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Volumn 725, Issue 4-5, 2013, Pages 200-207

Possible implications of asymmetric fermionic dark matter for neutron stars

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EID: 84883050938     PISSN: 03702693     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.physletb.2013.07.017     Document Type: Article
Times cited : (102)

References (44)
  • 6
    • 84866991931 scopus 로고    scopus 로고
    • for recent reviews and extensive list of references, see
    • Davoudiasl H., Mohapatra R.N. New J. Phys. 2012, 14:095011. for recent reviews and extensive list of references, see. arxiv:1203.1247.
    • (2012) New J. Phys. , vol.14 , pp. 095011
    • Davoudiasl, H.1    Mohapatra, R.N.2
  • 10
    • 12544254683 scopus 로고    scopus 로고
    • For a review and references to mirror models, see
    • Berezhiani Z. Int. J. Mod. Phys. A 2004, 19:3775. For a review and references to mirror models, see.
    • (2004) Int. J. Mod. Phys. A , vol.19 , pp. 3775
    • Berezhiani, Z.1
  • 11
    • 34547881175 scopus 로고    scopus 로고
    • Okun L.B. Phys. Usp. 2007, 50:380. arxiv:hep-ph/0606202.
    • (2007) Phys. Usp. , vol.50 , pp. 380
    • Okun, L.B.1
  • 27
    • 82455205661 scopus 로고    scopus 로고
    • Some preliminary results of this investigation were presented by
    • Goldman I. Acta Phys. Polon. B 2011, 42:2203. Some preliminary results of this investigation were presented by. arxiv:1112.1505.
    • (2011) Acta Phys. Polon. B , vol.42 , pp. 2203
    • Goldman, I.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.