Physical Review D最新文献

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Light propagation in 2PN approximation in the monopole and quadrupole field of a body at rest: The basic transformations 静止物体单极和四极场中2PN近似的光传播:基本变换
IF 5 2区 物理与天体物理
Physical Review D Pub Date : 2025-09-29 DOI: 10.1103/zmsk-wb2k
Sven Zschocke
{"title":"Light propagation in 2PN approximation in the monopole and quadrupole field of a body at rest: The basic transformations","authors":"Sven Zschocke","doi":"10.1103/zmsk-wb2k","DOIUrl":"https://doi.org/10.1103/zmsk-wb2k","url":null,"abstract":"","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"65 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-09-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145188940","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}
引用次数: 0
Cosmographic analysis of sign-switching dark energy 符号转换暗能量的宇宙学分析
IF 5 2区 物理与天体物理
Physical Review D Pub Date : 2025-09-29 DOI: 10.1103/v1cl-pr54
Mariam Bouhmadi-López, Beñat Ibarra-Uriondo
{"title":"Cosmographic analysis of sign-switching dark energy","authors":"Mariam Bouhmadi-López, Beñat Ibarra-Uriondo","doi":"10.1103/v1cl-pr54","DOIUrl":"https://doi.org/10.1103/v1cl-pr54","url":null,"abstract":"","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"101 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-09-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145188943","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}
引用次数: 0
B(s)→S(a0(1450), K0*(1430), f0(1500)) helicity form factors within QCD light-cone sum rules B(s)→s (a0(1450), K0*(1430), f0(1500)))螺旋形因子符合QCD光锥求和规则
IF 5 2区 物理与天体物理
Physical Review D Pub Date : 2025-09-29 DOI: 10.1103/27kn-4xz2
Yi Zhang, Wei Cheng, Jia-Wei Zhang, Tao Zhong, Hai-Bing Fu, Li-Sheng Geng
{"title":"B(s)→S(a0(1450), K0*(1430), f0(1500)) helicity form factors within QCD light-cone sum rules","authors":"Yi Zhang, Wei Cheng, Jia-Wei Zhang, Tao Zhong, Hai-Bing Fu, Li-Sheng Geng","doi":"10.1103/27kn-4xz2","DOIUrl":"https://doi.org/10.1103/27kn-4xz2","url":null,"abstract":"In this paper, we investigate the helicity form factors (HFFs) of the B</a:mi>(</a:mo>s</a:mi>)</a:mo></a:mrow></a:msub></a:math>-meson decay into a scalar meson with a mass larger than 1 GeV, i.e., <e:math xmlns:e=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><e:mi>B</e:mi><e:mo stretchy=\"false\">→</e:mo><e:msub><e:mi>a</e:mi><e:mn>0</e:mn></e:msub><e:mo stretchy=\"false\">(</e:mo><e:mn>1450</e:mn><e:mo stretchy=\"false\">)</e:mo></e:math>, <j:math xmlns:j=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><j:msub><j:mi>B</j:mi><j:mrow><j:mo stretchy=\"false\">(</j:mo><j:mi>s</j:mi><j:mo stretchy=\"false\">)</j:mo></j:mrow></j:msub><j:mo stretchy=\"false\">→</j:mo><j:msubsup><j:mi>K</j:mi><j:mn>0</j:mn><j:mo>*</j:mo></j:msubsup><j:mo stretchy=\"false\">(</j:mo><j:mn>1430</j:mn><j:mo stretchy=\"false\">)</j:mo></j:math>, and <q:math xmlns:q=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><q:msub><q:mi>B</q:mi><q:mi>s</q:mi></q:msub><q:mo stretchy=\"false\">→</q:mo><q:msub><q:mi>f</q:mi><q:mn>0</q:mn></q:msub><q:mo stretchy=\"false\">(</q:mo><q:mn>1500</q:mn><q:mo stretchy=\"false\">)</q:mo></q:math> by using the light-cone sum rules approach. We take the standard currents for correlation functions. To enhance the precision of our calculations, we incorporate the next-to-leading order (NLO) corrections and retain the scalar meson twist-3 light-cone distribution amplitudes. Furthermore, we extend the HFFs to the entire physical <v:math xmlns:v=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><v:msup><v:mi>q</v:mi><v:mn>2</v:mn></v:msup></v:math> region employing a simplified <x:math xmlns:x=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><x:mi>z</x:mi></x:math>-series expansion. At the point of <z:math xmlns:z=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><z:mrow><z:msup><z:mrow><z:mi>q</z:mi></z:mrow><z:mn>2</z:mn></z:msup><z:mo>=</z:mo><z:mn>1</z:mn><z:mtext> </z:mtext><z:mtext> </z:mtext><z:msup><z:mrow><z:mi>GeV</z:mi></z:mrow><z:mn>2</z:mn></z:msup></z:mrow></z:math>, all NLO contributions to the HFFs are negative, with the maximum contribution around 25%. Then, as applications