We determine the solar neutrino fluxes from the global analysis of the most uptodate terrestrial and solar neutrino data including the final results of the three phases of Borexino. The analysis are performed in the framework of threeneutrino mixing with and without accounting for the solar luminosity constraint. We discuss the independence of the results on the input from the Gallium experiments. The determined fluxes are then compared with the predictions provided by the latest Standard Solar Models. We quantify the dependence of the model comparison with the assumptions about the normalization of the solar neutrino fluxes produced in the CNOcycle as well as on the particular set of fluxes employed for the model testing.
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A<sc>bstract</sc> Free, publiclyaccessible full text available February 1, 2025 
A<sc>bstract</sc> In this paper, we analyze the loop corrections to celestial OPE for gluons and gravitons. Even at the loop level, the soft gluons and gravitons have conformal dimensions ∆ = 1
− . The only novelty is the presence of higher poles. At one loop level, there are two types of conformal soft gluons with a single pole and a double pole in the ∆ plane. The celestial OPEs are obtained using the collinear splitting functions. In the case of gluons, the splitting functions receive loop corrections. After taking the holomorphic soft limit, we find the OPE of conformal soft gluons. We find a novel mixing of simple and double poles soft gluon operators in the OPE. In the case of gravitons, where splitting functions are known to be all loop exact, we still find a wedge algebra of$${\mathbb{Z}}_{\ge 0}$$ w _{∞}which is in addition to the wedge algebra ofw _{1+∞}already found by Strominger.Free, publiclyaccessible full text available March 1, 2025 
A<sc>bstract</sc> We develop a general expression for weighted cross sections in leptonic annihilation to hadrons based on timeordered perturbation theory (TOPT). The analytic behavior of the resulting integrals over spatial momenta can be analyzed in the language of Landau equations and infrared (IR) power counting. For any infraredsafe weight, the cancellation of infrared divergences is implemented locally at the integrand level, and in principle can be evaluated numerically in four dimensions. We go on to show that it is possible to eliminate unphysical singularities that appear in timeordered perturbation theory for arbitrary amplitudes. This is done by reorganizing TOPT into an equivalent form that combines classes of time orderings into a “partially timeordered perturbation theory”. Applying the formalism to leptonic annihilation, we show how to derive diagrammatic expressions with only physical unitarity cuts.
Free, publiclyaccessible full text available February 1, 2025 
By leveraging the physics of the Higgs branch, we argue that the conformal central charges$a$and$c$of an arbitrary 4D$\mathcal{N}=2$superconformal field theory (SCFT) are rational numbers. Our proof of the rationality of$c$is conditioned on a wellsupported conjecture about how the Higgs branch of an SCFT is encoded in its protected chiral algebra. To establish the rationality of$a$, we further rely on a widely believed technical assumption on the hightemperature limit of the superconformal index.
<supplementarymaterial><permissions><copyrightstatement>Published by the American Physical Society</copyrightstatement><copyrightyear>2024</copyrightyear></permissions></supplementarymaterial></sec> </div> <a href='#' class='show openabstract' style='marginleft:10px;'>more »</a> <a href='#' class='hide closeabstract' style='marginleft:10px;'>« less</a> <div class="actions" style="paddingleft:10px;"> <span class="readercount"> Free, publiclyaccessible full text available May 1, 2025</span> </div> </div><div class="clearfix"></div> </div> </li> <li> <div class="article item document" itemscope itemtype="http://schema.org/TechArticle"> <div class="iteminfo"> <div class="title"> <a href="https://par.nsf.gov/biblio/10509761blackholeperturbationtheorymultiplepolylogarithms" itemprop="url"> <span class='spanlink' itemprop="name">Black hole perturbation theory and multiple polylogarithms</span> </a> </div> <div> <strong> <a class="misc externallink" href="https://doi.org/10.1007/JHEP11(2023)059" target="_blank" title="Link to document DOI">https://doi.org/10.1007/JHEP11(2023)059 <span class="fas faexternallinkalt"></span></a> </strong> </div> <div class="metadata"> <span class="authors"> <span class="author" itemprop="author">Aminov, Gleb</span> <span class="sep">; </span><span class="author" itemprop="author">Arnaudo, Paolo</span> <span class="sep">; </span><span class="author" itemprop="author">Bonelli, Giulio</span> <span class="sep">; </span><span class="author" itemprop="author">Grassi, Alba</span> <span class="sep">; </span><span class="author" itemprop="author">Tanzini, Alessandro</span> </span> <span class="year">( <time itemprop="datePublished" datetime="20231101">November 2023</time> , Journal of High Energy Physics) </span> </div> <div style="cursor: pointer;webkitlineclamp: 5;" class="abstract" itemprop="description"> <title>A<sc>bstract</sc> We study black hole linear perturbation theory in a fourdimensional Schwarzschild (anti) de Sitter background. When dealing with a
positive cosmological constant, the corresponding spectral problem is solved systematically via the NekrasovShatashvili functions or, equivalently, classical Virasoro conformal blocks. However, this approach can be more complicated to implement for certain perturbations if the cosmological constant isnegative . For these cases, we propose an alternative method to set up perturbation theory for both small and large black holes in an analytical manner. Our analysis reveals a new underlying recursive structure that involves multiple polylogarithms. We focus on gravitational, electromagnetic, and conformally coupled scalar perturbations subject to Dirichlet and Robin boundary conditions. The lowlying modes of the scalar sector of gravitational perturbations and its hydrodynamic limit are studied in detail.Free, publiclyaccessible full text available November 1, 2024 
Abstract Baryon number conservation is not guaranteed by any fundamental symmetry within the standard model, and therefore has been a subject of experimental and theoretical scrutiny for decades. So far, no evidence for baryon number violation has been observed. Large underground detectors have long been used for both neutrino detection and searches for baryon number violating processes. The next generation of large neutrino detectors will seek to improve upon the limits set by past and current experiments and will cover a range of lifetimes predicted by several Grand Unified Theories. In this White Paper, we summarize theoretical motivations and experimental aspects of searches for baryon number violation in neutrino experiments.

