We study an inhomogeneous U(1) Chern-Simons Higgs model with a magnetic impurity in the BPS limit. The potential is sextic with both broken and unbroken phases, but its minimum varies spatially depending on the strength of the impurity. While the system lacks translation symmetry, it admits a supersymmetric extension. Depending on the sign of the impurity term, it has either a BPS sector or an anti-BPS sector (but not both), which satisfies the Bogomolny equations. The vacuum configuration of the broken phase is not simply determined by the the minimum of the potential since it is no longer constant, but it becomes a nontrivial function satisfying the Bogomolny equations. Thus, the energy and angular momentum densities of the vacuum locally have nonzero distributions, although the total energy and angular momentum remain zero. As in the homogeneous case, the theory supports various BPS soliton solutions, including topological and nontopological vortices and Q-balls. The vorticities as well as the U(1) charges are exclusively positive or negative. For a Gaussian type impurity as a specific example, we obtain rotationally symmetric numerical solutions and analyze their detailed properties.
{"title":"Inhomogeneous Abelian Chern-Simons Higgs Model with New Inhomogeneous BPS Vacuum and Solitons","authors":"Yoonbai Kim, O-Kab Kwon, Hanwool Song, Chanju Kim","doi":"arxiv-2409.11978","DOIUrl":"https://doi.org/arxiv-2409.11978","url":null,"abstract":"We study an inhomogeneous U(1) Chern-Simons Higgs model with a magnetic\u0000impurity in the BPS limit. The potential is sextic with both broken and\u0000unbroken phases, but its minimum varies spatially depending on the strength of\u0000the impurity. While the system lacks translation symmetry, it admits a\u0000supersymmetric extension. Depending on the sign of the impurity term, it has\u0000either a BPS sector or an anti-BPS sector (but not both), which satisfies the\u0000Bogomolny equations. The vacuum configuration of the broken phase is not simply\u0000determined by the the minimum of the potential since it is no longer constant,\u0000but it becomes a nontrivial function satisfying the Bogomolny equations. Thus,\u0000the energy and angular momentum densities of the vacuum locally have nonzero\u0000distributions, although the total energy and angular momentum remain zero. As\u0000in the homogeneous case, the theory supports various BPS soliton solutions,\u0000including topological and nontopological vortices and Q-balls. The vorticities\u0000as well as the U(1) charges are exclusively positive or negative. For a\u0000Gaussian type impurity as a specific example, we obtain rotationally symmetric\u0000numerical solutions and analyze their detailed properties.","PeriodicalId":501339,"journal":{"name":"arXiv - PHYS - High Energy Physics - Theory","volume":"65 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142251473","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}
A dark sector with a very large number of massive degrees of freedom is generically constrained by radiative corrections to Newton's constant. However, there are caveats to this statement, especially if the degrees of freedom are light or mass-less. Here, we examine in detail and update a number of constraints on the possible number of dark degrees of freedom, including from black hole evaporation, from perturbations to systems including an evaporating black hole, from direct gravitational production at colliders, from high-energy cosmic rays, and from supernovae energy losses.
{"title":"Constraints on the maximal number of dark degrees of freedom from black hole evaporation, cosmic rays, colliders, and supernovae","authors":"Christopher Ewasiuk, Stefano Profumo","doi":"arxiv-2409.11359","DOIUrl":"https://doi.org/arxiv-2409.11359","url":null,"abstract":"A dark sector with a very large number of massive degrees of freedom is\u0000generically constrained by radiative corrections to Newton's constant. However,\u0000there are caveats to this statement, especially if the degrees of freedom are\u0000light or mass-less. Here, we examine in detail and update a number of\u0000constraints on the possible number of dark degrees of freedom, including from\u0000black hole evaporation, from perturbations to systems including an evaporating\u0000black hole, from direct gravitational production at colliders, from high-energy\u0000cosmic rays, and from supernovae energy losses.","PeriodicalId":501339,"journal":{"name":"arXiv - PHYS - High Energy Physics - Theory","volume":"542 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142251519","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}
We consider a higher derivative scalar field theory in the presence of a boundary and a classically marginal interaction. We first investigate the free limit where the scalar obeys the square of the Klein-Gordon equation. In precisely $d=6$ dimensions, modules generated by $d-2$ and $d-4$ dimensional primaries merge to form a staggered module. We compute the conformal block associated with this module and show that it is a generalized eigenvector of the Casimir operator. Next we include the effect of a classically marginal interaction that involves four scalar fields and two derivatives. The theory has an infrared fixed point in $d=6-{epsilon}$ dimensions. We compute boundary operator anomalous dimensions and boundary OPE coefficients at leading order in the ${epsilon}$ expansion for the allowed conformal boundary conditions.
