QUARK MATTER IN NEUTRON STARS

The models describing SIDIS on nuclei are based on the following processes: hadron absorption, parton energy loss and medium modified fragmentation functions.. Hadron absorption

This time dependence, well reproduced by the Lund model [Gallmeister 2005] (see figure 3.2 ), is due to the gluon emission during the vacuum fragmentation. In order to produce a

However, as we will develop in the next chapter, finite temperature nuclear matter as it is formed in supernova explosions and the cooling of proto-neutron stars is in

In this contribution, we will limit ourselves to the thermodynamic conditions where matter can be described by nucleonic or hadronic degrees of freedom and will examine two

In order to estimate the spurious shell effects due to the unbound neutrons, we simulate an homogeneous gas of neutron matter in W-S cell by removing all the proton states.

L’archive ouverte pluridisciplinaire HAL, est destinée au dépôt et à la diffusion de documents scientifiques de niveau recherche, publiés ou non, émanant des

In this contribution, we will present some experimental results concerning the transport proper- ties of nuclear matter, focusing specifically on the determination of

In a spinodal de- composition scenario, cluster properties as sizes and chemical compositions can be predicted from the characteristics of the most unstable mode at the onset