1,890 research outputs found
Fast opening diaphragm Patent
Magnetically opened diaphragm design with camera shutter and expansion tube application
Thermodynamics of baryonic matter with strangeness within non-relativistic energy density functional model
We study the thermodynamical properties of compressed baryonic matter with
strangeness within non-relativistic energy density functional models with a
particular emphasis on possible phase transitions found earlier for a simple
-mixture. The aim of the paper is twofold: I) examining the
phase structure of the complete system, including the full baryonic octet and
II) testing the sensitivity of the results to the model parameters. We find
that, associated to the onset of the different hyperonic families, up to three
separate strangeness-driven phase transitions may occur. Consequently, a large
fraction of the baryonic density domain is covered by phase coexistence with
potential relevance for (proto)-neutron star evolution. It is shown that the
presence of a phase transition is compatible both with the observational
constraint on the maximal neutron star mass, and with the present experimental
information on hypernuclei. In particular we show that two solar mass neutron
stars are compatible with important hyperon content. Still, the parameter space
is too large to give a definitive conclusion of the possible occurrence of a
strangeness driven phase transition, and further constraints from
multiple-hyperon nuclei and/or hyperon diffusion data are needed.Comment: 11 pages, 7 figure
Modification of magicity towards the dripline and its impact on electron-capture rates for stellar core-collapse
The importance of microphysical inputs from laboratory nuclear experiments
and theoretical nuclear structure calculations in the understanding of the core
collapse dynamics, and the subsequent supernova explosion, is largely
recognized in the recent literature. In this work, we analyze the impact of the
masses of very neutron rich nuclei on the matter composition during collapse,
and the corresponding electron capture rate. To this aim, we introduce an
empirical modification of the popular Duflo-Zuker mass model to account for
possible shell quenching far from stability, and study the effect of the
quenching on the average electron capture rate. We show that the preeminence of
the and closed shells in the collapse dynamics is considerably
decreased if the shell gaps are reduced in the region of Ni and beyond.
As a consequence, local modifications of the overall electron capture rate up
to 30\% can be expected, with integrated values strongly dependent on the
stiffness of magicity quenching and progenitor mass and potential important
consequences on the entropy generation, the neutrino emissivity, and the mass
of the core at bounce. Our work underlines the importance of new experimental
measurements in this region of the nuclear chart, the most crucial information
being the nuclear mass and the Gamow-Teller strength. Reliable microscopic
calculations of the associated elementary rate, in a wide range of temperatures
and electron densities, optimized on these new empirical information, will be
additionally needed to get quantitative predictions of the collapse dynamics.Comment: 12 pages, 10 figure
Particle size distribution of suspended solids in the Chesapeake Bay entrance and adjacent shelf waters
Characteristics of suspended solids, including total suspended matter, total suspended inorganics, total suspended organics, particle size distribution, and the presence of the ten most prominent particle types were determined. Four research vessels simultaneously collected samples along four transects. Samples were collected within a 2-hour period that coincided with the maximum ebb penetration of Chesapeake Bay outwelling. The distribution of primary and secondary particle size modes indicate the presence of a surface or near-surface plume, possibly associated with three sources: (1) runoff, (2) resuspension of material within the Bay, and/or (3) resuspension of material in the area of shoals at the Bay mouth. Additional supportive evidence for this conclusion is illustrated with ocean color scanner data
Hyperons in neutron stars and supernova cores
The properties of compact stars and their formation processes depend on many
physical ingredients. The composition and the thermodynamics of the involved
matter is one of them. We will investigate here uniform strongly interacting
matter at densities and temperatures, where potentially other components than
free nucleons appear such as hyperons, mesons or even quarks. In this paper we
will put the emphasis on two aspects of stellar matter with non-nucleonic
degrees of freedom. First, we will study the phase diagram of baryonic matter
with strangeness, showing that the onset of hyperons, as that of quark matter,
could be related to a very rich phase structure with a large density domain
covered by phase coexistence. Second, we will investigate thermal effects on
the equation of state (EoS), showing that they favor the appearance of
non-nucleonic particles. We will finish by reviewing some recent results on the
impact of non-nucleonic degrees freedom in compact star mergers and
core-collapse events, where thermal effects cannot be neglected.Comment: 20 pages, 14 figures, contribution to the EPJA topical issue "Exotic
matter in neutron stars
Hyperons in neutron star matter within relativistic mean-field models
Since the discovery of neutron stars with masses around 2 solar masses the
composition of matter in the central part of these massive stars has been
intensively discussed. Within this paper we will (re)investigate the question
of the appearance of hyperons. To that end we will perform an extensive
parameter study within relativistic mean field models. We will show that it is
possible to obtain high mass neutron stars (i) with a substantial amount of
hyperons, (ii) radii of 12-13 km for the canonical mass of 1.4 solar masses,
and (iii) a spinodal instability at the onset of hyperons. The results depend
strongly on the interaction in the hyperon-hyperon channels, on which only very
little information is available from terrestrial experiments up to now.Comment: 15 pages, 10 figure
Some aspects of the phase diagram of nuclear matter relevant to compact stars
Dense matter as it can be found in core-collapse supernovae and neutron stars
is expected to exhibit different phase transitions which impact the matter
composition and the equation of state, with important consequences on the
dynamics of core-collapse supernova explosion and on the structure of neutron
stars. In this paper we will address the specific phenomenology of two of such
transitions, namely the crust-core solid-liquid transition at sub-saturation
density, and the possible strange transition at super-saturation density in the
presence of hyperonic degrees of freedom. Concerning the neutron star
crust-core phase transition at zero and finite temperature, it will be shown
that, as a consequence of the presence of long-range Coulomb interactions, a
clusterized phase is expected which is not accessible in the grand-canonical
ensemble. A specific quasi-particle model will be introduced and some
quantitative results relevant for the supernova dynamics will be shown. The
opening of hyperonic degrees of freedom at higher densities corresponding to
the neutron stars core also modifies the equation of state. The general
characteristics and order of phase transitions in this regime will be analyzed
in the framework of a self-consistent mean-field approach.Comment: arXiv admin note: substantial text overlap with arXiv:1206.4924,
arXiv:1301.695
Phase transition towards strange matter
The phase diagram of a system constituted of neutrons and -hyperons
in thermal equilibrium is evaluated in the mean-field approximation. It is
shown that this simple system exhibits a complex phase diagram with first and
second order phase transitions. Due to the generic presence of attractive and
repulsive couplings, the existence of phase transitions involving strangeness
appears independent of the specific interaction model. In addition we will show
under which conditions a phase transition towards strange matter at high
density exists, which is expected to persist even within a complete treatment
including all the different strange and non- strange baryon states. The impact
of this transition on the composition of matter in the inner core of neutron
stars is discussed.Comment: 10 pages, 8 figure
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