{"title":"An Interacting, Higher Derivative, Boundary Conformal Field Theory","authors":"Christopher P. Herzog, Yanjun Zhou","doi":"arxiv-2409.11072","DOIUrl":"https://doi.org/arxiv-2409.11072","url":null,"abstract":"We consider a higher derivative scalar field theory in the presence of a\u0000boundary and a classically marginal interaction. We first investigate the free\u0000limit where the scalar obeys the square of the Klein-Gordon equation. In\u0000precisely $d=6$ dimensions, modules generated by $d-2$ and $d-4$ dimensional\u0000primaries merge to form a staggered module. We compute the conformal block\u0000associated with this module and show that it is a generalized eigenvector of\u0000the Casimir operator. Next we include the effect of a classically marginal\u0000interaction that involves four scalar fields and two derivatives. The theory\u0000has an infrared fixed point in $d=6-{epsilon}$ dimensions. We compute boundary\u0000operator anomalous dimensions and boundary OPE coefficients at leading order in\u0000the ${epsilon}$ expansion for the allowed conformal boundary conditions.","PeriodicalId":501339,"journal":{"name":"arXiv - PHYS - High Energy Physics - Theory","volume":"187 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142251633","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}
Daniel Baranowski, Maximilian Delto, Kirill Melnikov, Andrey Pikelner, Chen-Yu Wang
We present the high-precision result for the zero-jettiness soft function at next-to-next-to-next-to-leading order (N3LO) in perturbative QCD. At this perturbative order, the soft function is the last missing ingredient required for the computation of a hadronic colour singlet production or a colour singlet decay into two jets using the zero-jettiness variable as the slicing parameter. Furthermore, the knowledge of the N3LO soft function enables the re-summed description of the thrust distribution in the process $e^+ e^- to textrm{hadrons}$ through next-to-next-to-next-to-leading logarithmic order, which is important for the extraction of the strong coupling constant using this shape variable. On the methodological side, the complexity of the zero-jettiness variable forced us to develop a new semi-analytic method for phase-space integration in the presence of constraints parameterized through Heaviside functions which, hopefully, will be useful for further development of the $N$-jettiness slicing scheme.
{"title":"Zero-jettiness soft function to third order in perturbative QCD","authors":"Daniel Baranowski, Maximilian Delto, Kirill Melnikov, Andrey Pikelner, Chen-Yu Wang","doi":"arxiv-2409.11042","DOIUrl":"https://doi.org/arxiv-2409.11042","url":null,"abstract":"We present the high-precision result for the zero-jettiness soft function at\u0000next-to-next-to-next-to-leading order (N3LO) in perturbative QCD. At this\u0000perturbative order, the soft function is the last missing ingredient required\u0000for the computation of a hadronic colour singlet production or a colour singlet\u0000decay into two jets using the zero-jettiness variable as the slicing parameter.\u0000Furthermore, the knowledge of the N3LO soft function enables the re-summed\u0000description of the thrust distribution in the process $e^+ e^- to\u0000textrm{hadrons}$ through next-to-next-to-next-to-leading logarithmic order,\u0000which is important for the extraction of the strong coupling constant using\u0000this shape variable. On the methodological side, the complexity of the\u0000zero-jettiness variable forced us to develop a new semi-analytic method for\u0000phase-space integration in the presence of constraints parameterized through\u0000Heaviside functions which, hopefully, will be useful for further development of\u0000the $N$-jettiness slicing scheme.","PeriodicalId":501339,"journal":{"name":"arXiv - PHYS - High Energy Physics - Theory","volume":"192 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142251522","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}
We propose a triality relating the Double-Scaled SYK model, $SL(2,mathbb{C})$ Chern-Simons theory on a disk with an irregular singularity at the center and the outcome of ``real Schur quantization'' applied to $SU(2)$ Seiberg-Witten theory with Neumann boundary conditions. We give supporting evidence for our conjecture by establishing a precise match between a general class of correlators in all three systems.
