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LAP Lambert Academic Publishing Магнито- гидродинамические процессы в нейтронных звездах: Сверхсильные магнитные поля: происхождение и эволюция: Swerhsil'nye magnitnye polq: proishozhdenie i äwolüciq

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£67.00 £63.65 £64.99 £66.33 £67.67 £69.01 £70.35 11 August 2026 16 August 2026 22 August 2026 27 August 2026 02 September 2026
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23 days 0 6 12 17 23 £67 Days at Price

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Most common price: £67 (23 days, 100.0%)

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Description

Вещество нейтронных звезд представляет собойсверхплотную, быстро вращающуюся многокомпонентнуюплазму, аналогов которой в лабораторных условиях несуществует. Магнитные поля, наблюдаемые у нейтронныхзвезд, являются самыми сильными из известных вприроде. Сильные магнитные поля играют основную рольв наблюдательных проявлениях этих объектов. Полявлияют на их тепловую эволюцию и на кинетмческиесвойства плазмы, определяют свойства поверхности ихарактер различных нестационарных явлений. Поэтомупроблема происхождения сверхсильных магнитных полей,их структура и эволюция на разных этапах жизниявляется одной из центральных для астрофизикинейтронных звезд и, в более общем плане, для физикиэкстремального состояния вещества. В данной работерассмотрен широкий круг вопросов, относящихся кмагнитной гидродинамике нейтронных звезд. Основноевнимание уделено МГД устойчивости этих объектов ипроисхождению их магнитных полей. Также детальноисследуется магнитная и вращательная эволюциянейтронных звезд, находящихся в различных условиях.Книга расчитана на научных работников и студентовфизических специальностей, а также на всех читателей,интересующихся современной астрофизикой.

Product Specifications

Format
paperback
Domain
Amazon UK
Release Date
30 June 2011
Listed Since
29 January 2013

Barcode

No barcode data available

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