Evolution of isolated neutron stars: young coolers and old accretors Sergei Popov (SAI) Plan of the talk Magnetic rotator Evolution of neutron stars: rotation ...
Quantum simulations of equilibrium condensed matter systems. 2. Quantum dynamics: ... In cold atoms: start from free Bose gas and slowly turn on interactions. ...
Why do we need transactions to be isolated ? Concurrency problems ... prefer granular locks but will escalate locking level based on available memory resources. ...
... determinations and a linear least square fit using the 68% formal errors in ... Adding these to the linear square fit gives P0 = 8.39107 0.00005 s, dP/dt ...