{"title":"SYK-Schur duality: Double scaled SYK correlators from $N=2$ supersymmetric gauge theory","authors":"Davide Gaiotto, Herman Verlinde","doi":"arxiv-2409.11551","DOIUrl":"https://doi.org/arxiv-2409.11551","url":null,"abstract":"We propose a triality relating the Double-Scaled SYK model,\u0000$SL(2,mathbb{C})$ Chern-Simons theory on a disk with an irregular singularity\u0000at the center and the outcome of ``real Schur quantization'' applied to $SU(2)$\u0000Seiberg-Witten theory with Neumann boundary conditions. We give supporting\u0000evidence for our conjecture by establishing a precise match between a general\u0000class of correlators in all three systems.","PeriodicalId":501339,"journal":{"name":"arXiv - PHYS - High Energy Physics - Theory","volume":"15 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142251477","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}
We study particle production in Vaidya spacetime. Using the WKB approximation, the distribution of Hawking radiation is calculated without the near-horizon approximation, which leads to finite corrections to the purely thermal spectrum. We extend our analysis to extremal and non-extremal Reissner-Nordstr"om and Kerr black holes. Our results can be understood in terms of a thermodynamic toy model, where one regards Hawking radiation as Unruh radiation perceived by observers outside of the black hole. Moreover, we extend the model to incorporate the backreaction of Hawking quanta on spacetime geometry. Our study suggests that the backreaction may prevent the formation of the event horizon and spacetime singularity.
{"title":"Hawking radiation far away from the event horizon","authors":"Dawid Maskalaniec, Bartłomiej Sikorski","doi":"arxiv-2409.11021","DOIUrl":"https://doi.org/arxiv-2409.11021","url":null,"abstract":"We study particle production in Vaidya spacetime. Using the WKB\u0000approximation, the distribution of Hawking radiation is calculated without the\u0000near-horizon approximation, which leads to finite corrections to the purely\u0000thermal spectrum. We extend our analysis to extremal and non-extremal\u0000Reissner-Nordstr\"om and Kerr black holes. Our results can be understood in\u0000terms of a thermodynamic toy model, where one regards Hawking radiation as\u0000Unruh radiation perceived by observers outside of the black hole. Moreover, we\u0000extend the model to incorporate the backreaction of Hawking quanta on spacetime\u0000geometry. Our study suggests that the backreaction may prevent the formation of\u0000the event horizon and spacetime singularity.","PeriodicalId":501339,"journal":{"name":"arXiv - PHYS - High Energy Physics - Theory","volume":"27 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142251523","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}
Farid Thaalba, Nicola Franchini, Miguel Bezares, Thomas P. Sotiriou
We study the dynamics of spherically symmetric black holes in scalar Gauss-Bonnet gravity with an additional coupling between the scalar field and the Ricci scalar using non-linear simulations that employ excision. In this class of theories, black holes possess hair if they lie in a specific mass range, in which case they exhibit a finite-area singularity, unlike general relativity. Our results show that the Ricci coupling can mitigate the loss of hyperbolicity in spherical evolution with black hole initial data. Using excision can enlarge the parameter space for which the system remains well-posed, as one can excise the elliptic region that forms inside the horizon. Furthermore, we explore a possible relation between the loss of hyperbolicity and the formation of the finite-area singularity inside the horizon. We find that the location of the singularity extracted from the static analysis matches the location of the sonic line well. Finally, when possible, we extract the monopolar quasi-normal modes and the time scale of the linear tachyonic instability associated with scalarization. We also check our results by utilizing a continued fraction analysis and supposing linear perturbations of the static solutions.
