PaperPanorama

HEP Phenomenology·hep-ph

Fri·Jun 14, 2024

26 papers15 primary·11 cross-listed·reconstructed*

  1. 01*

    SHIFT@LHC: Searches for New Physics with Shifted Interaction on a Fixed Target at the Large Hadron Collider

    Jeremi Niedziela🇩🇪

    New low-mass particles with very small couplings to standard model particles that travel significant distances before decaying are interesting candidates to address some of the most intriguing questions of modern physics. In this paper, I propose to extend the LHC's research program by installing a gaseous fixed target referred to as SHIFT at around 160 meters from the CMS interaction point. When the LHC proton beam collides with this target, interactions at a center of mass energy of 113 GeV would occur. The particles produced in such collisions, or their decay products, would travel through the rock and other material on their path, potentially reaching the CMS detector where they can be registered and studied. Such an approach would allow us to access otherwise uncovered regions of parameters phase space at a relatively low cost since it does not require constructing a new detector. Various aspects such as angular and lifetime coverage or material survival probability have been studied. The results are interpreted within two new physics models, namely, the Dark Photons and the Hidden Valley scenarios, and compared with the standard proton-proton physics program of CMS. A comparison is also made with the fixed target program at LHCb, as well as parasitic detectors such as FASER or MATHUSLA. The obtained results indicate that, despite assuming just 1% of the nominal CMS luminosity to be available to SHIFT, the physics reach could be extended by a factor of up to 150 (1000) for Dark Photon (Hidden Valley) scenarios, depending on the signal model parameters.

    hep-phhep-exJHEP(2024)·12 citations
  2. 02*

    The connection between Nucleon Energy Correlators and Fracture Functions

    Kai-Bao Chen🇨🇳 · Jian-Ping Ma🇨🇳 · Xuan-Bo Tong🇫🇮

    We establish a sum rule that connects fracture functions to nucleon energy-energy correlators~(NEECs) in a one-to-one correspondence. Using this sum rule, we study the energy pattern in the target fragmentation region of deep inelastic scatterings. Through investigations up to twist-3, we express all eighteen energy-pattern structure functions in terms of associated NEECs, elucidating various azimuthal and spin asymmetries critical for nucleon tomography. Additionally, we investigate the perturbative matching of the twist-2 quark NEECs. We demonstrate that the Sivers-type and worm-gear-type quark NEECs match onto twist-3 multi-parton distributions. Our work provides a framework for examining energy-weighted observables through hadron production processes in the target fragmentation region, offering new insights into nucleon tomography.

    hep-phnucl-thJHEP(2024)·24 citations
  3. 03*

    FastEEC: Fast Evaluation of N-point Energy Correlators

    Ankita Budhraja🇳🇱 · Wouter J. Waalewijn🇳🇱

    Energy correlators characterize the asymptotic energy flow in scattering events produced at colliders, from which the microscopic physics of the scattering can be deduced. This view of collisions is akin to analyses of the Cosmic Microwave Background, and a range of promising phenomenological applications of energy correlators have been identified, including the study of hadronization, the deadcone effect, measuring and the top quark mass. While -point energy correlators are interesting to study for larger values of , their evaluation is computationally intensive, scaling like , where is the number of particles. In this Letter, we develop a fast, approximate method for their evaluation exploiting that correlations at a given angular scale are insensitive to effects at other (widely-separated) scales. This implies that the energy correlator can be computed on (sub)jets, effectively reducing M. Furthermore, we utilize a dynamical (sub)jet radius that allows us to obtain reliable results without restricting the angular scales being probed. For concreteness we focus on the projected energy correlator, which projects onto the largest separation between the directions. E.g.~for we find a speed up of up to four orders of magnitude, depending on the desired accuracy. We also consider the possibility of raising the energy to a power higher than one in the energy correlator, which has been proposed to reduce soft sensitivity, and further cuts back the required computation time. These higher-power correlators are not collinear safe, but as a byproduct our approach suggests a natural method to regularize them, such that they can be described using perturbation theory. This letter is accompanied by a public code that implements our method.

