The latter transition may be induced by a relatively small change in compound composition (cf. the behavior of La2 − xSrxO4 or YBa2Cu3O7 − x as a function of x). It is quite interesting to note that oxides such as YBa2Cu3O7 − x may be synthesized in either insulating (x ...
Now, the EoS of matter in the interior of NSs and its importance is still an open challenge in research of particle physics as well as stellar astrophysics. The interior structure and composition mainly depend on the nature and interaction of different type matters, presented as mixture in the...
Pion Production Via Resonance Decay in a Non-extensive Quark-Gluon Medium with Non-additive Energy Composition Ruledoi:10.1051/EPJCONF/20111305003Karoly UrmossyTamas S. BiroGergely G. BarnafldiarXiv: High Energy Physics - Phenomenology
For resonances, X˜ i is still related to the squared wave function of the channel i, in a phase prescription that automatically renders the wave function real for bound states, and so it can be used as a measure of the weight of that meson-baryon channel in the composition of the ...
the effect of such a mech- anism on the hadrochemical composition of the produced particles? Fortunately, the answer to this theoretical question is positive, provided that hadron pro- duction is characterized by the sudden recombi- nation of constituent quarks into hadrons, as de- scribed by...
Pion Production Via Resonance Decay in a Non-extensive Quark-Gluon Medium with Non-additive Energy Composition Ruledoi:10.1051/EPJCONF/20111305003K. UrmossyT.S. BiroG.G. BarnafldiEDP SciencesInternational Workshop on Hot and Cold Baryonic Matter, HCBM 2010...
. This uncertainty is not included for tt + tW since the non-prompt-lepton contributions in CRs and SRs have the same composition and are fully dominated by semileptonic b-decays. Background rate uncertainty. For ttZ and tWZ productions, a cross-section uncer- tainty of 12% is used [73...
This parameter depends on the microphysical properties of the matter composition of the star and it is a measure of the influence of a star’s internal structure on the waveform. Effects on this quantity related to the appearance of quark matter in the inner cores of compact stars have been ...
The atmospheric composition can be approximated considering only molecular nitrogen, which represents nearly 78% of the atmospheric concentration, and oxygen, accounting for 21%. Molecular nitrogen has a triple bond between the two atoms, one sigma bond, and two pi bonds. This bond is very strong...
range of densities, starting from the density of ordinary matter of atomic-molecular composition to values tens of times higher than the nuclear density at which various exotic structures can appear, such as the pion condensate, kaon condensate, deconfined quark phase, and color superconducting ...