Phases of dense matter in neuron stars

Recent equations of state for dense nuclear matter are discussed with possi ble phase transitions arising in neutron stars such as pion, kaon and hyper on condensation, superfluidity and quark matter. Specifically, we treat the nuclear to quark matter phase transition, the possible mixed phase and its structure. A number of numerical calculations of rotating neutron stars wi th and without phase transitions are given and compared to observed masses, radii, temperatures and glitches. (C) 2000 Elsevier Science B.V. All right s reserved.