of these HFFs, we analyze the differential decay widths, branching ratios, and lepton polarization asymmetries for the semileptonic <bb:math xmlns:bb=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><bb:msub><bb:mi>B</bb:mi><bb:mrow><bb:mo stretchy=\"false\">(</bb:mo><bb:mi>s</bb:mi><bb:mo stretchy=\"false\">)</bb:mo></bb:mrow></bb:msub><bb:mo stretchy=\"false\">→</bb:mo><bb:mi>S</bb:mi><bb:mo>ℓ</bb:mo><bb:msub><bb:mover accent=\"true\"><bb:mi>ν</bb:mi><bb:mo stretchy=\"false\">¯</bb:mo></bb:mover><bb:mo>ℓ</bb:mo></bb:msub></bb:math>, FCNC <ib:math xmlns:ib=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><ib:msub><ib:mi>B</ib:mi><ib:mrow><ib:mo stretchy=\"false\">(</ib:mo><ib:mi>s</ib:mi><ib:mo stretchy=\"false\">)</ib:mo></ib:mrow></ib:msub><ib:mo stretchy=\"false\">→</ib:mo><ib:mi>S</ib:mi><ib:mo>ℓ</ib:mo><ib:mover accent=\"true\"><ib:mo>ℓ</ib:mo><ib:mo stretc","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"5 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-09-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145188949","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}
引用次数: 0
Theory of time based on wave function collapse 基于波函数坍缩的时间理论
IF 5 2区 物理与天体物理
Physical Review D Pub Date : 2025-09-29 DOI: 10.1103/glfz-yvnl
Sung-Sik Lee
{"title":"Theory of time based on wave function collapse","authors":"Sung-Sik Lee","doi":"10.1103/glfz-yvnl","DOIUrl":"https://doi.org/10.1103/glfz-yvnl","url":null,"abstract":"","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"64 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-09-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145183010","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}
引用次数: 0
SN1987A bounds on neutrino quantum decoherence 中微子量子退相干的SN1987A界
IF 5 2区 物理与天体物理
Physical Review D Pub Date : 2025-09-29 DOI: 10.1103/4j6r-d2wx
Christoph A. Ternes, Giulia Pagliaroli, Francesco L. Villante
{"title":"SN1987A bounds on neutrino quantum decoherence","authors":"Christoph A. Ternes, Giulia Pagliaroli, Francesco L. Villante","doi":"10.1103/4j6r-d2wx","DOIUrl":"https://doi.org/10.1103/4j6r-d2wx","url":null,"abstract":"We obtain stringent bounds on neutrino quantum decoherence from the analysis of SN1987A data. We show that for the decoherence model considered here, which allows for neutrino loss along the trajectory, the bounds are many orders of magnitude stronger than the ones that can be obtained from the analysis of data from reactor neutrino oscillation experiments or neutrino telescopes.","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"23 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-09-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145183147","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}
引用次数: 0
Saturation of chaos bound in a phenomenological rotating black hole effective matter system at low-temperature limit 低温极限下现象学旋转黑洞有效物质系统混沌界的饱和
IF 5 2区 物理与天体物理
Physical Review D Pub Date : 2025-09-29 DOI: 10.1103/d2b7-t7y7
Reza Pourkhodabakhshi
{"title":"Saturation of chaos bound in a phenomenological rotating black hole effective matter system at low-temperature limit","authors":"Reza Pourkhodabakhshi","doi":"10.1103/d2b7-t7y7","DOIUrl":"https://doi.org/10.1103/d2b7-t7y7","url":null,"abstract":"","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"7 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-09-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145189498","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}
引用次数: 0
Revisiting reactor antineutrino 5 MeV bump with C13 neutral-current interaction 用C13中性电流相互作用重访反应堆反中微子5mev碰撞
IF 5 2区 物理与天体物理
Physical Review D Pub Date : 2025-09-29 DOI: 10.1103/s64c-l1p9
Pouya Bakhti, Min-Gwa Park, Meshkat Rajaee, Chang Sub Shin, Seodong Shin