    hep-phhep-exnucl-thPLB(2025)·12 citations
  4. 04*

    Dark Neutrino Moments From Light Loops

    Gonzalo Herrera🇺🇸 · Ian M. Shoemaker🇺🇸

    Active and sterile neutrinos may acquire "dark moments" via one-loop diagrams with a massless dark photon and new light particles in the loop. Due to the kinetic mixing between the dark photon and the Standard Model photon, neutrinos would obtain effective electromagnetic moments. This mechanism allows for enhanced electromagnetic moments that can evade constraints on particles directly charged under electromagnetism. We show that in a wide region of parameter space, the model features testable predictions for the anapole and magnetic moment of active and sterile neutrinos with dark matter direct detection experiments sensitive to the solar neutrino flux.

    hep-phastro-ph.CO2 citations
  5. 05*

    The Generalized Scalar Weak Gravity Conjecture and its Implications

    Fayez Abu-Ajamieh🇮🇳 · Nobuchika Okada🇺🇸 · Sudhir K. Vempati🇮🇳

    We propose a generalized formulation of the Scalar Weak Gravity Conjecture (SWGC) based on the analogy with the derivation of the Gauge Weak Gravity Conjecture (GWGC). We discuss some phenomenological implications of this Generalized SWGC, including the scale of New Physics (NP) when applied to the SM Higgs sector, and the bounds on the axion's couplings to fermions and the photon when applied to the axion. The Generalized SWGC constraints rule out most of the parameter space of axion-nucleon couplings, leaving only a tiny parameter space.

    hep-phPLB(2025)·4 citations
  6. 06*

    in the Diabatic Diquark Model: Effects of Isospin

    Richard F. Lebed🇺🇸 · Steven R. Martinez🇺🇸

    is an isoscalar 4-quark state with mass lying barely below the threshold, and several times further below the threshold. It allows both di-meson molecular and elementary diquark-antidiquark substructures. The diabatic generalization of the adiabatic approximation within the Born-Oppenheimer formalism rigorously incorporates the mixing of such elementary eigenstates with states corresponding to two-particle thresholds. We examine the separate influence of the two isospin channels and find that the influence of is larger than that of but not overwhelmingly so, and that contains an component. We then explore the variation of these results if the isospin breaking between the di-meson thresholds is varied, and also the sensitivity of our results to variation of the mixing-potential parameters.

    hep-phPRD(2024)·12 citations
  7. 07*

    Scotogenic gauge mechanism for neutrino mass and dark matter

    Phung Van Dong🇻🇳 · Nguyen Huy Thao🇻🇳

    Scotogenic is a scheme for neutrino mass generation through the one-loop contribution of an inert scalar doublet and three sterile neutrinos. This work argues that such inert scalar doublet is a Goldstone boson mode associated with a gauge symmetry breaking. Hence, the resultant scotogenic gauge mechanism is very predictive, generating neutrino mass as contributed by a new gauge boson doublet that eats such Goldstone bosons. The dark matter stability is manifestly ensured by a matter parity as residual gauge symmetry for which a vector dark matter candidate is hinted.

    hep-phCommun.in Phys.(2024)·1 citation
  8. 08*

    Energy-momentum tensor in theory at one loop

    Brean Maynard🇺🇸

    The energy-momentum tensor form factors are studied in theory to one-loop order with particular focus on the -term, a particle property which has attracted a lot of attention in the recent literature. It is shown that the free Klein-Gordon theory value of the -term is reduced to even if the interaction is infinitesimally small. A companion work in theory confirms this result which may indicate that it is independent of the type of interaction as long as the scalar theory is renormalizable. Dispersion relations are studied. Various definitions of mean square radii including the mechanical radius are investigated. The findings contribute to a better understanding of the EMT properties of particles and their interpretation.

    hep-phPRD(2025)·9 citations
  9. 09*

    W-boson pair production at lepton colliders in the Feynman-diagram gauge

    Hiroyuki Furusato🇯🇵 · Kentarou Mawatari🇯🇵 · Yutaro Suzuki🇯🇵 · Ya-Juan Zheng🇯🇵

    We calculate helicity amplitudes for analytically in the Feynman-diagram (FD) gauge. We show that, unlike in the unitary gauge, there is no energy growth of the individual Feynman amplitudes for the longitudinally polarized W bosons, and the contributions from the associated Goldstone bosons are manifest even without taking the high-energy limit. We also find that the physical distributions can be interpreted by the individual amplitudes in the FD gauge.

