496 papers
This paper utilizes the QCD functional formalism to extract quark spectral functions by solving coupled Dyson-Schwinger and Bethe-Salpeter equations under the ladder-rainbow approximation, with results validated against the masses and decays of pseudoscalar mesons like the pion and to demonstrate the significance of dynamical charm mass variations and the nature of confinement.
This paper analyzes Planck and SPT-3G 2018 data to search for super-imposed oscillations in the primordial power spectrum, finding that combined datasets provide tighter constraints on oscillation amplitudes and reveal improved fits with significant statistical gains compared to individual datasets.
This paper demonstrates that thin accretion disks surrounding black holes can induce significant tidal Love numbers that may obscure modified gravity effects and limit tests of black-hole mimickers, while also showing that next-generation gravitational wave detectors like LISA and the Einstein Telescope could precisely measure these environmental parameters.
This paper translates current bounds on axion-like particle (ALP) photon couplings into constraints on the size of the extra dimension within the Randall-Sundrum model, demonstrating that these limits fail to resolve the gauge hierarchy problem for light ALPs and instead necessitate a massive ALP ( GeV) to be relevant.
This paper demonstrates that parton shower event generators offer a more accurate description of dilepton spectra from photon conversion in heavy-ion collisions compared to the traditional Kroll-Wada approach, particularly at larger invariant masses where they better account for phase-space suppression, recoil kinematics, and higher-order corrections.
This paper presents a phenomenological study of the symmetric Type-Z Three Higgs Doublet Model at a 1000 GeV International Linear Collider, demonstrating that specific production channels involving heavier Higgs bosons offer promising opportunities to discover new physics beyond the Standard Model.
This paper proposes a SM model based on an extension of the Standard Model that simultaneously explains the observed dark matter relic abundance through freeze-in production of a singlet fermion and the baryon asymmetry via leptogenesis, while also generating light neutrino masses through the type-I seesaw mechanism.
By unifying 104 localized fast radio bursts and 47 gravitational-wave events, this study presents an -free measurement of the cosmic baryon density fraction () that aligns with early-Universe observations and offers a robust late-Universe probe to address the tension and missing baryon problem.
This paper investigates whether small dark matter clumps passing near Earth could generate the gravitational-wave glitches observed in LIGO/Virgo/KAGRA data, finding that while most glitches are inconsistent with this hypothesis, the analysis establishes the first direct upper limits on the local over-density of such dark matter clumps.
This paper proposes that the Cherenkov Telescope Array (CTA) can detect gamma-ray signatures from strangelets potentially emitted by the exotic strange quark star candidate HESS J1731-347, thereby validating the existence of strange quark matter and its role in cosmic-ray acceleration.
This paper establishes exact analytical boundaries and efficient computational procedures for determining the necessary and sufficient bounded-from-below conditions of scalar potentials in Standard Model extensions featuring an quadruplet of scalars, significantly reducing the required computational time by scanning specific lines rather than surfaces.
This paper proposes that local spin polarization of quarks, induced by color-field correlators arising from the interplay of chromo-Lorentz force, chromo-magnetic polarization, and momentum anisotropy in glasma or quark-gluon plasma, generates a longitudinal polarization spectrum for hyperons with a characteristic sinusoidal structure that aligns with experimental observations in relativistic heavy ion collisions.
This paper proposes a Kullback-Leibler divergence-based methodology to quantify differences between nuclear and free nucleon parton distribution functions, successfully modeling the EMC effect for quarks and revealing that the EPPS21 gluon nPDFs align more closely with the "minimum relative entropy" hypothesis than nNNPDF3.0, thereby offering a novel tool for future global fits in data-scarce regimes.
This paper systematically investigates the mass spectra and decay channels of fully heavy tetraquark states using a diquark-antidiquark model, concluding that while , , and are unlikely to be $1SX(6200)2^{++}$ state and predicting several narrow states for future experimental observation.
This paper investigates how future space-borne gravitational wave detectors can test the B-L gauge extension of the Standard Model by distinguishing between Dirac and Majorana thermal Leptogenesis scenarios through the stochastic background generated by cosmic strings, with the former being probeable up to $10^910^{12}$ GeV.
This paper utilizes a semi-analytical model of galaxy and supermassive black hole evolution within the CDM paradigm to demonstrate that the observed stellar mass–black hole mass relation at high redshifts disfavours fuzzy dark matter fields with masses below $2.0\times 10^{-20}$ eV and warm dark matter particles with masses below 7.2 keV at the 95% confidence level.
This paper derives vorticity-induced effects on Nambu-Goldstone modes in chiral perturbation theory by treating vorticity as an axial-vector field within the Wess-Zumino-Witten framework, resulting in new contributions such as vorticity-induced currents, magnetic-field-induced angular momentum, and modified photon-pion couplings in the presence of electromagnetic fields and finite chemical potentials.
This paper demonstrates that a transformer model can efficiently predict the energy evolution of the dipole amplitude governed by the Balitsky-Kovchegov equation, enabling rapid fitting of its initial condition to HERA deep inelastic scattering data and revealing that a smaller starting evolution point yields better agreement with experimental results.
This paper demonstrates that embedding natural inflation within Palatini gravity, specifically with the model where $7/4 \lesssim n \leq 2n > 2$ fail to provide comparable improvements.
Using dispersion theory to account for strong pion-pion final-state interactions, this study demonstrates that the substructure near the threshold in decays can be reproduced without invoking an extra resonance, attributing the observed dip primarily to a helicity-flip amplitude rather than the virtual exchange of the state.