3148 papers
Hep-Th, or high-energy theoretical physics, explores the fundamental building blocks of our universe and the forces that govern them. Researchers in this field use complex mathematics to understand everything from subatomic particles to the behavior of black holes, often pushing the boundaries of what we know about space and time.
At Gist.Science, we monitor the arXiv repository to ensure you stay ahead of the curve in this rapidly evolving discipline. For every new preprint uploaded to arXiv under this category, our team generates both accessible plain-language overviews and detailed technical summaries, making cutting-edge research understandable regardless of your background.
Below are the latest papers in high-energy theoretical physics, curated to help you navigate the most significant recent discoveries.
This paper presents a singularity-free de Broglie–Bohm quantum bounce cosmology that is strongly compatible with Planck 2018 CMB data, places a stringent upper bound on the bounce scale, and offers a potential mechanism to mitigate the - tension through a unique scale-dependent anticorrelation.
This paper presents a systematic framework for constructing (3+1)-dimensional fermionic topological quantum field theories that realize specified finite symmetry anomalies by translating supercohomology data into fusion 2-categories, ultimately proving that all supercohomology anomalies are realizable while beyond-supercohomology anomalies are not.
This article provides a comprehensive overview of gravitational waves, tracing their theoretical origins in general relativity and historical prediction to their experimental confirmation via interferometers like LIGO and Virgo, while analyzing their emission mechanisms, detection milestones such as GW150914, and their transformative role in multi-messenger astronomy.
By computing the Wigner function of inflationary curvature perturbations using the EFT of inflation, this paper demonstrates that primordial non-Gaussianities generate persistent quantum interference fringes and growing Wigner negativity on super-Hubble scales, proving that squeezing alone is insufficient to ensure classicality and suggesting that genuinely quantum signatures of the universe's origins may be detectable.
This paper proposes and validates a UV completion for gauge theory via a 6d SCFT by demonstrating consistency through 6d anomaly cancellation, 5d Coulomb branch prepotentials, and a modular bootstrap calculation of the elliptic genus that matches the vacuum character of the corresponding vertex operator algebra.
This paper introduces new rotating, asymptotically flat black hole solutions in string theory with linear dilaton vacua and mass-independent temperatures, demonstrating their derivation from the large- limit of Myers-Perry black holes and highlighting their unique thermodynamic properties and restricted asymptotic symmetry groups.
This paper improves the upper bound on the number of diffeomorphism classes of Calabi-Yau threefolds arising from Batyrev's construction to by analyzing 2-face equivalence classes of FRSTs for reflexive polytopes with , while also establishing a lower bound of on these equivalence classes.
This paper presents a convolutional neural network trained on improved Gaussian data to reconstruct spectral densities from imaginary-time Green's functions, demonstrating that while it outperforms the standard Maximum Entropy method on data similar to its training set, the latter remains superior for identifying physical features in complex models like the 1d Hubbard and 2d SSH systems.
This paper proposes a viable glueball dark matter candidate arising from a confined Yang-Mills sector coupled to the Standard Model via vector-like fermion portals, developing a non-perturbative effective field theory framework that predicts a steeply scaling spin-independent scattering cross-section () within the sensitivity reach of current and next-generation xenon direct-detection experiments.
This paper investigates two specific gravity models with and , demonstrating through observational data analysis and parameter constraints that they successfully reproduce the Universe's transition from deceleration to late-time acceleration while remaining consistent with the standard CDM model and satisfying key energy conditions.