    hep-phPRD(2024)·5 citations
  10. 10*

    Pseudo-Nambu-Goldstone Boson Production from Inflaton Coupling during Reheating

    Kunio Kaneta🇯🇵 · Sung Mook Lee🇰🇷 · Kin-ya Oda🇯🇵 · Tomo Takahashi🇯🇵

    The existence of pseudo-Nambu-Goldstone boson (pNGB) fields is a common feature in many models beyond the Standard Model, characterized by their exclusive derivative couplings. This paper investigates a scenario where a pNGB is coupled to the inflaton field during the reheating phase of the early universe. We calculate the perturbative decay rate of a coherently oscillating inflaton into pNGBs on a general basis, considering both constant and field-dependent couplings with monomial potentials at the minimum. As a concrete application, we explore the production of axions when the radial mode of the Peccei-Quinn (PQ) scalar serves as the inflaton, particularly in the presence of a large gravitational non-minimal coupling. Our findings suggest that the presence of pNGBs during reheating can lead to significant non-thermal relics, offering new constraints on inflationary reheating models and providing potential observational signatures in the form of dark radiation.

    hep-phastro-ph.COgr-qchep-thJCAP(2024)·5 citations
  11. 11*

    Vector-like quarks: status and new directions at the LHC

    Avik Banerjee🇸🇪 · Elin Bergeaas Kuutmann🇸🇪 · Venugopal Ellajosyula🇸🇪 · Rikard Enberg🇸🇪 · Gabriele Ferretti🇸🇪 · Luca Panizzi🇮🇹

    Experimental searches for vector-like quarks have until now only considered their decays into Standard Model particles. However, various new physics scenarios predict additional scalars, so that these vector-like quarks can decay to new channels. These new channels reduce the branching ratios into Standard Model final states, significantly affecting current mass bounds. In this article, we quantitatively assess the relevance and observability of single and pair production processes of vector-like quarks, followed by decays into both standard and exotic final states. We highlight the importance of large widths and the relative interaction strengths with Standard Model particles and new scalars. Then, we review the post-Moriond 2024 status of these models in light of available LHC data and discuss potential future strategies to enhance the scope of vector-like quark searches.

    hep-phhep-exSciPost Phys.Core(2024)·47 citations
  12. 12*

    Absorptive corrections to the electromagnetic form factor in high-energy elastic proton-proton scattering

    Andrei Poblaguev🇺🇸

    Recently, it was noted that absorptive corrections to the electromagnetic form factor in high-energy proton-proton scattering are important for the theoretical interpretation of the and analyzing power measurements with the Hydrogen Jet Target polarimeter (HJET) at RHIC. Here, a concise expression for the absorptive correction was derived within the eikonal approach. The resulting analysis reveals a systematic bias, nearly independent of the beam energy, in the experimental determination of the real-to-imaginary ratio when absorption effects are overlooked in the data analysis. Quantification of this bias, as , was achieved using a Regge fit applied to available proton-proton measurements of and . Considering the potential impact of such an effect on the experimentally determined , one may enhance consistency between the HJET and STAR measurements of the hadronic spin-flip amplitude. While the sign of the bias in the value of aligns with the anticipated effective increase in the proton charge radius in scattering due to absorption, it amplifies the observed discrepancy between and values at as measured in the TOTEM experiment. Evaluation (using published TOTEM data) of the measured proton-proton dependence on the absorptive corrections indicated that possible soft photon corrections to the hadronic amplitude slope may be essential for such data analysis.

    hep-phPRD(2024)·2 citations
  13. 13*

    Extraction of Information from Polarized Deep Exclusive Scattering with Machine Learning

    Simonetta Liuti🇺🇸

    A framework defining benchmarks for the analysis of polarized exclusive scattering cross sections is proposed that uses physics symmetry constraints as well as lattice QCD predictions. These constraints are built into machine learning (ML) algorithms. Both physics driven and ML based benchmarks are applied to a wide range of deeply virtual exclusive processes through explainable ML techniques with controllable uncertainties. The observables, namely the Compton Form Factors (CFFs) which are convolutions of Generalized Parton Distributions (GPDs), are extracted using methods such as the random targets method to evaluate the separate contribution of the aleatoric and epistemic uncertainties in exclusive scattering analyses.