{"title":"The dynamics of spherically symmetric black holes in scalar-Gauss-Bonnet gravity with a Ricci coupling","authors":"Farid Thaalba, Nicola Franchini, Miguel Bezares, Thomas P. Sotiriou","doi":"arxiv-2409.11398","DOIUrl":"https://doi.org/arxiv-2409.11398","url":null,"abstract":"We study the dynamics of spherically symmetric black holes in scalar\u0000Gauss-Bonnet gravity with an additional coupling between the scalar field and\u0000the Ricci scalar using non-linear simulations that employ excision. In this\u0000class of theories, black holes possess hair if they lie in a specific mass\u0000range, in which case they exhibit a finite-area singularity, unlike general\u0000relativity. Our results show that the Ricci coupling can mitigate the loss of\u0000hyperbolicity in spherical evolution with black hole initial data. Using\u0000excision can enlarge the parameter space for which the system remains\u0000well-posed, as one can excise the elliptic region that forms inside the\u0000horizon. Furthermore, we explore a possible relation between the loss of\u0000hyperbolicity and the formation of the finite-area singularity inside the\u0000horizon. We find that the location of the singularity extracted from the static\u0000analysis matches the location of the sonic line well. Finally, when possible,\u0000we extract the monopolar quasi-normal modes and the time scale of the linear\u0000tachyonic instability associated with scalarization. We also check our results\u0000by utilizing a continued fraction analysis and supposing linear perturbations\u0000of the static solutions.","PeriodicalId":501339,"journal":{"name":"arXiv - PHYS - High Energy Physics - Theory","volume":"48 3 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142251518","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}
We build up the notion of metallic holography for $mathcal{N}=2$ SCFTs in four dimensions, in the presence of a finite $U(1)$ chemical potential. We compute two point correlation functions and study their properties in the regime of low frequency and low momentum. The color sector reveals gapless excitations, one of which propagates with a finite phase velocity while the other mode attenuates through scattering. The flavour sector, on the other hand, reveals spectrum that contains quasiparticle excitations which propagate with a definite phase velocity together with modes that propagate with a finite group velocity which quantum attenuates quite similar in spirit as that of Landau's zero sound modes. We also compute associated AC conductivities, which exhibit different characteristics for different (color and flavour) sectors of $mathcal{N}=2$ SCFTs.
{"title":"Metallic holography for $mathcal{N}=2$ SCFTs in 4d","authors":"Dibakar Roychowdhury","doi":"arxiv-2409.11118","DOIUrl":"https://doi.org/arxiv-2409.11118","url":null,"abstract":"We build up the notion of metallic holography for $mathcal{N}=2$ SCFTs in\u0000four dimensions, in the presence of a finite $U(1)$ chemical potential. We\u0000compute two point correlation functions and study their properties in the\u0000regime of low frequency and low momentum. The color sector reveals gapless\u0000excitations, one of which propagates with a finite phase velocity while the\u0000other mode attenuates through scattering. The flavour sector, on the other\u0000hand, reveals spectrum that contains quasiparticle excitations which propagate\u0000with a definite phase velocity together with modes that propagate with a finite\u0000group velocity which quantum attenuates quite similar in spirit as that of\u0000Landau's zero sound modes. We also compute associated AC conductivities, which\u0000exhibit different characteristics for different (color and flavour) sectors of\u0000$mathcal{N}=2$ SCFTs.","PeriodicalId":501339,"journal":{"name":"arXiv - PHYS - High Energy Physics - Theory","volume":"16 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142251514","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}
We investigate the thermodynamics of a Schwarzschild black hole, surrounded by the quintessence energy-matter in the linear and quadratic generalized uncertainty principle framework. Considering the variance in the position to be of the order of the event horizon radius and equating the variance in the momentum to the Hawking temperature of the black hole, we substitute these variances in the deformed algebra. From there we obtained the generalized uncertainty principle-modified black hole temperature and eventually the specific heat of the black hole. Then we calculate the critical as well as the remnant mass and obtain the entropy relation. We observe that the entropy relation includes the usual leading order ``textit{area divided by four}" term, sub-leading logarithmic term, and higher order inverse of the area corrections. Finally, calculating the energy output as a function of time, we obtain the evaporation time of the black hole. The results show the dependence of the quintessence parameter on the thermodynamic quantities in the framework of linear and quadratic generalized uncertainty principle.