A<sc>bstract</sc> We consider the 𝒩 = (2, 2) AdS_{3}/CFT_{2}dualities proposed by Eberhardt, where the bulk geometry is AdS_{3}× (
S ^{3}×T ^{4})/ℤ_{k}, and the CFT is a deformation of the symmetric orbifold of the supersymmetric sigma modelT ^{4}/ℤ_{k}(withk = 2, 3, 4, 6). The elliptic genera of the two sides vanish due to fermionic zero modes, so for microstate counting applications one must consider modified supersymmetric indices. In an analysis similar to that of Maldacena, Moore, and Strominger for the standard 𝒩 = (4, 4) case ofT ^{4}, we study the appropriate helicitytrace index of the boundary CFTs. We encounter a strange phenomenon where a saddlepoint analysis of our indices reproduces only a fraction (respectively ,$$ \frac{1}{2} $$ $\frac{1}{2}$ ,$$ \frac{2}{3} $$ $\frac{2}{3}$ ,$$ \frac{3}{4} $$ $\frac{3}{4}$ ) of the BekensteinHawking entropy of the associated macroscopic black branes.$$ \frac{5}{6} $$ $\frac{5}{6}$Free, publiclyaccessible full text available January 1, 2025 
A<sc>bstract</sc> In [1], logarithmic correction to subleading soft photon and soft graviton theorems have been derived in four spacetime dimensions from the ratio of IRfinite Smatrices. This has been achieved after factoring out IRdivergent components from the traditional electromagnetic and gravitational Smatrices using GrammerYennie prescription. Although the loop corrected subleading soft theorems are derived from oneloop scattering amplitudes involving scalar particles in a minimally coupled theory with scalar contact interaction, it has been conjectured that the soft factors are universal (theory independent) and oneloop exact (don’t receive corrections from higher loops).
This paper extends the analysis conducted in [1] to encompass general spinning particle scattering with nonminimal couplings permitted by gauge invariance and general coordinate invariance. By rederiving the ln
ω soft factors in this generic setup, we establish their universal nature. Furthermore, we summarize the results of loop corrected soft photon and graviton theorems up to subsubleading order, which follows from the analysis of one and two loop QED and quantum gravity Smatrices. While the classical versions of these soft factors have already been derived in the literature, we put forth conjectures regarding the quantum soft factors and outline potential strategies for their derivation.Free, publiclyaccessible full text available November 1, 2024 
A<sc>bstract</sc> The interpretation of Higgs data is typically based on different assumptions about whether there can be additional decay modes of the Higgs or if any couplings can be bounded by theoretical arguments. Going beyond these assumptions requires either a precision measurement of the Higgs width or an absolute measurement of a coupling to eliminate a flat direction in precision fits that occurs when
> 1, where$$ \left{g}_{hVV}/{g}_{hVV}^{SM}\right $$ $\left({g}_{\mathrm{hVV}}/{g}_{\mathrm{hVV}}^{\mathrm{SM}}\right)$V =W ^{±},Z . In this paper we explore how well a high energy muon collider can test Higgs physics without having to make assumptions on the total width of the Higgs. In particular, we investigate offshell methods for Higgs production used at the LHC and searches for invisible decays of the Higgs to see how powerful they are at a muon collider. We then investigate the theoretical requirements on a model which can exist in such a flat direction. Combining expected Higgs precision with other constraints, the most dangerous flat direction is described by generalized GeorgiMachacek models. We find that by combining direct searches with Higgs precision, a high energy muon collider can robustly test single Higgs precision down to the level without having to assume SM Higgs decays. Furthermore, it allows one to bound new contributions to the width at the subpercent level as well. Finally, we comment on how even in this difficult flat direction for Higgs precision, a muon collider can robustly test or discover new physics in multiple ways. Expanding beyond simple coupling modifiers/EFTs, there is a large region of parameter space that muon colliders can explore for EWSB that is not probed with only standard Higgs precision observables.$$ \mathcal{O}\left(.1\%\right) $$ $O\left(.1\%\right)$Free, publiclyaccessible full text available January 1, 2025 
Abstract Dark matter freezein is a compelling cosmological production mechanism in which all or some of the observed abundance of dark matter is generated through feeble interactions it has with the Standard Model. In this work we present the first analysis of freezein dark matter fluctuations and consider two benchmark models: freezein through the direct decay of a heavy vector boson and freezein through pair annihilation of Standard Model particles in the thermal bath. We provide a theoretical framework for determining the impact of freezein on curvature and dark matter isocurvature perturbations. We determine freezein dark matter fluid properties from first principles, tracking its evolution from its relativistic production to its final cold state, and calculate the evolution of the dark matter isocurvature perturbation. We find that in the absence of initial isocurvature, the freezein production of dark matter does not source isocurvature. However, for an initial isocurvature perturbation seeded by inflation, the nonthermal freezein process may allow for a fraction of the isocurvature to persist, in contrast to the exponential suppression it receives in the case of thermal dark matter. In either case, the evolution of the curvature mode is unaffected by the freezein process. We show sensitivity projections of future cosmic microwave background experiments to the amplitude of uncorrelated, totally anticorrelated, and totally correlated dark matter isocurvature perturbations. From these projections, we infer the sensitivity to the abundance of freezein dark matter that sustains some fraction of the primordial isocurvature.
Free, publiclyaccessible full text available November 1, 2024