scholarly journals The role of Lattice QCD in flavor physics

2005 ◽  
Vol 140 ◽  
pp. 48-57 ◽  
Author(s):  
V. Lubicz
Keyword(s):  
2012 ◽  
Vol 13 (2) ◽  
pp. 121-126 ◽  
Author(s):  
Damir Bečirević ◽  
Vittorio Lubicz
Keyword(s):  

2012 ◽  
Author(s):  
Hiroshi Ueda ◽  
Takahiro M Doi ◽  
Sho Fujibayashi ◽  
Shoichiro Tsutsui ◽  
Takumi Iritani ◽  
...  
Keyword(s):  

2018 ◽  
Vol 171 ◽  
pp. 14006
Author(s):  
Volodymyr Vovchenko ◽  
Paolo Alba ◽  
Mark I. Gorenstein ◽  
Horst Stoecker

The quantum van der Waals (QvdW) extension of the ideal hadron resonance gas (HRG) model which includes the attractive and repulsive interactions between baryons – the QvdW-HRG model – is applied to study the behavior of the baryon number related susceptibilities in the crossover temperature region. Inclusion of the QvdW interactions leads to a qualitatively different behavior of susceptibilities, in many cases resembling lattice QCD simulations. It is shown that for some observables, in particular for χBQ11/χB2, effects of the QvdW interactions essentially cancel out. It is found that the inclusion of the finite resonance widths leads to an improved description of χB2, but it also leads to a worse description of χBQ11/χB2, as compared to the lattice data. On the other hand, inclusion of the extra, unconfirmed baryons into the hadron list leads to a simultaneous improvement in the description of both observables.


2013 ◽  
Author(s):  
Hiroshi Ueda ◽  
Takahiro M Doi ◽  
Sho Fujibayashi ◽  
Shoichiro Tsutsui ◽  
Takumi Iritani ◽  
...  
Keyword(s):  

2021 ◽  
Vol 81 (1) ◽  
Author(s):  
P. Jakobus ◽  
A. Motornenko ◽  
R. O. Gomes ◽  
J. Steinheimer ◽  
H. Stoecker

AbstractThe properties of compact stars and in particular the existence of twin star solutions are investigated within an effective model that is constrained by lattice QCD thermodynamics. The model is modified at large baryon densities to incorporate a large variety of scenarios of first order phase transitions to a phase of deconfined quarks. This is achieved by matching two different variants of the bag model equation of state, in order to estimate the role of the Bag model parameters on the appearance of a second family of neutron stars. The produced sequences of neutron stars are compared with modern constrains on stellar masses, radii, and tidal deformability from astrophysical observations and gravitational wave analyses. It is found that those scenarios in our analysis, in which a third family of stars appeared due to the deconfinement transition, are disfavored from astrophysical constraints.


2019 ◽  
Vol 55 (11) ◽  
Author(s):  
Christoph Lehner ◽  
◽  
Stefan Meinel ◽  
Tom Blum ◽  
Norman H. Christ ◽  
...  

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