    hep-ph1 citation
  14. 14*

    Novel azimuthal observables from two-photon collision at colliders

    Yu Jia🇨🇳 · Jian Zhou🇨🇳 · Ya-jin Zhou🇨🇳

    In this work we advocate a set of novel azimuthal-angle-related observables associated with exclusive hadron production from two-photon fusion at colliders, taking the as a benchmark process. As a direct consequence of the linearly polarized quasi-real photons emitted off the electron and positron beams, the azimuthal asymmetry in dipion production is predicted within the transverse-momentum-dependent (TMD) factorization framework. In numerical analysis, we take the helicity amplitudes of determined from the partial wave solutions in dispersion relation as input, and find that the predicted azimuthal modulation may reach 40\% for the typical kinematical setup of {\tt Belle 2} and {\tt BESIII} experiments. Future accurate measurement of this azimuthal asymmetry may facilitate the direct extraction of the relative phase between two helicity amplitudes with photon helicity configurations and . This knowledge provides a valuable input for the dispersive determination of the hadronic light-by-light (Hlbl) contributions.

    hep-phhep-exPRL(2025)·7 citations
  15. 15*

    Axion Stars: Mass Functions and Constraints

    Jae Hyeok Chang🇺🇸 · Patrick J. Fox🇺🇸 · Huangyu Xiao🇺🇸

    The QCD axion and axion-like particles, as leading dark matter candidates, can also have interesting implications for dark matter substructures if the Peccei-Quinn symmetry is broken after inflation. In such a scenario, axion perturbations on small scales will lead to the formation of axion miniclusters at matter-radiation equality, and subsequently the formation of axion stars. Such compact objects open new windows for indirect searches for axions. We compute the axion star mass function based on recent axion minicluster studies and Bose star simulations. Applying this mass function, we find post-inflation axion-like particles with masses are constrained by the lack of dynamical heating of stars in ultrafaint dwarfs. We also find that current microlensing surveys are insensitive to QCD axion stars. While we focus on the gravitational detectability of axion stars, our result can be directly applied to other interesting signatures of axion stars, e.g. their decay to photons, that require as input the abundance, mass, and density distribution of axion stars.

    hep-phastro-ph.COJCAP(2024)·24 citations
  16. 16*

    Tagging more quark jet flavours at FCC-ee at 91 GeV with a transformer-based neural network

    Freya Blekman🇩🇪 · Florencia Canelli🇨🇭 · Alexandre De Moor🇧🇪 · Kunal Gautam🇧🇪 · Armin Ilg🇨🇭 · Anna Macchiolo🇨🇭 · Eduardo Ploerer🇧🇪

    Jet flavour tagging is crucial in experimental high-energy physics. A tagging algorithm, DeepJetTransformer, is presented, which exploits a transformer-based neural network that is substantially faster to train than state-of-the-art graph neural networks. The DeepJetTransformer algorithm uses information from particle flow-style objects and secondary vertex reconstruction for - and -jet identification, supplemented by additional information that is not always included in tagging algorithms at the LHC, such as reconstructed and and discrimination. The model is trained as a multiclassifier to identify all quark flavours separately and performs excellently in identifying - and -jets. An -tagging efficiency of can be achieved with a -jet background efficiency. The performance improvement achieved by including and reconstruction and discrimination is presented. The algorithm is applied on exclusive samples to examine the physics potential and is shown to isolate events. Assuming all non- backgrounds can be efficiently rejected, a discovery significance for can be achieved with an integrated luminosity of of collisions at , corresponding to less than a second of the FCC-ee run plan at the boson resonance.

    hep-exhep-phEPJC(2025)·28 citations
  17. 17*

    Constraints on Ultra Heavy Dark Matter Properties from Dwarf Spheroidal Galaxies with LHAASO Observations

