PaperPanorama

Nuclear Theory·nucl-th

Thursday·November 3, 2022

8 papers5 primary·3 cross-listed

  1. 06

    Faster spectral density calculation using energy moments

    Jeremy Hartse🇺🇸 · Alessandro Roggero🇺🇸

    Accurate predictions of inclusive scattering cross sections in the linear response regime require efficient and controllable methods to calculate the spectral density in a strongly-correlated many-body system. In this work we reformulate the recently proposed Gaussian Integral Transform technique in terms of Fourier moments of the system Hamiltonian which can be computed efficiently on a quantum computer. One of the main advantages of this framework is that it allows for an important reduction of the computational cost by exploiting previous knowledge about the energy moments of the spectral density. For a simple model of medium mass nucleus like Ca and target energy resolution of MeV we find an expected speed-up of times for the calculation of the giant dipole response and of times for the simulation of quasi-elastic electron scattering at typical momentum transfers.

    quant-phnucl-thEPJA(2023)·9 citations
  2. 07

    Determining the Property of Coupling via a Novel Jet Substructure Observable

    Zhite Yu🇺🇸 · Kirtimaan A. Mohan🇺🇸 · C.-P. Yuan🇺🇸

    Determining the property of the Higgs boson is important for a precision test of the Standard Model as well as for the search for new physics. We propose a novel jet substructure observable based on the azimuthal anisotropy in a linearly polarized gluon jet that is produced in association with a Higgs boson at hadron colliders, and demonstrate that it provides a new -odd observable for determining the property of the Higgs-top interaction. We introduce a factorization formalism to define a polarized gluon jet function with the insertion of an infrared-safe azimuthal observable to capture the linear polarization.

    hep-phhep-exhep-latnucl-thPLB(2024)·9 citations
  3. 08

    Effects of electromagnetic fluctuations in plasmas on solar neutrino fluxes

    Eunseok Hwang🇰🇷 · Dukjae Jang🇰🇷 · Kiwan Park🇰🇷 · Motohiko Kusakabe🇨🇳 · Toshitaka Kajino🇨🇳 · A. Baha Balantekin🇺🇸 · Tomoyuki Maruyama🇯🇵 · Youngshin Kwon🇰🇷 · Kyujin Kwak🇰🇷 · Myung-Ki Cheoun🇰🇷

    We explore the effects of electromagnetic (EM) fluctuations in plasmas on solar neutrino fluxes exploiting the fluctuation-dissipation theorem. We find that the EM spectrum in the solar core is enhanced by the EM fluctuations due to the high density of the Sun, which increases the radiation energy density and pressure. By the EM fluctuations involving the modified radiation formula, the central temperature decreases when the central pressure of the Sun is fixed. With a help of the empirical relation between central temperature and neutrino fluxes deduced from the numerical solar models, we present the change in each of the solar neutrino fluxes by the EM fluctuations. We also discuss the enhanced radiation pressure and energy density by the EM fluctuations for other astronomical objects.

    astro-ph.SRastro-ph.HEnucl-thphysics.plasm-ph0 citations

Affiliations

first authorsco-authorsvia INSPIRE