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      Quantum Monte Carlo methods for nuclear physics

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          Abstract

          Quantum Monte Carlo methods have proved very valuable to study the structure and reactions of light nuclei and nucleonic matter starting from realistic nuclear interactions and currents. These ab-initio calculations reproduce many low-lying states, moments and transitions in light nuclei, and simultaneously predict many properties of light nuclei and neutron matter over a rather wide range of energy and momenta. We review the nuclear interactions and currents, and describe the continuum Quantum Monte Carlo methods used in nuclear physics. These methods are similar to those used in condensed matter and electronic structure but naturally include spin-isospin, tensor, spin-orbit, and three-body interactions. We present a variety of results including the low-lying spectra of light nuclei, nuclear form factors, and transition matrix elements. We also describe low-energy scattering techniques, studies of the electroweak response of nuclei relevant in electron and neutrino scattering, and the properties of dense nucleonic matter as found in neutron stars. A coherent picture of nuclear structure and dynamics emerges based upon rather simple but realistic interactions and currents.

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          Shapiro delay measurement of a two solar mass neutron star

          Neutron stars are composed of the densest form of matter known to exist in our universe, and thus provide a unique laboratory for exploring the properties of cold matter at super-nuclear density. Measurements of the masses or radii of these objects can strongly constrain the neutron-star matter equation of state, and consequently the interior composition of neutron stars. Neutron stars that are visible as millisecond radio pulsars are especially useful in this respect, as timing observations of the radio pulses provide an extremely precise probe of both the pulsar's motion and the surrounding space-time metric. In particular, for a pulsar in a binary system, detection of the general relativistic Shapiro delay allows us to infer the masses of both the neutron star and its binary companion to high precision. Here we present radio timing observations of the binary millisecond pulsar PSR J1614-2230, which show a strong Shapiro delay signature. The implied pulsar mass of 1.97 +/- 0.04 M_sun is by far the highest yet measured with such certainty, and effectively rules out the presence of hyperons, bosons, or free quarks at densities comparable to the nuclear saturation density.
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            Nuclear charge-density-distribution parameters from elastic electron scattering

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              Bayesian inference and the analytic continuation of imaginary-time quantum Monte Carlo data

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                Author and article information

                Journal
                2014-12-09
                2015-04-29
                Article
                10.1103/RevModPhys.87.1067
                1412.3081
                f574ebfd-469e-484a-b24d-4cabc686a86e

                http://arxiv.org/licenses/nonexclusive-distrib/1.0/

                History
                Custom metadata
                LA-UR-14-29251
                57 pages, 40 figures, accepted for publication in Reviews of Modern Physics
                nucl-th astro-ph.SR cond-mat.quant-gas nucl-ex quant-ph

                Quantum physics & Field theory,Quantum gases & Cold atoms,Nuclear physics,Solar & Stellar astrophysics

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