    Zhen Cao🇨🇳 · F. Aharonian🇮🇪 · Q. An🇨🇳 · Axikegu🇨🇳 · Y.X. Bai🇨🇳 · Y.W. Bao🇨🇳 · D. Bastieri🇨🇳 · X.J. Bi🇨🇳 · Y.J. Bi🇨🇳 · J.T. Cai🇨🇳 · Q. Cao🇨🇳 · W.Y. Cao🇨🇳 and 268 other authors

    In this work we try to search for signals generated by ultra-heavy dark matter at the Large High Altitude Air Shower Observatory (LHAASO) data. We look for possible gamma-ray by dark matter annihilation or decay from 16 dwarf spheroidal galaxies in the field of view of LHAASO. Dwarf spheroidal galaxies are among the most promising targets for indirect detection of dark matter which have low fluxes of astrophysical -ray background while large amount of dark matter. By analyzing more than 700 days observational data at LHAASO, no significant dark matter signal from 1 TeV to 1 EeV is detected. Accordingly we derive the most stringent constraints on the ultra-heavy dark matter annihilation cross-section up to EeV. The constraints on the lifetime of dark matter in decay mode are also derived.

    astro-ph.HEhep-phPRL(2024)·30 citations
  18. 18*

    Exploring Faraday rotation signatures and population bounds for primordial magnetic black holes

    Arka Banerjee🇮🇳 · Lalit Singh Bhandari🇮🇳 · Ashwat Jain🇬🇧 · Arun M. Thalapillil🇮🇳

    Primordial black holes bearing magnetic charges may bypass the constraints imposed by Hawking radiation, thereby enabling reasonable present-day populations, even for masses below --a range previously considered improbable. They could, therefore, conceivably contribute to a component of dark matter. We investigate novel Faraday rotation signatures exhibited by primordial magnetic black holes while also establishing new Parker-type bounds on their populations. For the latter, we bound the dark matter fraction from intergalactic magnetic fields in cosmic voids and cosmic web filaments , notably eclipsing previous bounds. Exploring Faraday rotation effects, we discern a pronounced rotation of the polarization angle and the rotation measure values for extremal primordial magnetic black holes with masses . This makes them potentially detectable in current observations. A comparative investigation finds that the effects are notably greater than for a neutron star, like a Magnetar, with a similar magnetic field at the surface. Moreover, the polarization angle maps for primordial magnetic black holes exhibit unique features, notably absent in other astrophysical magnetic configurations. In this context, we also introduce a simple integral measure, offering a quantitative measure for their discrimination in many scenarios. These traits potentially suggest a robust avenue for their observational detection and differentiation.

    astro-ph.COhep-phhep-thJCAP(2025)·9 citations
  19. 19*

    Stabilization of a twisted modulus on a mirror of rigid Calabi-Yau manifold

    Keiya Ishiguro🇯🇵 · Takafumi Kai🇯🇵 · Hajime Otsuka🇯🇵

    We study the stabilization of a twisted modulus in Type IIB flux compactifications on a mirror of the rigid Calabi-Yau threefold. By analyzing the effective action of twisted and untwisted moduli, we find that three-form fluxes satisfying the tadpole cancellation conditions lead to supersymmetric AdS vacua. We also investigate swampland conjectures on this non-geometric background.

    hep-thhep-phJHEP(2024)·7 citations
  20. 20*

    MURCA driven Bulk viscosity in neutrino trapped baryonic matter

    Sreemoyee Sarkar🇮🇳 · Rana Nandi🇮🇳

    We examine bulk viscosity, taking into account trapped neutrinos in baryonic matter, in the context of binary neutron star mergers. Following the merging event, the binary star can yield a remnant compact object with densities up to nuclear saturation density and temperature upto MeV resulting in the retention of neutrinos. We employ two relativistic mean field models, NL3 and DDME2, to describe the neutrino-trapped baryonic matter. The dissipation coefficient is determined by evaluating the Modified URCA interaction rate in the dense baryonic medium, and accounting for perturbations caused by density oscillations. We observe the resonant behavior of bulk viscosity as it varies with the temperature of the medium. The bulk viscosity peak remains within the temperature range of MeV, depending upon the underlying equation of states and lepton fractions. This temperature range corresponds to the relevant domain of binary neutron star mergers. We also note that in presence of neutrinos in the medium the bulk viscosity peak shifts towards higher temperature and the peak value of bulk viscosity also changes. The time scale of viscous dissipation is dictated by the beta-off-equilibrium susceptibilities derived from the nuclear equation of state. The resulting viscous decay time scale ranges from milliseconds, which aligns with the order of magnitude of the post-merger object's survival time in some specific scenarios.

    nucl-thastro-ph.HEhep-phEPJC(2024)·4 citations
  21. 21*

    Primordial black hole formation from self-resonant preheating?

