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Exploring the Parameter Space of Inflation Model on the Brane and its Compatibility with the Swampland Conjectures 布莱恩通胀模型参数空间探索及其与沼泽地猜想的兼容性
arXiv - PHYS - High Energy Physics - Theory Pub Date : 2024-09-10 DOI: arxiv-2409.06488
Saeed Noori Gashti, Mohammad Reza Alipour, Mohammad Ali S. Afshar
{"title":"Exploring the Parameter Space of Inflation Model on the Brane and its Compatibility with the Swampland Conjectures","authors":"Saeed Noori Gashti, Mohammad Reza Alipour, Mohammad Ali S. Afshar","doi":"arxiv-2409.06488","DOIUrl":"https://doi.org/arxiv-2409.06488","url":null,"abstract":"In recent years, inflationary models have been studied from different\u0000perspectives using different conditions. Now, in this paper, we want to\u0000investigate the inverse monomial Inflation $(IMI)$ on the brane. We limit our\u0000results to the potentials of the form $frac{M^{4+sigma}}{phi^{sigma}}$. We\u0000calculate some cosmological parameters and then we investigate the satisfaction\u0000of the model with some conjectures of the swampland program. We will check the\u0000model's compatibility with the refined dS swampland conjecture(RDSSC), further\u0000refining the de Sitter swampland conjecture (FRSDC), scalar weak gravity\u0000(SWGC), and strong scalar weak gravity conjecture (SSWGC). Despite the\u0000incompatibility with (DSSC), We find a specific region of compatibility with\u0000other ones which means it satisfied the (FRDSSC) for example with (a=0.982873,\u0000b=0.017127, q=2.2). Also, the model is compatible with the (SWGC) with the\u0000($phileq sigma+2$) condition and consistent with the (SSWGC) with the ($phi\u0000leq sqrt{(sigma+2)(sigma+1)}$) condition. Since inverse monomial\u0000Inflation(IMI) on the brane could satisfy some swampland conjecture\u0000simultaneously, it has the potential to be a \"real\" inflation model of the\u0000universe.","PeriodicalId":501339,"journal":{"name":"arXiv - PHYS - High Energy Physics - Theory","volume":"384 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142176037","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Fermions in the fuzzy sphere Kaluza-Klein model 模糊球卡卢扎-克莱因模型中的费米子
arXiv - PHYS - High Energy Physics - Theory Pub Date : 2024-09-10 DOI: arxiv-2409.06668
Chengcheng Liu, Shahn Majid
{"title":"Fermions in the fuzzy sphere Kaluza-Klein model","authors":"Chengcheng Liu, Shahn Majid","doi":"arxiv-2409.06668","DOIUrl":"https://doi.org/arxiv-2409.06668","url":null,"abstract":"We consider spinors on the total space of a Kaluza-Klein model with fuzzy\u0000sphere fibre and geometrically realised Dirac operator on the product. We show\u0000that a single massless spinor on the product appears on spacetime as multiplets\u0000of spinors with a particular signature of differing masses and $SU(2)$\u0000Yang-Mills charges. For example, for the reduced fuzzy sphere isomorphic to\u0000$M_2(mathbb{C})$, a massless spinor appears as two $SU(2)$ doublets and an\u0000$SU(2)$ quadruplet in mass ratios $1:5/3:7/3$. Although such signatures do not\u0000appear to exactly math the Standard Model, the paper provides proof of concept\u0000of the approach, which can be applied to other noncommutative fibre algebras.","PeriodicalId":501339,"journal":{"name":"arXiv - PHYS - High Energy Physics - Theory","volume":"86 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142176028","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Asymptotic Hodge Theory in String Compactifications and Integrable Systems 弦压缩和可积分系统中的渐近霍奇理论
arXiv - PHYS - High Energy Physics - Theory Pub Date : 2024-09-10 DOI: arxiv-2409.06794
Jeroen Monnee
