메뉴 건너뛰기




Volumn 58, Issue 1, 1998, Pages

[Formula Presented] constraints on the minimal supergravity model with large [Formula Presented]

Author keywords

[No Author keywords available]

Indexed keywords


EID: 85039014907     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.58.015007     Document Type: Article
Times cited : (12)

References (65)
  • 2
    • 85038983000 scopus 로고    scopus 로고
    • See, e.g., M. Drees and S. Martin, in Electroweak Symmetry Breaking and New Physics at the TeV Scale, edited by T. Barklow, S. Dawson, H. Haber, and J. Seigrist (World Scientific, Singapore, 1995)
    • Drees and, M.1    Martin, S.2
  • 3
    • 85039017187 scopus 로고    scopus 로고
    • hep-ph/9609374
    • see also J. Amundson, in New Directions for High Energy Physics, edited by D. G. Cassel, L. Trindle Gennari, and R. H. Siemann (Stanford Linear Accelerator Center, Stanford, CA, 1996), hep-ph/9609374.
    • Amundson, J.1
  • 7
    • 4244034193 scopus 로고
    • Note that recently the ALEPH Collaboration (at the International Europhysics Conference on High Energy Physics, Jerusalem, Israel, 1997) has made a preliminary announcement of a measurement of (Formula presented). We do not include this preliminary result in our analysis, and caution the reader that some of our conclusions may change if the (Formula presented) decay rate turns out to be closer to this ALEPH value
    • CLEO Collaboration, M. S. Alam, Phys. Rev. Lett. 74, 2885 (1995). Note that recently the ALEPH Collaboration (at the International Europhysics Conference on High Energy Physics, Jerusalem, Israel, 1997) has made a preliminary announcement of a measurement of (Formula presented). We do not include this preliminary result in our analysis, and caution the reader that some of our conclusions may change if the (Formula presented) decay rate turns out to be closer to this ALEPH value.
    • (1995) Phys. Rev. Lett. , vol.74 , pp. 2885
    • Alam, M.S.1
  • 28
    • 85039031501 scopus 로고
    • C. Wagner, hep-ph/9510341 (1995)
    • (1995)
    • Wagner, C.1
  • 34
    • 85039010288 scopus 로고    scopus 로고
    • See Borzumati
    • See Borzumati 6.
  • 52
  • 53
    • 85039012971 scopus 로고    scopus 로고
    • and C. Grueb and T. Hurth, hep-ph/9708214 (1997) quote a somewhat higher SM value of (Formula presented) than is presented here. The above works include a 3% increase due to non-perturbative effects calculated by
    • (1997)
    • Grueb, C.1    Hurth, T.2
  • 54
    • 0000988533 scopus 로고    scopus 로고
    • M. B. Voloshin, Phys. Lett. B 397, 275 (1997) plus the corrected value of (Formula presented) in their calculations, which conspire to increase the SM decay rate by about 10%. These effects would similarly increase our estimate of the SUSY contributions.
    • (1997) Phys. Lett. B , vol.397 , pp. 275
    • Voloshin, M.B.1
  • 61
    • 0001576549 scopus 로고    scopus 로고
    • Phys. Rev. Dthe results shown here are from H. Baer and M. Brhlik, 53, 597 (1996); further references are included in these reports.
    • (1996) Phys. Rev. D , vol.53 , pp. 597
    • Baer, H.1    Brhlik, M.2
  • 62
    • 85039012167 scopus 로고    scopus 로고
    • See e.g., J. Primack, astro-ph/9707285 (1997).
    • (1997)
    • Primack, J.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.