PaperPanorama

Nuclear Theory·nucl-th

Tuesday·August 15, 2017

11 papers8 primary·3 cross-listed

  1. 09

    Revisiting the Hybrid Quantum Monte Carlo Method for Hubbard and Electron-Phonon Models

    Stefan Beyl · Florian Goth · Fakher F. Assaad

    A unique feature of the hybrid quantum Monte Carlo (HQMC) method is the potential to simulate negative sign free lattice fermion models with subcubic scaling in system size. Here we will revisit the algorithm for various models. We will show that for the Hubbard model the HQMC suffers from ergodicity issues and unbounded forces in the effective action. Solutions to these issues can be found in terms of a complexification of the auxiliary fields. This implementation of the HQMC that does not attempt to regularize the fermionic matrix so as to circumvent the aforementioned singularities does not outperform single spin flip determinantal methods with cubic scaling. On the other hand we will argue that there is a set of models for which the HQMC is very efficient. This class is characterized by effective actions free of singularities. Using the Majorana representation, we show that models such as the Su-Schrieffer-Heeger Hamiltonian at half filling and on a bipartite lattice belong to this class. For this specific model sub-cubic scaling is achieved.

    cond-mat.str-elhep-latnucl-thPRB(2018)·65 citations
  2. 10

    Probing mass-radius relation of protoneutron stars from gravitational-wave asteroseismology

    Hajime Sotani🇯🇵 · Takami Kuroda🇨🇭 · Tomoya Takiwaki🇯🇵 · Kei Kotake🇯🇵

    The gravitational-wave (GW) asteroseismology is a powerful technique for extracting interior information of compact objects. In this work, we focus on spacetime modes, the so-called -modes, of GWs emitted from a proto-neutron star (PNS) in the postbounce phase of core-collapse supernovae. Using results from recent three-dimensional supernova models, we study how to infer the properties of the PNS based on a quasi-normal mode analysis in the context of the GW asteroseismology. We find that the -mode frequency multiplied by the PNS radius is expressed as a linear function with respect to the ratio of the PNS mass to the PNS radius. This relation is insensitive to the nuclear equation of state (EOS) employed in this work. Combining with another universal relation of the -mode oscillations, we point out that the time dependent mass-radius relation of the PNS can be obtained by observing both the - and -mode GWs simultaneously. Our results suggest that the simultaneous detection of the two modes could provide a new probe into finite-temperature nuclear EOS that predominantly determines the PNS evolution.

    astro-ph.HEnucl-thPRD(2017)·66 citations
  3. 11

    Strangeon Matter in a Liquid Drop Model

    Zheng Wang🇨🇳 · Jiguang Lu🇨🇳 · Renxin Xu🇨🇳

    The liquid drop model of 2-flavored ( and ) nucleus is well known and successful, analogically, a similar drop model for 3-flavored (, and ) nucleus is developed. A 3-flavored nucleus conjectured could be stable only if its baryon number is lager than a critical one, , in which strangeons are the constituent as an analogy of nucleons for nucleus. We try to model strangeon matter in a sense of phenomenological liquid drop, with two free parameters: the mass per bayron of a strangeon in vacuum, , and potential deep between strangeons, . It is found that, for GeV and MeV, strangeon matter could be stable and its critical number could be as low as .

    astro-ph.HEnucl-thJPS Conf.Proc.(2018)·1 citation

Affiliations

first authorsco-authorsvia INSPIRE