{"title":"Thermodynamics of a Schwarzschild black hole surrounded by quintessence in the generalized uncertainty principle framework","authors":"Soham Sen, Abhijit Dutta, Sunandan Gangopadhyay","doi":"arxiv-2409.11073","DOIUrl":"https://doi.org/arxiv-2409.11073","url":null,"abstract":"We investigate the thermodynamics of a Schwarzschild black hole, surrounded\u0000by the quintessence energy-matter in the linear and quadratic generalized\u0000uncertainty principle framework. Considering the variance in the position to be\u0000of the order of the event horizon radius and equating the variance in the\u0000momentum to the Hawking temperature of the black hole, we substitute these\u0000variances in the deformed algebra. From there we obtained the generalized\u0000uncertainty principle-modified black hole temperature and eventually the\u0000specific heat of the black hole. Then we calculate the critical as well as the\u0000remnant mass and obtain the entropy relation. We observe that the entropy\u0000relation includes the usual leading order ``textit{area divided by four}\"\u0000term, sub-leading logarithmic term, and higher order inverse of the area\u0000corrections. Finally, calculating the energy output as a function of time, we\u0000obtain the evaporation time of the black hole. The results show the dependence\u0000of the quintessence parameter on the thermodynamic quantities in the framework\u0000of linear and quadratic generalized uncertainty principle.","PeriodicalId":501339,"journal":{"name":"arXiv - PHYS - High Energy Physics - Theory","volume":"17 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142251521","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}
Nicolas Chagnet, Sam Arend, Floris Balm, Martijn Janse, Joshua Saldi, Koenraad Schalm
We study DC magnetotransport in a quantum critical metal in the presence of a lattice. In the regime where the transport is hydrodynamical the interplay of the Lorentz force and the lattice gives rise to a natural anomalous contribution to the cyclotron frequency that changes it from its canonical charge-to-mass ratio. The size of this effect is universal as it is determined only by thermodynamic quantities. Remarkably the Drude weight changes in such a way that to first subleading order in the lattice strength the Hall resistivity and Hall coefficient do not change, though the Hall angle does change. We confirm our results with numerical simulations in a holographic model of a strange metal. For weak lattice strength these hydrodynamic effects are shown to be present. The numerical simulations also suggest that strong lattice effects beyond a hydrodynamic regime may provide a resolution to the experimentally observed anomalous Hall response of cuprate strange metals.
{"title":"Natural anomalous cyclotron response in a hydrodynamic local quantum critical metal in a periodic potential","authors":"Nicolas Chagnet, Sam Arend, Floris Balm, Martijn Janse, Joshua Saldi, Koenraad Schalm","doi":"arxiv-2409.11095","DOIUrl":"https://doi.org/arxiv-2409.11095","url":null,"abstract":"We study DC magnetotransport in a quantum critical metal in the presence of a\u0000lattice. In the regime where the transport is hydrodynamical the interplay of\u0000the Lorentz force and the lattice gives rise to a natural anomalous\u0000contribution to the cyclotron frequency that changes it from its canonical\u0000charge-to-mass ratio. The size of this effect is universal as it is determined\u0000only by thermodynamic quantities. Remarkably the Drude weight changes in such a\u0000way that to first subleading order in the lattice strength the Hall resistivity\u0000and Hall coefficient do not change, though the Hall angle does change. We\u0000confirm our results with numerical simulations in a holographic model of a\u0000strange metal. For weak lattice strength these hydrodynamic effects are shown\u0000to be present. The numerical simulations also suggest that strong lattice\u0000effects beyond a hydrodynamic regime may provide a resolution to the\u0000experimentally observed anomalous Hall response of cuprate strange metals.","PeriodicalId":501339,"journal":{"name":"arXiv - PHYS - High Energy Physics - Theory","volume":"17 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142251520","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}
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