o:msubsup><o:mi>B</o:mi><o:mi>c</o:mi><o:mo>±</o:mo></o:msubsup><o:mo stretchy=\"false\">→</o:mo><o:msup><o:mi>B</o:mi><o:mo>±</o:mo></o:msup><o:msup><o:mi>K</o:mi><o:mn>0</o:mn></o:msup><o:mo>+</o:mo><o:msup><o:mi>B</o:mi><o:mo>±</o:mo></o:msup><o:msup><o:mover accent=\"true\"><o:mi>K</o:mi><o:mo stretchy=\"false\">¯</o:mo></o:mover><o:mn>0</o:mn></o:msup><o:mo stretchy=\"false\">→</o:mo><o:msup><o:mi>B</o:mi><o:mo>±</o:mo></o:msup><o:msup><o:mi>π</o:mi><o:mo>∓</o:mo></o:msup><o:msup><o:mi>e</o:mi><o:mo>±</o:mo></o:msup><o:msub><o:mi>ν</o:mi><o:mi>e</o:mi></o:msub></o:math> decays; both of them consist of three parts: the indirect <u:math xmlns:u=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><u:mi>C</u:mi><u:mi>P</u:mi></u:math> violations in <w:math xmlns:w=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><w:msup><w:mi>K</w:mi><w:mn>0</w:mn></w:msup><w:mo>−</w:mo><w:msup><w:mover accent=\"true\"><w:mi>K</w:mi><w:mo stretchy=\"false\">¯</w:mo></w:mover><w:mn>0</w:mn></w:msup></w:math> mixing A</ab:mi>C</ab:mi>P</ab:mi>,</ab:mo>mix</ab:mi></ab:mrow>p</ab:mi>m</ab:mi></ab:mrow></ab:msubsup></ab:math> and <cb:math xmlns:cb=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><cb:msubsup><cb:mi>A</cb:mi><cb:mrow><cb:mi>C</cb:mi><cb:mi>P</cb:mi><cb:mo>,</cb:mo><cb:mi>mix</cb:mi></cb:mrow><cb:mrow><cb:mi>m</cb:mi><cb:mi>p</cb:mi></cb:mrow></cb:msubsup></cb:math>, the direct <eb:math xmlns:eb=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><eb:mi>C</eb:mi><eb:mi>P</eb:mi></eb:math> violations in <gb:math xmlns:gb=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><gb:msub><gb:mi>B</gb:mi><gb:mi>c</gb:mi></gb:msub></gb:math> decay <ib:math xmlns:ib=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><ib:msubsu","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"12 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-10-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145311415","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Rapid inference for individual binaries and a stochastic background with pulsar timing array data","authors":"Aiden Gundersen, Neil J. Cornish","doi":"10.1103/5xh1-kgtk","DOIUrl":"https://doi.org/10.1103/5xh1-kgtk","url":null,"abstract":"","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"131 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-10-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145311437","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Else Magnus, Jannes Loonen, Rose S. Stanley, Krijn D. de Vries, Nick van Eijndhoven, Paul Coppin
{"title":"Average power-density spectrum of short and long Fermi-GBM gamma-ray bursts","authors":"Else Magnus, Jannes Loonen, Rose S. Stanley, Krijn D. de Vries, Nick van Eijndhoven, Paul Coppin","doi":"10.1103/9gtg-bwfy","DOIUrl":"https://doi.org/10.1103/9gtg-bwfy","url":null,"abstract":"","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"131 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-10-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145311562","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Superfluids in expanding backgrounds and attractor times","authors":"Guri K. Buza, Toshali Mitra, Alexander Soloviev","doi":"10.1103/45fr-wb1w","DOIUrl":"https://doi.org/10.1103/45fr-wb1w","url":null,"abstract":"We determine the behavior of an out-of-equilibrium superfluid, composed of a U</a:mi>(</a:mo>1</a:mn>)</a:mo></a:math> Goldstone mode coupled to hydrodynamic modes in a Müller-Israel-Stewart theory, in expanding backgrounds relevant to heavy ion collision experiments and cosmology. For suitable initial conditions, the evolution of the hydrodynamic variables leads to a change in the potential of the Goldstone mode, spontaneously breaking the symmetry. After some time, the condensate becomes small, leading the system evolution to be well described via hydrodynamic attractors for a timescale that we determine in Bjorken and Gubser flows. We define this new timescale as the and show its dependence on initial conditions. In the case of the Gubser flow, we provide for the first time a complete description of the nonlinear evolution of the system, including a novel nonlinear regime of constant anisotropy not found in the Bjorken evolution. Finally, we consider the superfluid in the dynamical Friedmann-Lemaitre-Roberston-Walker (FLRW) background, where we observe a similar attractor behavior, dependent on the initial conditions, that at late times approaches a regime dominated by the condensate.","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"35 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-10-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145311564","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
André G. da Silva, Dyana C. Duarte, Ricardo L. S. Farias, Marcus Benghi Pinto, Rudnei O. Ramos, William R. Tavares