    Guillermo Ballesteros🇪🇸 · Joaquim Iguaz Juan🇺🇸 · Paquale D. Serpico🇫🇷 · Marco Taoso🇮🇹

    We revisit the question of how generic is the formation of primordial black holes via self-resonant growth of inflaton fluctuations in the post-inflationary, preheating phase. Using analytical and lattice calculations, we find that primordial black hole production is far from being a generic outcome. Also, in most of the parameter space of viable inflationary models, the metric preheating term is subleading to the anharmonic terms and the approximation of a quadratic potential for describing the resonance dynamics is inadequate. Nonetheless, the anharmonicity of the potential cannot be used to rescue the mechanism: The generic outcome of the non-linear evolution of the scalar field in this case is the formation of metastable transients or oscillons, that do not generically collapse into black holes.

    astro-ph.COgr-qchep-phhep-thPRD(2025)·18 citations
  22. 22*

    To curve, or not to curve: Is curvature-assisted quintessence observationally viable?

    George Alestas🇪🇸 · Matilda Delgado🇪🇸 · Ignacio Ruiz🇪🇸 · Yashar Akrami🇪🇸 · Miguel Montero🇪🇸 · Savvas Nesseris🇪🇸

    Single-field models of accelerated expansion with nearly flat potentials, despite being able to provide observationally viable explanations for the early-time cosmic inflation and the late-time cosmic acceleration, are in strong tension with string theory evidence and the associated de Sitter swampland constraints. It has recently been argued that in an open universe, where the spatial curvature is negative (i.e., with ), a new stable fixed point arises, which may lead to viable single-field-based accelerated expansion with an arbitrarily steep potential. Here, we show, through a dynamical systems analysis and a Bayesian statistical inference of cosmological parameters, that the additional cosmological solutions based on the new fixed point do not render steep-potential, single-field, accelerated expansion observationally viable. We mainly focus on quintessence models of dark energy, but we also argue that a similar conclusion can be drawn for cosmic inflation.

    hep-thastro-ph.COgr-qchep-phPRD(2024)·30 citations
  23. 23*

    Final-state interactions in neutrino-induced proton knockout from argon in MicroBooNE

    A. Nikolakopoulos🇺🇸 · A. Ershova🇫🇷 · R. González-Jiménez🇪🇸 · J. Isaacson🇺🇸 · A. M. Kelly🇺🇸 · K. Niewczas🇧🇪 · N. Rocco🇺🇸 · F. Sánchez🇨🇭

    Neutrino event generators make use of intranuclear cascade models (INCs), to predict the kinematics of hadrons produced in neutrino-nucleus interactions. We perform a consistent comparison of different INCs, by using the same set of events as input to the NEUT, NuWro, Achilles and INCL INCs. The inputs correspond to calculations of the fully differential single-proton knockout cross section, either in the distorted-wave impulse approximation (DWIA) or plane-wave impulse approximation (PWIA), both including realistic nuclear hole spectral functions. We compare the INC results to DWIA calculations with an optical potential, used extensively in the analysis of (e,e'p) experiments. We point out a systematic discrepancy between both approaches. We apply the INC results to recent MicroBooNE data. We assess the influence of the choice of spectral function, finding that large variations in realistic spectral functions are indistinguishable with present data. The data is underpredicted, with strength missing in the region where two-nucleon knockout and resonance production contribute. However, the data is underpredicted also in regions of low transverse missing momentum, where one-nucleon knockout dominates. The inclusion of the interference with two-body currents could lead to additional strength in this region.

