We calculate the thermal and dynamical evolution of the surface layers of anaccreting neutron star during the rise of a superburst. For the first few hoursfollowing unstable 12C ignition, the nuclear energy release is transported byconvection. However, as the base temperature rises, the heating time becomesshorter than the eddy turnover time and convection becomes inefficient. Thisresults in a hydrodynamic nuclear runaway, in which the heating time becomesshorter than the local dynamical time. Such hydrodynamic burning can driveshock waves into the surrounding layers and may be the trigger for the normalX-ray burst found to immediately precede the onset of the superburst in bothcases where the Rossi X-Ray Timing Explorer was observing.
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机译:用等离子体约束实现重力场的动态控制热核聚变(TLTS)方法,通过热辐射等离子体绝缘的壁反应堆防止中子辐射并节省磁场和等离子体的混合,使用旋转磁场的异步磁惯性约束反应堆(AMITYAR和HFM)为实施该方法,在该反应器中点燃热核反应的方法,爆炸式等离子发生器(VIP)的实施方法,以及具有HFM的特立普安瓿,以实现D + T反应和具有超高温热度的HFM D +3НЕ和1Н+11В的高温反应