{"title":"Two-flavor chirally imbalanced quark matter beyond large Nc","authors":"André G. da Silva, Dyana C. Duarte, Ricardo L. S. Farias, Marcus Benghi Pinto, Rudnei O. Ramos, William R. Tavares","doi":"10.1103/cks2-8m69","DOIUrl":"https://doi.org/10.1103/cks2-8m69","url":null,"abstract":"We investigate a chirally imbalanced medium in the context of the two-flavor Nambu-Jona-Lasinio model using both the large-N</a:mi>c</a:mi></a:msub></a:math> (LN) and beyond large-<c:math xmlns:c=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><c:msub><c:mi>N</c:mi><c:mi>c</c:mi></c:msub></c:math> (BLN) approximations. To incorporate BLN effects, we consider the optimized perturbation theory (OPT) to the first nontrivial order, which includes two-loop (exchange) contributions. This procedure allows us to explicitly explore how finite <e:math xmlns:e=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><e:msub><e:mi>N</e:mi><e:mi>c</e:mi></e:msub></e:math> corrections affect the thermodynamics as well as the phase diagram of chirally imbalanced quark matter. We then compare the results obtained with a sharp three-dimensional cutoff—generically referred to as the traditional regularization scheme—and with an alternative procedure called the medium separation scheme (MSS). In the first case, we observe that the pseudocritical temperature decreases as the chiral chemical potential increases, an effect dubbed inverse chiral catalysis. On the other hand, when considering the MSS regularization, which properly isolates the medium contributions from the vacuum, we find the opposite result. We show that the results obtained with MSS are consistent with well-established lattice quantum chromodynamics data in both the LN and BLN approximations. Finally, we suggest that to cope with the high-density limit, the standard OPT interpolation prescription must be modified with the inclusion of an extra variational parameter.","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"13 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-10-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145311567","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Lorenzo Calibbi, Claudia Hagedorn, Michael A. Schmidt, James Vandeleur
{"title":"Selection rules for charged lepton flavor violating processes from residual flavor groups","authors":"Lorenzo Calibbi, Claudia Hagedorn, Michael A. Schmidt, James Vandeleur","doi":"10.1103/b6gz-c1c9","DOIUrl":"https://doi.org/10.1103/b6gz-c1c9","url":null,"abstract":"We systematically investigate the possible phenomenological impact of residual flavor groups in the charged lepton sector. We consider all possible flavor charge assignments for Abelian residual symmetries up to Z</a:mi>8</a:mn></a:msub></a:math>. The allowed flavor structures of operators in Standard Model effective field theory (up to dimension six) lead to distinctive and observable patterns of charged lepton flavor violating processes. We illustrate the relevance of such selection rules displaying the current bounds on and the future sensitivities to the new physics scale. These results demonstrate, in particular, the importance and discriminating power of searches for lepton flavor violating <d:math xmlns:d=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><d:mi>τ</d:mi></d:math> lepton decays and muonium to antimuonium conversion.","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"11 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-10-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145311280","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Charged current neutrino and antineutrino induced associated particle production from nucleons","authors":"A. Fatima, M. Sajjad Athar, S. K. Singh","doi":"10.1103/6c5c-sl4t","DOIUrl":"https://doi.org/10.1103/6c5c-sl4t","url":null,"abstract":"In this work, we study the charged-current (anti)neutrino induced associated particle (K</a:mi>Λ</a:mi></a:math>) production (<d:math xmlns:d=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><d:mi mathvariant=\"normal\">Δ</d:mi><d:mi>S</d:mi><d:mo>=</d:mo><d:mn>0</d:mn></d:math>) from free nucleons in the energy region of a few GeV, relevant to the (anti)neutrino oscillation experiments with accelerator and atmospheric neutrinos. We employ a model based on effective Lagrangians to evaluate the contributions from the nonresonant and the resonant diagrams. The nonresonant background terms are calculated using a microscopic model derived from the SU(3) chiral Lagrangians. For the resonant contributions, we consider the low-lying spin-<g:math xmlns:g=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><g:mfrac><g:mn>1</g:mn><g:mn>2</g:mn></g:mfrac></g:math> resonances, such as <i:math xmlns:i=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><i:msub><i:mi>S</i:mi><i:mn>11</i:mn></i:msub><i:mo stretchy=\"false\">(</i:mo><i:mn>1650</i:mn><i:mo stretchy=\"false\">)</i:mo></i:math>, <m:math xmlns:m=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><m:msub><m:mi>P</m:mi><m:mn>11</m:mn></m:msub><m:mo stretchy=\"false\">(</m:mo><m:mn>1710</m:mn><m:mo stretchy=\"false\">)</m:mo></m:math>, <q:math