메뉴 건너뛰기




Volumn 8, Issue S291, 2012, Pages 73-76

How free are free neutrons in neutron-star crusts and what does it imply for pulsar glitches?

Author keywords

(stars:) pulsars: general; dense matter; equation of state; gravitation; hydrodynamics; stars: neutron; stars: rotation; stellar dynamics

Indexed keywords


EID: 84876583194     PISSN: 17439213     EISSN: 17439221     Source Type: Book Series    
DOI: 10.1017/S1743921312023198     Document Type: Conference Paper
Times cited : (1)

References (31)
  • 20
    • 84876517558 scopus 로고    scopus 로고
    • in Superdense QCD Matter and Compact Stars, ed. by D. Blaschke and D. Sedrakian. Proceedings of the NATO Advanced Research Workshop, 27 September-4 October, 2003, in Yerevan, Armenia, Springer, Dordrecht, The Netherlands
    • Oertel, M. & Buballa, M. 2006, in: "Color superconducting quark matter and the interior of neutron stars" in Superdense QCD Matter and Compact Stars, ed. by D. Blaschke and D. Sedrakian. Proceedings of the NATO Advanced Research Workshop, 27 September-4 October, 2003, in Yerevan, Armenia, Springer, Dordrecht, The Netherlands, p. 187
    • (2006) Color Superconducting Quark Matter and the Interior of Neutron Stars , pp. 187
    • Oertel, M.1    Buballa, M.2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.