{"title":"Revisiting reactor antineutrino 5 MeV bump with C13 neutral-current interaction","authors":"Pouya Bakhti, Min-Gwa Park, Meshkat Rajaee, Chang Sub Shin, Seodong Shin","doi":"10.1103/s64c-l1p9","DOIUrl":"https://doi.org/10.1103/s64c-l1p9","url":null,"abstract":"For the first time, we comprehensively examine the potential of a neutral-current interaction of reactor neutrino with C</a:mi></a:mrow>13</a:mn></a:mrow></a:mmultiscripts></a:mrow></a:math> emitting a 3.685 MeV photon to identify the origin of the 5 MeV bump in reactor antineutrino spectra observed through the inverse beta decay process. This anomaly may be due to new physics, reactor antineutrino flux inaccuracies, or inverse beta decay systematics. The 3.685 MeV photon released during the deexcitation of <d:math xmlns:d=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><d:mrow><d:mrow><d:mmultiscripts><d:mrow><d:msup><d:mrow><d:mi mathvariant=\"normal\">C</d:mi></d:mrow><d:mrow><d:mo>*</d:mo></d:mrow></d:msup></d:mrow><d:mprescripts/><d:none/><d:mrow><d:mn>13</d:mn></d:mrow></d:mmultiscripts></d:mrow></d:mrow></d:math> to its ground state is observable in liquid scintillator detectors. Remarkably, we confirm the powerfulness of our proposal by completely ruling out a new physics scenario explaining the bump from the existing NEOS data. We also explore the potential of current and forthcoming experiments, including solar neutrino studies at JUNO, pion and muon decay-at-rest experiments at OscSNS, and isotope decay-at-rest studies at Yemilab, to measure the cross section precisely enough to distinguish the expected bump and the theoretical flux models via our channel. Additionally, we propose a novel method to track the time evolution of reactor isotopes by analyzing the <g:math xmlns:g=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><g:mrow><g:mmultiscripts><g:mrow><g:mi mathvariant=\"normal\">C</g:mi></g:mrow><g:mprescripts/><g:none/><g:mrow><g:mn>13</g:mn></g:mrow></g:mmultiscripts></g:mrow></g:math> signal, which yields critical insights into the contributions of <j:math xmlns:j=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><j:mrow><j:mmultiscripts><j:mrow><j:mi mathvariant=\"normal\">U</j:mi></j:mrow><j:mprescripts/><j:none/><j:mrow><j:mn>235</j:mn></j:mrow></j:mmultiscripts></j:mrow></j:math> and <m:math xmlns:m=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><m:mrow><m:mmultiscripts><m:mrow><m:mi>Pu</m:mi></m:mrow><m:mprescripts/><m:none/><m:mrow><m:mn>239</m:mn></m:mrow></m:mmultiscripts></m:mrow></m:math> to the bump, acting as a robust tool.","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"16 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-09-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145189501","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}
引用次数: 0
Lepton flavor violation by three units 轻子味违反了三个单位
IF 5 2区 物理与天体物理
Physical Review D Pub Date : 2025-09-29 DOI: 10.1103/2zkx-d3yk
Julian Heeck, Mikheil Sokhashvili, Anil Thapa
{"title":"Lepton flavor violation by three units","authors":"Julian Heeck, Mikheil Sokhashvili, Anil Thapa","doi":"10.1103/2zkx-d3yk","DOIUrl":"https://doi.org/10.1103/2zkx-d3yk","url":null,"abstract":"The conservation of lepton flavor is a prediction of the Standard Model and is still an excellent approximate symmetry despite our observation of neutrino oscillations. Lepton flavor violation by one or two units has been discussed for decades, with several dedicated experiments exploring the vast model landscape but no discoveries so far. Here, we explore operators and processes that violate at least one lepton flavor by three units and identify testable signatures. In the Standard Model effective field theory, such operators already arise at mass dimension 7 and can be tested through their contributions to Michel parameters in leptonic decays. True neutrinoless charged-lepton flavor violation arises at mass dimension 10 and can realistically only be seen in the tau decay channels τ</a:mi>→</a:mo>e</a:mi>e</a:mi>e</a:mi>μ</a:mi>¯</a:mo></a:mover>μ</a:mi>¯</a:mo></a:mover></a:math> or <h:math xmlns:h=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><h:mi>τ</h:mi><h:mo stretchy=\"false\">→</h:mo><h:mi>μ</h:mi><h:mi>μ</h:mi><h:mi>μ</h:mi><h:mover accent=\"true\"><h:mi>e</h:mi><h:mo stretchy=\"false\">¯</h:mo></h:mover><h:mover accent=\"true\"><h:mi>e</h:mi><h:mo stretchy=\"false\">¯</h:mo></h:mover></h:math>, for example in Belle II. Testable rates for these tau decays require light new particles and subsequently predict an avalanche of remarkably clean but so-far unconstrained collider signatures.","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"38 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-09-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145182953","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}