    nucl-thhep-exhep-phPRC(2024)·17 citations
  24. 24*

    Illuminating the Cosmos: Dark matter, primordial black holes, and cosmic dawn

    Wenzer Qin🇺🇸

    The -CDM model of cosmology has done much to clarify our picture of the early universe. However, there are still some questions that -CDM does not necessarily answer; questions such as what is the fundamental nature of dark matter? What is its origin? And what causes the intriguing measurements that we are seeing from cosmic dawn? In this thesis, I will describe three directions in which I have pushed forward our understanding of how fundamental physics manifests in cosmology. First, I have studied the signatures of exotic energy injection in various astrophysical and cosmological probes, including the Lyman- forest, the blackbody spectrum of the cosmic microwave background, the power spectrum of the cosmic microwave background, and the formation of the earliest stars in our universe. Second, I have investigated the formation of primordial black hole dark matter in a general model for inflation with multiple scalar fields. I have identified the space of models that can generate primordial black holes while remaining in compliance with observational constraints using a Markov Chain Monte Carlo, and also showed that future gravitational wave observatories will be able to further constrain these models. Finally, I have developed an analytic description of signals from 21\,cm cosmology using methods inspired by effective field theory. This method includes realistic observational effects and has been validated against state-of-the-art radiation hydrodynamic simulations, including those with alternative dark matter scenarios. With these recent efforts, we are advancing the frontiers of dark matter phenomenology and cosmology, thereby paving the way towards illuminating the remaining mysteries of our cosmos and drawing closer to a comprehensive understanding of the universe.

    astro-ph.COhep-ph1 citation
  25. 25*

    PSALTer: Particle Spectrum for Any Tensor Lagrangian

    Will Barker🇬🇧 · Carlo Marzo🇪🇪 · Claire Rigouzzo🇬🇧

    We present the PSALTer software for efficiently computing the mass and energy of the particle spectrum for any (e.g. higher-rank) tensor field theory in the Wolfram Language. The user must provide a Lagrangian density which is expanded quadratically in the fields around a Minkowski vacuum, is linear in the coupling coefficients, and otherwise built from the partial derivative and Minkowski metric. PSALTer automatically computes the spin-projection operators, saturated propagator, bare masses, residues of massive and massless poles and overall unitarity conditions in terms of the coupling coefficients. The constraints on the source currents and total number of gauge symmetries are produced as a by-product. We provide examples from scalar, vector, tensor and gauge theories of gravity. Each example, including spectra of higher-spin modified gravity theories, may be obtained on a personal computer in a matter of minutes. The software is also parallelised for use on high-performance computing resources. The initial release allows for parity-preserving operators constructed from fields of up to rank three: this functionality will be extended in future versions. PSALTer is a contribution to the xAct project.

    hep-thgr-qchep-phphysics.comp-phPRD(2025)·25 citations
  26. 26*

    Neutrino quantum kinetics in a core-collapse supernova

    Shashank Shalgar🇩🇰 · Irene Tamborra🇩🇰

    Our understanding of neutrino flavor conversion in the supernova core is still preliminary, despite its likely relevance to the neutrino-driven supernova mechanism. We present multi-angle and multi-energy numerical simulations of neutrino quantum kinetics within a spherically symmetric shell in the proximity of the region of neutrino decoupling. We rely on inputs from a one-dimensional core-collapse supernova model with a mass of and find that, at early post-bounce times (~s), no crossing is present in the angular distribution of the electron neutrino lepton number and flavor conversion is triggered by slow collective instabilities. Angular crossings appear for ~s and fast flavor conversion leads to flavor equipartition, with the spectral energy distribution of () and () becoming comparable. Notably, flavor equipartition is not a generic outcome of fast flavor conversion, rather it is a consequence of the relatively similar properties of neutrinos of different flavors characterizing the late accretion phase. Artificially tweaking the collision term to introduce an electron lepton number angular crossing for ~s, we observe that flavor equipartition is not achieved. While our findings are restricted to a specific supernova model, and they only take into account the feedback of the neutrino background on the flavor conversion, they suggest a rich phenomenology in the supernova core as a function of the post-bounce time which needs to be further explored to assess its impact on the explosion mechanism.

    astro-ph.HEhep-phJCAP(2024)·27 citations

* Reconstructed cohort: no mailing for this day survives in the archive. Papers are grouped by their submission times and arXiv's announcement cut-off, assuming announcement without delay; positions follow identifier order. Validated at ~91% exact-day agreement against the archived era.