Magnito- Gidrodinamicheskie Protsessy V Neytronnykh Zvezdakh

Veshchestvo neytronnykh zvezd predstavlyaet soboysverkhplotnuyu, bystro vrashchayushchuyusya mnogokomponentnuyuplazmu, analogov kotoroy v laboratornykh usloviyakh nesushchestvuet. Magnitnye polya, nablyudaemye u neytronnykhzvezd, yavlyayutsya samymi sil'nymi iz izvestnykh vprirode. Sil'nye magnitnye polya igrayut osnovnuyu rol'v nablyudatel'nykh proyavleniyakh etikh ob"ektov. Polyavliyayut na ikh teplovuyu evolyutsiyu i na kinetmcheskiesvoystva plazmy, opredelyayut svoystva poverkhnosti ikharakter razlichnykh nestatsionarnykh yavleniy. Poetomuproblema proiskhozhdeniya sverkhsil'nykh magnitnykh poley,ikh struktura i evolyutsiya na raznykh etapakh zhizniyavlyaetsya odnoy iz tsentral'nykh dlya astrofizikineytronnykh zvezd i, v bolee obshchem plane, dlya fizikiekstremal'nogo sostoyaniya veshchestva. V dannoy raboterassmotren shirokiy krug voprosov, otnosyashchikhsya kmagnitnoy gidrodinamike neytronnykh zvezd. Osnovnoevnimanie udeleno MGD ustoychivosti etikh ob"ektov iproiskhozhdeniyu ikh magnitnykh poley. Takzhe detal'noissleduetsya magnitnaya i vrashchatel'naya evolyutsiyaneytronnykh zvezd, nakhodyashchikhsya v razlichnykh usloviyakh.Kniga raschitana na nauchnykh rabotnikov i studentovfizicheskikh spetsial'nostey, a takzhe na vsekh chitateley,interesuyushchikhsya sovremennoy astrofizikoy.