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Stelle di neutroni asimmetriche in rapida rotazione e materia di quark

Stelle di neutroni asimmetriche in rapida rotazione e materia di quark

          
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About the Book

Le stelle di neutroni (NS) sono laboratori astrofisici ideali per testare le teorie sulla materia densa e forniscono connessioni tra astrofisica, fisica nucleare e delle particelle.materia densa e forniscono connessioni tra astrofisica, fisica nucleare e delle particelle. Le recenti scoperte delle pulsar binarie al millisecondo PSR J0952-0607, PSR J0740+6620, PSR J0348+0432 e PSR J1614-2230 suggeriscono che la massa massima Mmax sia compresa tra 2. 35±0.17M⊙, 2.5±0.17M⊙ e 2.5±0.17M⊙.35±0,17M⊙, 2,08 ± 0,07 M⊙, 2,01 ± 0,04 M⊙ e 1,97 ± 0,04 M⊙ rispettivamente, dove M⊙ è la massa solare. Le misure della massa massima influenzano fortemente il comportamento dell'energia di simmetria nucleare vicino alla densità di saturazione nucleare e l'equazione di stato (EdS) ad alta densità a causa dell'esistenza della massa massima. Qui vengono discusse le proprietà delle stelle compatte adroniche pure e ibride utilizzando un'equazione di stato nucleare realistica per la materia β-equilibrata delle stelle di neutroni . Abbiamo utilizzato l'EoS adronica pura e l'EoS combinata con il quark per il nucleo interno ultra-denso per determinare la massa delle NS. È statariscontratauna significativa riduzione della massa massima con l'inclusione del nucleo di quark.


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Product Details
  • ISBN-13: 9786207434343
  • Publisher: KS Omniscriptum Publishing
  • Publisher Imprint: Edizioni Sapienza
  • Height: 229 mm
  • No of Pages: 100
  • Spine Width: 6 mm
  • Width: 152 mm
  • ISBN-10: 620743434X
  • Publisher Date: 25 Apr 2024
  • Binding: Paperback
  • Language: Italian
  • Returnable: N
  • Weight: 159 gr

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