Properties of nucleons in dense/hot nuclear matter

As everyone knows, nucleons are compound objects with some size and some ma­ss. Results of investigation on change of their properties in nuclear matter at 0K equilibrium and in a dense hadron matter inside neutron stars will be presented. Change of nucleon structure function in nuclear ma­tte­r present inside heavy atom nuclei will be discussed first. Simple model can explain how the properties change under the influence of hadron matter pressure. Finally, a possible mo­dification of sta­tistics around phase transition of hot nuclear matter into quark-gluon matter will be discussed.

All interested prsons are invited
M. Ko­wal, W. Pie­choc­ki, L. Rosz­kow­ski, J. Skal­ski