引用次数: 0
Interpreting luminosity bursts in a Kepler-measured ZZ Ceti using avalanche statistics 用雪崩统计解释开普勒测量的ZZ Ceti的光度爆发
IF 5 2区 物理与天体物理
Physical Review D Pub Date : 2025-09-29 DOI: 10.1103/3kby-v1rp
Jordan Sickle, Gabriel H. Myers, Kameron Gausling, Ethan Mullen, Amartya Shah, Steve Kawaler, Karin A. Dahmen
{"title":"Interpreting luminosity bursts in a Kepler-measured ZZ Ceti using avalanche statistics","authors":"Jordan Sickle, Gabriel H. Myers, Kameron Gausling, Ethan Mullen, Amartya Shah, Steve Kawaler, Karin A. Dahmen","doi":"10.1103/3kby-v1rp","DOIUrl":"https://doi.org/10.1103/3kby-v1rp","url":null,"abstract":"","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"92 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-09-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145183007","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}
引用次数: 0
Double Higgs boson production via vector boson fusion in SMEFT SMEFT中矢量玻色子聚变产生双希格斯玻色子
IF 5 2区 物理与天体物理
Physical Review D Pub Date : 2025-09-29 DOI: 10.1103/bywd-2dy1
Athanasios Dedes, Janusz Rosiek, Michał Ryczkowski
{"title":"Double Higgs boson production via vector boson fusion in SMEFT","authors":"Athanasios Dedes, Janusz Rosiek, Michał Ryczkowski","doi":"10.1103/bywd-2dy1","DOIUrl":"https://doi.org/10.1103/bywd-2dy1","url":null,"abstract":"While gluon fusion dominates Higgs pair production at the LHC, vector boson fusion (VBF) offers a unique window into beyond the Standard Model (BSM) physics through its distinctive kinematic features and direct sensitivity to Higgs-vector boson interactions. We perform a comprehensive analysis of double Higgs production via VBF in the Standard Model effective field theory (SMEFT), systematically investigating how dimension-6 and dimension-8 bosonic operators—particularly those involving field derivatives—can enhance the production rate. We identify the most relevant Wilson coefficients (WCs) affecting the trilinear Higgs coupling (h</a:mi>h</a:mi>h</a:mi></a:math>) and Higgs-vector boson interactions (<c:math xmlns:c=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><c:mi>h</c:mi><c:mi>V</c:mi><c:mi>V</c:mi></c:math>, <e:math xmlns:e=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><e:mi>h</e:mi><e:mi>h</e:mi><e:mi>V</e:mi><e:mi>V</e:mi></e:math>). Using constraints from global fits and interpolating fit results for unconstrained WCs with naive dimensional analysis, we assess their effects on the <g:math xmlns:g=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><g:mi>V</g:mi><g:mi>V</g:mi><g:mo stretchy=\"false\">→</g:mo><g:mi>h</g:mi><g:mi>h</g:mi></g:math> (<j:math xmlns:j=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><j:mrow><j:mrow><j:mi>V</j:mi><j:mo>=</j:mo><j:mi>W</j:mi></j:mrow><j:mo>,</j:mo><j:mrow><j:mi>Z</j:mi></j:mrow></j:mrow></j:math>) scattering amplitudes and cross sections. Our analysis includes a study of EFT convergence and validity in models with scalar extensions of the SM. Numerical simulations for the planned High-Luminosity LHC experiment (HL-LHC) in general reveal only a modest and challenging to detect enhancement of the VBF di-Higgs production rate over the SM prediction. However, we show that in optimistic scenarios, such a process could be observed at the HL-LHC. In certain cases, when the enhancement is dominated by the dimension-6 or dimension-8 operators containing field derivatives (and thus leading to stronger energy-dependent effects), this channel becomes competitive with di-Higgs production via gluon fusion. This work highlights the role of VBF di-Higgs production as a complementary channel for probing anomalous Higgs couplings and their impact on BSM physics.","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"97 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-09-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145183146","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}
引用次数: 0
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