PaperPanorama

Nuclear Theory·nucl-th

Friday·January 24, 2020

17 papers10 primary·7 cross-listed

  1. 11

    Computation of effective front form Hamiltonians for massive Abelian gauge theory

    Stanislaw D. Glazek🇵🇱

    Renormalization group procedure for effective particles (RGPEP) is applied in terms of a second-order perturbative computation to an Abelian gauge theory, as an example of application worth studying on the way toward derivation of a dynamical connection between the spectroscopy of bound states and their parton-model picture in the front form of Hamiltonian dynamics. In addition to the ultraviolet transverse divergences that are handled using the RGPEP in previously known ways, the small-x divergences are handled by introducing a mass parameter and a third polarization state for gauge bosons using a mechanism analogous to spontaneous breaking of global gauge symmetry, in a special limit that simplifies the theory to Soper's front form of massive QED. The resulting orders of magnitude of scales involved in the dynamics of effective constituents or partons in the simplified theory are identified for the fermion and boson mass counter terms, effective masses and self-interactions, as well as for the Coulomb-like effective interactions in bound states of fermions. Computations in orders higher than second are mentioned but not described in this article.

    hep-thnucl-thPRD(2020)·7 citations
  2. 12

    Gradient Tomography of Jet Quenching in Heavy-Ion Collisions

    Yayun He🇨🇳 · Long-Gang Pang🇨🇳 · Xin-Nian Wang🇨🇳

    Transverse momentum broadening and energy loss of a propagating parton are dictated by the space-time profile of the jet transport coefficient in a dense QCD medium. The spatial gradient of perpendicular to the propagation direction can lead to a drift and asymmetry in parton transverse momentum distribution. Such an asymmetry depends on both the spatial position along the transverse gradient and path length of a propagating parton as shown by numerical solutions of the Boltzmann transport in the simplified form of a drift-diffusion equation. In high-energy heavy-ion collisions, this asymmetry with respect to a plane defined by the beam and trigger particle (photon, hadron or jet) with a given orientation relative to the event plane is shown to be closely related to the transverse position of the initial jet production in full event-by-event simulations within the linear Boltzmann transport model. Such a gradient tomography can be used to localize the initial jet production position for more detailed study of jet quenching and properties of the quark-gluon plasma along a given propagation path in heavy-ion collisions.

    hep-phnucl-thPRL(2020)·55 citations
  3. 13

    Gauge boson mass as regulator

    Stanislaw D. Glazek🇵🇱

    Small-x divergences of Abelian gauge theory in the front form of Hamiltonian dynamics are regulated using a mass parameter for gauge bosons, introduced through a mechanism analogous to the spontaneous breaking of global gauge symmetry. A corresponding family of ultraviolet and infrared finite scale-dependent renormalized Hamiltonians, is calculable order-by-order using the renormalization group procedure for effective particles. The second-order terms described here suggest the magnitude of mass corrections that may be involved in resolving the small-x parton and front-form vacuum and zero-mode problems, assuming that the gauge boson mass that counts does not exceed the current upper bound on the photon mass.

    hep-thnucl-thPoS(2020)·0 citations
  4. 14

    Constraining the Ne(,)Mg and Ne(,n)Mg reaction rates using sub-Coulomb -transfer reactions

    H. Jayatissa · G.V. Rogachev · V.Z. Goldberg · E. Koshchiy · G. Christian · J. Hooker · S. Ota · B.T. Roeder · A. Saastamoinen · O. Trippella · S. Upadhyayula · E. Uberseder

    The Ne(,)Mg and Ne(,n)Mg reactions play an important role in astrophysics because they have significant influence on the neutron flux during the weak branch of the s-process. We constrain the astrophysical rates for these reactions by measuring partial -widths of resonances in Mg located in the Gamow window for the Ne+ capture. These resonances were populated using Ne(Li,d)Mg and Ne(Li,t)Mg reactions at energies near the Coulomb barrier. At these low energies -transfer reactions favor population of low spin states and the extracted partial -widths for the observed resonances exhibit only minor dependence on the model parameters. The astrophysical rates for both the Ne(,)Mg and the Ne(,n)Mg reactions are shown to be significantly different than the previously suggested values.

    nucl-exastro-ph.SRnucl-thPLB(2020)·28 citations
  5. 15

    An approach to constrain models of accreting neutron stars with the use of an equation of state

    Akira Dohi · Masa-aki Hashimoto · Rio Yamada · Yasuhide Matsuo · Masayuki Fujimoto

    We investigate X-ray bursts during the thermal evolution of an accreting neutron star which corresponds to the X-ray burster GS\ 1826-24. Physical quantities of the neutron star are included using an equation of state below and above the nuclear matter density. We adopt an equation of state and construct an approximate network that saves the computational time and calculates nuclear energy generation rates accompanying the abundance evolutions. The mass and radius of the neutron star are got by solving the stellar evolution equations from the center to the surface which involve necessary information such as the nuclear energy generation in accreting layers, heating from the crust, and neutrino emissions inside the stellar core. We reproduce the light curve and recurrence time of the X-ray burst from GS 1826-24 within the standard deviation of 1 for the assumed accretion rate, metallicity, and equation of state. It is concluded that the observed recurrence time is consistent with the theoretical model having metallicity of the initial CNO elements = 0.01. We suggest that the nuclear reaction rates responsible for the -process should be examined in detail, because the rates may change the shape of the light curve and our conclusion.

    astro-ph.SRastro-ph.HEnucl-thPTEP(2020)·19 citations
  6. 16

    On lower bound of relaxation time for massless fluid in presence of magnetic field

    Sarthak Satapathy🇮🇳 · Jayanta Dey🇮🇳 · Prashant Murmu🇮🇳 · Sabyasachi Ghosh🇮🇳

    Due to lowest possible quantum fluctuation, shear viscosity to entropy density ratio never reach to zero, rather has some lower bound (0.08 approx). Here, we have attempted to link our calculation, based on relaxation time approximation for massless relativistic fluid, with that value and interestingly found a lower and also an upper limit of relaxation time.

    hep-phnucl-thDAE Symp.Nucl.Phys.(2019)·0 citations
  7. 17

    Strong decays of strange quarkonia in a corrected 3P0 model

    J. N. de Quadros🇧🇷 · D. T. da Silva🇧🇷 · M. L. L. da Silva🇧🇷 · D. Hadjimichef🇧🇷

    Extensively applied to both light and heavy meson decay and standing as one of the most successful strong decay models is the model, in which pair production is the dominant mechanism. In this paper we evaluate strong decay amplitudes and partial widths of strange and state mesons, namely , , , , and , in the bound-state corrected decay model (C). The C model is obtained in the context of the Fock-Tani formalism, which is a mapping technique.

    hep-phnucl-thPRC(2020)·6 citations

Affiliations

first authorsco-authorsvia INSPIRE