The Monte Carlo (MC) replica method quantifies parameter uncertainties in global fits of parton distribution functions (PDFs) and Standard Model Effective Field Theory (SMEFT) Wilson coefficients by fitting a model to many noise-perturbed copies of the data and taking the empirical distribution of the best-fit parameters as the uncertainty. The method reproduces the Bayesian posterior exactly only when the model is linear in its parameters, and departs from it in the nonlinear case. We derive the leading-order distribution the method produces and compare it with the Laplace approximation of the Bayesian posterior: the two differ by a single computable matrix, the residual-weighted Hessian of the model at the best fit, whose sign and magnitude set the over- or under-estimation of the parameter uncertainties. This closed-form expression quantifies when and by how much the MC method departs from Bayesian inference. We illustrate it on two single-parameter examples solvable in closed form and point to its evaluation in full PDF and SMEFT fits as a natural next step.
{"title":"Propagating data noise through the fit: the Monte Carlo replica distribution","authors":"Mark N. Costantini","doi":"10.1007/JHEP10(2026)246","DOIUrl":"10.1007/JHEP10(2026)246","url":null,"abstract":"<p>The Monte Carlo (MC) replica method quantifies parameter uncertainties in global fits of parton distribution functions (PDFs) and Standard Model Effective Field Theory (SMEFT) Wilson coefficients by fitting a model to many noise-perturbed copies of the data and taking the empirical distribution of the best-fit parameters as the uncertainty. The method reproduces the Bayesian posterior exactly only when the model is linear in its parameters, and departs from it in the nonlinear case. We derive the leading-order distribution the method produces and compare it with the Laplace approximation of the Bayesian posterior: the two differ by a single computable matrix, the residual-weighted Hessian of the model at the best fit, whose sign and magnitude set the over- or under-estimation of the parameter uncertainties. This closed-form expression quantifies when and by how much the MC method departs from Bayesian inference. We illustrate it on two single-parameter examples solvable in closed form and point to its evaluation in full PDF and SMEFT fits as a natural next step.</p>","PeriodicalId":635,"journal":{"name":"Journal of High Energy Physics","volume":"2026 10","pages":""},"PeriodicalIF":5.5,"publicationDate":"2026-10-23","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1007/JHEP10(2026)246.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"149235083","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Thermal fluctuations are generally expected to destroy order and restore symmetries at sufficiently high temperatures. Recently, however, a family of scalar theories in 2 + 1 dimensions was shown to exhibit ℤ2 symmetry breaking that persists to arbitrarily high temperatures using a variety of approaches, including the ϵ-expansion, the FRG, and large-N techniques. Although the similarities among these theories suggest that they belong to the same universality class, this connection has not been established explicitly. In this work, we fill this gap. Using large-N methods, we analytically study the biconical vector model in a range of spacetime dimensions, including 2 + 1, at leading and next-to-leading order in the 1/N expansion. We determine the RG flow, fixed-point structure, and the CFT data of the infrared theory, reproducing and extending previous results and thereby unifying the apparently distinct constructions within a common analytic framework. We derive the effective potential, establish its stable minima at zero and finite temperature, and demonstrate spontaneous ℤ2 symmetry breaking at arbitrarily high temperatures for large finite N.
{"title":"Thermal order in the biconical model","authors":"Michael Smolkin, Lev Yung","doi":"10.1007/JHEP10(2026)245","DOIUrl":"10.1007/JHEP10(2026)245","url":null,"abstract":"<p>Thermal fluctuations are generally expected to destroy order and restore symmetries at sufficiently high temperatures. Recently, however, a family of scalar theories in 2 + 1 dimensions was shown to exhibit <i>ℤ</i><sub>2</sub> symmetry breaking that persists to arbitrarily high temperatures using a variety of approaches, including the <i>ϵ</i>-expansion, the FRG, and large-<i>N</i> techniques. Although the similarities among these theories suggest that they belong to the same universality class, this connection has not been established explicitly. In this work, we fill this gap. Using large-<i>N</i> methods, we analytically study the biconical vector model in a range of spacetime dimensions, including 2 + 1, at leading and next-to-leading order in the 1/<i>N</i> expansion. We determine the RG flow, fixed-point structure, and the CFT data of the infrared theory, reproducing and extending previous results and thereby unifying the apparently distinct constructions within a common analytic framework. We derive the effective potential, establish its stable minima at zero and finite temperature, and demonstrate spontaneous <i>ℤ</i><sub>2</sub> symmetry breaking at arbitrarily high temperatures for large finite <i>N</i>.</p>","PeriodicalId":635,"journal":{"name":"Journal of High Energy Physics","volume":"2026 10","pages":""},"PeriodicalIF":5.5,"publicationDate":"2026-10-23","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1007/JHEP10(2026)245.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"149234993","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
We calculate the “kinematic” corrections ( t/{P}_z^2 ) and ( {m}_N^2/{P}_z^2 ) to the short distance expansion of gauge-invariant nonlocal quark-antiquark operators sandwiched between nucleon states with different momenta. Here t is the momentum transfer, mN is the nucleon mass and Pz is the momentum component in the direction of the quark-antiquark separation, which is assumed to be large. These matrix elements can be calculated in lattice QCD and, at leading twist, expressed in terms of moments of the generalized parton distributions (GPDs). Our results allow one to control one of principal uncertainties in such calculations and extend their region of applicability to larger momentum transfers, which is important in the quest to access the three-dimension image of the proton. The calculated corrections turn out to be significant for a realistic lattice QCD setup.
{"title":"Finite-t and target mass corrections for the short-distance expansion of quasi(pseudo) GPDs","authors":"Vladimir M. Braun, Hua-Yu Jiang","doi":"10.1007/JHEP10(2026)244","DOIUrl":"10.1007/JHEP10(2026)244","url":null,"abstract":"<p>We calculate the “kinematic” corrections <span>( t/{P}_z^2 )</span> and <span>( {m}_N^2/{P}_z^2 )</span> to the short distance expansion of gauge-invariant nonlocal quark-antiquark operators sandwiched between nucleon states with different momenta. Here <i>t</i> is the momentum transfer, <i>m</i><sub><i>N</i></sub> is the nucleon mass and <i>P</i><sub><i>z</i></sub> is the momentum component in the direction of the quark-antiquark separation, which is assumed to be large. These matrix elements can be calculated in lattice QCD and, at leading twist, expressed in terms of moments of the generalized parton distributions (GPDs). Our results allow one to control one of principal uncertainties in such calculations and extend their region of applicability to larger momentum transfers, which is important in the quest to access the three-dimension image of the proton. The calculated corrections turn out to be significant for a realistic lattice QCD setup.</p>","PeriodicalId":635,"journal":{"name":"Journal of High Energy Physics","volume":"2026 10","pages":""},"PeriodicalIF":5.5,"publicationDate":"2026-10-23","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1007/JHEP10(2026)244.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"149234994","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}