{"title":"Asymptotic Hodge Theory in String Compactifications and Integrable Systems","authors":"Jeroen Monnee","doi":"arxiv-2409.06794","DOIUrl":"https://doi.org/arxiv-2409.06794","url":null,"abstract":"In this thesis we study the framework of asymptotic Hodge theory and its\u0000applications in both the string landscape and the landscape of 2d integrable\u0000field theories. We show how this mathematical framework allows for a general\u0000characterization of the asymptotic behaviour of physical couplings in\u0000low-energy effective theories coming from string theory, and apply this\u0000knowledge to investigate the finiteness and geometric structure of the string\u0000landscape landscape. At the same time, we find that the defining equations of\u0000variations of Hodge structure also arise in the context of certain integrable\u0000field theories, which opens the way to finding new classes of very general\u0000solutions to said models. Part I reviews the relevant aspects of type IIB / F-theory flux\u0000compactifications and the resulting landscape of 4d low-energy effective\u0000$mathcal{N}=1$ supergravity theories. Part II provides an in-depth discussion on asymptotic Hodge theory, including\u0000detailed explanations on the nilpotent orbit theorem of Schmid, and the\u0000multi-variable Sl(2)-orbit theorem of Cattani, Kaplan, and Schmid. This part of\u0000the thesis also contains new results regarding the multi-variable bulk\u0000reconstruction procedure, which have not appeared in the author's previous\u0000publications. Part III concerns the application of the aforementioned results to study the\u0000finiteness of the F-theory flux landscape. Additionally, motivated by recent\u0000advances in the field of o-minimal geometry and the theory of unlikely\u0000intersections, we propose three conjectures which aim to address finer features\u0000of the flux landscape. Part IV investigates two corners of the landscape of 2d integrable non-linear\u0000sigma-models, namely the $lambda$-deformed gauged WZW model and the critical\u0000bi-Yang-Baxter model. Notably, it is shown that asymptotic Hodge theory can be\u0000used to find broad classes of solutions these models.","PeriodicalId":501339,"journal":{"name":"arXiv - PHYS - High Energy Physics - Theory","volume":"6 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142176019","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Anomaly freedom in effective Loop Quantum Cosmology: pedagogical summary and generalized holonomy corrections 有效环量子宇宙学中的反常自由:教学总结和广义整体性修正
arXiv - PHYS - High Energy Physics - Theory Pub Date : 2024-09-10 DOI: arxiv-2409.06441
Maxime De Sousa, Aurélien Barrau, Killian Martineau
{"title":"Anomaly freedom in effective Loop Quantum Cosmology: pedagogical summary and generalized holonomy corrections","authors":"Maxime De Sousa, Aurélien Barrau, Killian Martineau","doi":"arxiv-2409.06441","DOIUrl":"https://doi.org/arxiv-2409.06441","url":null,"abstract":"The issue of consistency is crucial in quantum gravity. It has recently been\u0000intensively addressed for effective symmetry-reduced models. In this article,\u0000we exhaustively study the anomaly freedom of effective loop quantum cosmology\u0000with generalized holonomy corrections, considering loop correction of the\u0000constraints at the perturbative order. We pedagogically explain why, although\u0000the holonomy correction -- including the details of the chosen scheme --\u0000applied on the background part of the constraints is crucial, it becomes\u0000irrelevant when implemented on perturbative expansions, in the sense that all\u0000consequences are \"absorbed\" in the counter-terms used for the regularization.\u0000The possibility of closing the algebra of constraints without counter-terms is\u0000also studied. It is argued that, although enforcing a first-class algebra is a\u0000strong requirement, this can be achieved in several different ways, often\u0000overlooked, which generates ambiguities on the restriction of the form of the\u0000generalized holonomy correction. Those ambiguities are examined in details,\u0000leading to the conclusion that the consistency of the effective theory for\u0000cosmological perturbations, especially when considering scalar modes, cannot be\u0000achieved without counter-terms. We also take the opportunity of this work to\u0000clarify, as much as possible, all the required steps so that future works have\u0000a clear material at disposal. In particular, a highly detailed calculation of\u0000all the brackets is provided, emphasizing the (usually implicit) assumptions,\u0000hypotheses and manipulations required to ensure the closure of the algebra.\u0000Prospects for future works are underlined.","PeriodicalId":501339,"journal":{"name":"arXiv - PHYS - High Energy Physics - Theory","volume":"122 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142176064","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