xmlns:q=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><q:msub><q:mi>P</q:mi><q:mn>11</q:mn></q:msub><q:mo stretchy=\"false\">(</q:mo><q:mn>1880</q:mn><q:mo stretchy=\"false\">)</q:mo></q:math>, and <u:math xmlns:u=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><u:msub><u:mi>S</u:mi><u:mn>11</u:mn></u:msub><u:mo stretchy=\"false\">(</u:mo><u:mn>1895</u:mn><u:mo stretchy=\"false\">)</u:mo></u:math>, and spin-<y:math xmlns:y=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><y:mfrac><y:mn>3</y:mn><y:mn>2</y:mn></y:mfrac></y:math> resonances, such as P</ab:mi>13</ab:mn></ab:msub>(</ab:mo>1720</ab:mn>)</ab:mo></ab:math> and <eb:math xmlns:eb=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><eb:msub><eb:mi>P</eb:mi><eb:mn>13</eb:mn></eb:msub><eb:mo stretchy=\"false\">(</eb:mo><eb:mn>1900</eb:mn><eb:mo stretchy=\"false\">)</eb:mo></eb:math>, which have finite branching ratios to the <ib:math xmlns:ib=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><ib:mi>K</ib:mi><ib:mi mathvariant=\"normal\">Λ</ib:mi></ib:math> channel. These resonant contributions are modeled using an effective phenomenological Lagrangian approach, with strong couplings determined from the experimental branching ratios and the decay widths to the <lb:math xmlns:lb=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><lb:mi>K</lb:mi><lb:mi mathvariant=\"normal\">Λ</lb:mi></lb:math> channel. To fix the parameters of the vector current interaction, the model is first used to reproduce satisfactorily the MAMI@Mainz experimental data on the real photon induced scattering off the nucleon resulting an eta meson in the final state and with the CLAS@JLab data for the <ob:math xmlns:ob=\"http://","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"45 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-10-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145311420","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Laura Barrio, Kotaro Fujisawa, Ryuichiro Akaho, Hiroki Nagakura, Shoichi Yamada
{"title":"Asymmetric emissions of neutrinos in the cooling of rotating protoneutron stars","authors":"Laura Barrio, Kotaro Fujisawa, Ryuichiro Akaho, Hiroki Nagakura, Shoichi Yamada","doi":"10.1103/jmqs-zpnk","DOIUrl":"https://doi.org/10.1103/jmqs-zpnk","url":null,"abstract":"We evaluate global asymmetry in the luminosities of neutrinos emitted from rapidly rotating protoneutron stars (PNSs). We build axisymmetric models of PNSs in mechanical equilibrium with rotation by adding prescribed angular momentum distributions by hand to nonrotational PNS models, which are extracted from a one-dimensional (spherically symmetric) PNS cooling calculation at different times: t</a:mi>=</a:mo>2</a:mn></a:math>, 6, 10, 20, and 30 s after a supernova explosion. We then conduct two-dimensional (spatially axisymmetric) neutrino transport calculations on top of them with the matter profiles (and the spacetime geometry) fixed. We find for the rapidly rotating models with <c:math xmlns:c=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><c:mi>T</c:mi><c:mo>/</c:mo><c:mo stretchy=\"false\">|</c:mo><c:mi>W</c:mi><c:mo stretchy=\"false\">|</c:mo><c:mo>∼</c:mo><c:mn>5</c:mn><c:mo>×</c:mo><c:msup><c:mn>10</c:mn><c:mrow><c:mo>−</c:mo><c:mn>2</c:mn></c:mrow></c:msup></c:math> that the neutrino luminosity changes by <g:math xmlns:g=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><g:mo>∼</g:mo><g:mn>3</g:mn><g:mo>%</g:mo></g:math> depending on the observer position. We give detailed analyses of the neutrino hemispheres, as well as the neutrino luminosities that are defined observerwise. We also calculate the low-frequency (<i:math xmlns:i=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><i:mo>≲</i:mo><i:mn>1</i:mn><i:mtext> </i:mtext><i:mtext> </i:mtext><i:mi>Hz</i:mi></i:math>) gravitational waves produced by the neutrinos radiated asymmetrically. We find that those gravitational waves, if emitted from the Galactic Center, can be detected by planned detectors such as B-DECIGO, DECIGO, and AILA. Finally, we look for crossings in the energy-integrated angular distributions in momentum space for the electron neutrino sector, a signature of the fast flavor conversion. We find them near the PNS surface in all models.","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"35 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-10-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145311422","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Erratum: Effect of interactions on the topological expression for the chiral separation effect [Phys. Rev. D 107 , 094021 (2023)]","authors":"M. A. Zubkov, Ruslan A. Abramchuk","doi":"10.1103/35gw-mr8b","DOIUrl":"https://doi.org/10.1103/35gw-mr8b","url":null,"abstract":"","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"1 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-10-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145311427","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}