Warm dense matter
Ion structure in warm dense matter: benchmarking solutions of hypernetted chain equations by first principle simulations
... of warm dense matter (WDM) provide the basis for a general understanding of such diverse systems as giant gas planets [1, 2], laser-heated solids and imploding capsules of hydrogen during inertial ...
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Dynamic ion structure factor of warm dense matter
... and warm dense matter (WDM) is of great importance as it contains the complete information on the ions in these strongly interacting systems and is also influenced by the electron ...of matter ...
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Low frequency structural dynamics of warm dense matter
... of warm dense matter pose severe challenges since WDM spans the intermediate states between solids and plasmas and retains properties common to ...
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Theory of x ray Thomson scattering in warm dense matter
... to dense matter with high energy density has significantly changed over the last ...of matter that naturally only occur in stars or large ...compress matter up to a few hundred times solid or ...
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Guiding of relativistic electron beams in dense matter by laser-driven magnetostatic fields
... denser matter is a major chal- lenge for improving laser-driven sources of energetic particles and radiation 1–3 , or for driving matter to temperatures relevant to the study of structural and dynamic ...
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A reduced coupled mode description for the electron ion energy relaxation in dense matter
... modes exist. In the following, we want to discuss three different systems with very different ionic mode structures: i) a weakly coupled ion subsystem (gas-like plasma); ii) WDM with ions that form a strongly coupled ...
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Enhanced relativistic-electron-beam energy loss in warm dense aluminum
... in warm-compressed aluminum (Al) samples of identical areal density ...the warm dense matter state [15]. The Al warm samples, obtained by ns laser- generated planar shock-compression, ...
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Laboratory measurements of resistivity in warm dense plasmas relevant to the microphysics of brown dwarfs
... a warm, dense matter in the ...creating matter in states like those believed to occur in brown dwarf stars and larger exoplanets 1 ...in dense plasmas, and at the centre of a brown ...
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Probing the dynamic response of dense matter with x ray Thomson scattering
... • For partially ionized plasmas, it was shown that the DSF can be decomposed to recover the well-known expression of Chihara. The multicomponent generalisation of this model was adopted as the basic framework in order to ...
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Laboratory measurements of resistivity in warm dense plasmas relevant to the microphysics of brown dwarfs
... In ultra-intense laser-plasma interactions, beams of relativistic ‘hot’ electrons are driven from the interaction region 6 into materials of much higher density. Anisotropies in the speed distributions of both hot and ...
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Towards Dense Nuclear Matter in A Modified Sakai-Sugimoto Model
... Abstract. As a part of the attempt to address dense baryonic matter, we first review holographic approaches to QCD. The big advantage of the holographic approaches is that they render strongly coupled 4D ...
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What can neutron stars reveal about the equation of state of dense matter?
... To extract reliable constraints from NS observations, it is necessary to use EOS with reliable uncer- tainties at low densities and model-agnostic extensions to higher densities to reduce systematic errors. Together with ...
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Nuclear phase transition and thermodynamic instabilities in dense nuclear matter
... nucleonic matter to ∆-excited nuclear matter can take place and the occurrence of this transition sensibly depends on the ∆-meson coupling constants [11, ...
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Dense and hot matter in compact stars and heavy-ion collisions
... Abstract. We discuss the effect of exotic particles in neutron star matter and the cor- responding impact on gross properties of neutron stars within effective models for the strong interaction. Particularly, for ...
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ALMA Observations of Warm Dense Gas in NGC 1614{__Breaking of the Star Formation Law in the Central Kiloparsec
... In Figure 9, we compare the spectral line energy distributions (SLEDs) of the total CO emission (measured by single-dish observations) of these two galaxies, taken from observations of Herschel-SPIRE FTS observations (N. ...
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Dense quark matter with chiral and isospin imbalance: NJL-model consideration
... asymmetric quark matter. Also, we have investigated discrete symmetry (dual- ity) between chiral and pion condensates in the case of massless quarks, which stay relatively instructive even if the quarks have bare ...
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Effective equation of state of hot and dense matter in nuclear collisions around FAIR energy
... and 160 AGeV, respectively. These reactions can probe the domain of temperatures and baryon chem- ical potentials where, according to the lattice QCD calculations, the tricritical point of nuclear phase diagram is ...
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Skyrme-RPA study of charged-current neutrino opacity in hot and dense supernova matter
... ing factor for the outgoing lepton. In the protoneutron star matter positrons are nondegenerate and their spectrum ap- proaches the Boltzmann distribution. Therefore, we can neglect the final-state blocking for ...
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Parallel Algorithm for Solving TOV Equations for Sequence of Cold and Dense Nuclear Matter Models
... We have introduced the algorithm solving TOV equations for set of EoS models, which is parallelized on the level of different models. Such algorithm is important for investigation of models of cold and dense ...
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Probing properties of hot and dense QCD matter with heavy flavor in the PHENIX experiment at RHIC
... Abstract. Hadrons carrying heavy quarks, i.e. charm or bottom, are important probes of the hot and dense medium created in relativistic heavy ion collisions. Heavy quark- antiquark pairs are mainly produced in ...
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