From spacetime thermodynamics to Weyl transverse gravity 从时空热力学到韦尔横向引力
arXiv - PHYS - High Energy Physics - Theory Pub Date : 2024-09-10 DOI: arxiv-2409.06645
Ana Alonso-Serrano, Luis J. Garay, Marek Liška
{"title":"From spacetime thermodynamics to Weyl transverse gravity","authors":"Ana Alonso-Serrano, Luis J. Garay, Marek Liška","doi":"arxiv-2409.06645","DOIUrl":"https://doi.org/arxiv-2409.06645","url":null,"abstract":"There exist two consistent theories of self-interacting gravitons: general\u0000relativity and Weyl transverse gravity. The latter has the same classical\u0000solutions as general relativity, but different local symmetries. We argue that\u0000Weyl transverse gravity also naturally arises from thermodynamic arguments. In\u0000particular, we show that thermodynamic equilibrium of local causal diamonds\u0000together with the strong equivalence principle encodes the gravitational\u0000dynamics of Weyl transverse gravity rather than general relativity. We obtain\u0000this result in a self-consistent way, verifying the validity of our initial\u0000assumptions, i.e. the proportionality between entropy and area and the\u0000different versions of the equivalence principle in Weyl transverse gravity.\u0000Furthermore, we extend the thermodynamic derivation of the equations of motion\u0000from Weyl transverse gravity to a class of modified theories of gravity with\u0000the same local symmetries. For this purpose, we employ the general expression\u0000for Wald entropy in such theories.","PeriodicalId":501339,"journal":{"name":"arXiv - PHYS - High Energy Physics - Theory","volume":"1 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142176035","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Induced Gravitational Waves probing Primordial Black Hole Dark Matter with Memory Burden 用记忆负担探测原始黑洞暗物质的诱导引力波
arXiv - PHYS - High Energy Physics - Theory Pub Date : 2024-09-10 DOI: arxiv-2409.06365
Kazunori Kohri, Takahiro Terada, Tsutomu T. Yanagida
{"title":"Induced Gravitational Waves probing Primordial Black Hole Dark Matter with Memory Burden","authors":"Kazunori Kohri, Takahiro Terada, Tsutomu T. Yanagida","doi":"arxiv-2409.06365","DOIUrl":"https://doi.org/arxiv-2409.06365","url":null,"abstract":"Quantum evaporation of a black hole is conventionally studied semiclassically\u0000by assuming self-similarity of the black hole throughout the evaporation\u0000process. However, its validity was recently questioned, and the lifetime of a\u0000black hole is conjectured to be much extended by the memory burden effect. It\u0000gives rise to the possibility that the primordial black holes (PBHs) lighter\u0000than $10^{10}$ grams are the dark matter in the Universe. To probe such PBH\u0000dark matter, we study gravitational waves (GWs) induced by primordial curvature\u0000perturbations that produced the PBHs. We find\u0000$Omega_text{GW}(f_text{peak})h^2 = 7 times 10^{-9}$ with the peak frequency\u0000$f_text{peak} = 1times 10^{3} ,\u0000(M_text{PBH}/(10^{10},mathrm{g}))^{-1/2}, mathrm{Hz}$, and the induced GWs\u0000associated with the PBH dark matter whose initial mass is greater than about\u0000$10^7$ grams can be tested by future observations such as Cosmic Explorer.\u0000Furthermore, the scenario can be in principle confirmed by detecting another GW\u0000signal from the mergers of PBHs, which leads to high-frequency GWs with\u0000$f_text{peak} = 2 times 10^{27}, (M_text{PBH, ini}/(10^{10},\u0000mathrm{g}))^{-1} , mathrm{Hz} $. On the other hand, the induced GW signals\u0000stronger than expected would contradict the dark matter abundance and exclude\u0000the memory burden effect.","PeriodicalId":501339,"journal":{"name":"arXiv - PHYS - High Energy Physics - Theory","volume":"31 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142176071","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Reconstructing inflation and reheating in the framework of a generalized $mathcal{F}(H)$ Friedmann equation 在广义$mathcal{F}(H)$ 弗里德曼方程框架内重建膨胀和再热
arXiv - PHYS - High Energy Physics - Theory Pub Date : 2024-09-10 DOI: arxiv-2409.06844
Ramon Herrera, Carlos Rios
{"title":"Reconstructing inflation and reheating in the framework of a generalized $mathcal{F}(H)$ Friedmann equation","authors":"Ramon Herrera, Carlos Rios","doi":"arxiv-2409.06844","DOIUrl":"https://doi.org/arxiv-2409.06844","url":null,"abstract":"The reconstruction of an inflationary universe considering the\u0000parametrization of the scalar spectral index as a function of the number of\u0000$e-$folds in the framework of a modified Friedmann equation is analyzed. In\u0000this context, we examine the possibility of reconstructing the Hubble parameter\u0000together with the effective potential considering a modified Friedmann equation\u0000specified by $mathcal{F}(H)propto rho$, where $mathcal{F}(H)$ corresponds\u0000to an arbitrary function of the Hubble parameter $H$ and $rho$ denotes the\u0000energy density associated with the matter in the universe. To reconstruct the\u0000background variables during the inflationary scenario, we develop a new\u0000methodology by expressing the spectral index in terms of the Hubble parameter\u0000and its derivatives. Thus, we obtain a general formalism for the reconstruction\u0000of the inflation, using the slow roll approximation together with the\u0000parametrization of the scalar spectral index as a function of the number of\u0000$e-$folds $N$. As specific examples, we consider the simplest attractor\u0000$n_s-1=-2/N$ together with different functions $mathcal{F}(H)$, associated to\u0000the modified Friedmann equation, to rebuild the Hubble parameter and the\u0000effective potential in terms of the scalar field $phi$. Additionally, we\u0000examine the reheating epoch by considering a constant equation of state\u0000parameter, in which we determine the temperature and the number of e-folds\u0000during this epoch, using the background variables found during the\u0000reconstruction of the different $mathcal{F}(H)-$models studied. Besides, we\u0000constrain the different parameters associated with the reconstructed\u0000inflationary $mathcal{F}(H)-$models during the epochs of inflation and\u0000reheating, using current astronomical data from Planck and BICEP/Keck results.","PeriodicalId":501339,"journal":{"name":"arXiv - PHYS - High Energy Physics - Theory","volume":"3 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142176025","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Quantizing the folded string in AdS$_2$ 量化 AdS$_2$ 中的折叠弦
arXiv - PHYS - High Energy Physics - Theory Pub Date : 2024-09-10 DOI: arxiv-2409.06663
David Vegh
{"title":"Quantizing the folded string in AdS$_2$","authors":"David Vegh","doi":"arxiv-2409.06663","DOIUrl":"https://doi.org/arxiv-2409.06663","url":null,"abstract":"In two-dimensional flat space, the oscillatory motion of a closed folded\u0000string--or alternatively, two massless particles connected by a string--can be\u0000quantized using the 't Hooft equation. This paper presents an alternative\u0000method for quantizing the folded string in anti-de Sitter space. By using\u0000variables inspired by integrability, setting $g equiv {(R_text{AdS})^2 over\u00002pi alpha'}$ to a specific p-dependent $mathcal{O}(1)$ value, and applying a\u0000particular boundary condition to the antisymmetrized wavefunction, we obtain a\u0000spectrum that precisely matches that of fermion bilinear operators in the\u0000disorder-averaged Sachdev-Ye-Kitaev model with p-fermion interactions.","PeriodicalId":501339,"journal":{"name":"arXiv - PHYS - High Energy Physics - Theory","volume":"1 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142176030","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Testing EGB gravity coupled to bumblebee field and black hole parameter estimation with EHT observations 利用 EHT 观测测试与大黄蜂场和黑洞参数估计耦合的 EGB 引力
arXiv - PHYS - High Energy Physics - Theory Pub Date : 2024-09-10 DOI: arxiv-2409.06218
Misba Afrin, Sushant G. Ghosh, Anzhong Wang
{"title":"Testing EGB gravity coupled to bumblebee field and black hole parameter estimation with EHT observations","authors":"Misba Afrin, Sushant G. Ghosh, Anzhong Wang","doi":"arxiv-2409.06218","DOIUrl":"https://doi.org/arxiv-2409.06218","url":null,"abstract":"A general covariant Einstein-Gauss-Bonnet Gravity in Four-Dimensional (4D\u0000EGB) spacetime is shown to bypass Lovelock's theorem and is free from\u0000Ostrogradsky instability. Meanwhile, the bumblebee theory is a vector-tensor\u0000theory. It extends the Einstein--Maxwell theory that allows for the spontaneous\u0000symmetry breaking that leads to the field acquiring a vacuum expectation value,\u0000introducing Lorentz violation into the system. We investigate rotating black\u0000holes in the 4D EGB-bumblebee gravity model where Lorentz symmetry is\u0000spontaneously broken -- Kerr EGB bumblebee (KEGBB) black holes. The latest\u0000observations from the Event Horizon Telescope (EHT) of the supermassive black\u0000holes (SMBHs) M87* and Sgr A* have sparked intensified interest in the study of\u0000black hole shadows, which present a novel avenue for investigating SMBHs within\u0000the strong-field regime. Motivated by this, we model SMBHs M87* and Sgr A* as\u0000KEGBB black holes, and using the EHT observation result, for given $l$, to find\u0000earlier upper limits on the $alpha$ and $a$ are altered. The KEGBB and Kerr\u0000black holes are indiscernible in some parameter space, and one cannot rule out\u0000the possibility that the former may serve as strong candidates for\u0000astrophysical black holes. Employing our newly developed parameter estimation\u0000technique, we use two EHT observables -- namely, the angular diameter of the\u0000shadow, $d_{sh}$, and the axial ratio, $mathcal{D}_A$ -- to estimate\u0000parameters of M87* and Sgr A* taking into account observational errors\u0000associated with the EHT results.","PeriodicalId":501339,"journal":{"name":"arXiv - PHYS - High Energy Physics - Theory","volume":"3 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142176067","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Holography for Boundary Lifshitz Field Theory 全息边界利夫希兹场论
arXiv - PHYS - High Energy Physics - Theory Pub Date : 2024-09-10 DOI: arxiv-2409.06667
Chong-Sun Chu, Ignacio Garrido Gonzalez, Himanshu Parihar
{"title":"Holography for Boundary Lifshitz Field Theory","authors":"Chong-Sun Chu, Ignacio Garrido Gonzalez, Himanshu Parihar","doi":"arxiv-2409.06667","DOIUrl":"https://doi.org/arxiv-2409.06667","url":null,"abstract":"We propose a holographic duality for the boundary Lifshitz field theory\u0000(BLFT). Similar to holographic BCFT, holographic BLFT can be consistently\u0000defined by imposing either a Neumann boundary condition (NBC) or a conformal\u0000boundary condition (CBC) on the end of the world (EOW) brane. We propose\u0000$g$-functions and derive $g$-theorem for these two types of holographic BLFT.\u0000On the field theory side, we consider BLFT whose path integral is prescribed to\u0000include also paths bouncing off the boundary. The entanglement entropy for an\u0000interval for the Lifshitz invariant ground state is computed in the saddle\u0000point approximation, and is found to agree precisely with the holographic\u0000result in both limits when the interval is very close or very far away from the\u0000boundary.","PeriodicalId":501339,"journal":{"name":"arXiv - PHYS - High Energy Physics - Theory","volume":"37 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142176029","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","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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