Vanishing corrections on the intermediate scale and implications for unification of forces.pdf

Vanishing corrections on the intermediate scale and implications for unification of forces.pdf

  1. 1、本文档共21页,可阅读全部内容。
  2. 2、有哪些信誉好的足球投注网站(book118)网站文档一经付费(服务费),不意味着购买了该文档的版权,仅供个人/单位学习、研究之用,不得用于商业用途,未经授权,严禁复制、发行、汇编、翻译或者网络传播等,侵权必究。
  3. 3、本站所有内容均由合作方或网友上传,本站不对文档的完整性、权威性及其观点立场正确性做任何保证或承诺!文档内容仅供研究参考,付费前请自行鉴别。如您付费,意味着您自己接受本站规则且自行承担风险,本站不退款、不进行额外附加服务;查看《如何避免下载的几个坑》。如果您已付费下载过本站文档,您可以点击 这里二次下载
  4. 4、如文档侵犯商业秘密、侵犯著作权、侵犯人身权等,请点击“版权申诉”(推荐),也可以打举报电话:400-050-0827(电话支持时间:9:00-18:30)。
查看更多
Vanishing corrections on the intermediate scale and implications for unification of forces

a r X i v : h e p - p h / 9 7 1 0 2 4 6 v 1 5 O c t 1 9 9 7 VANISHING CORRECTIONS ON INTERMEDIATE SCALE AND IMPLICATIONS FOR UNIFICATION OF FORCES M.K.Parida High Energy Physics Group International Center for Theoretical Physics I-34100 Trieste,Italy and Physics Department North–Eastern Hill University P.O.Box 21, Laitumkhrah, Shillong 793 003 India (March 19, 1996) Abstract In two–step breaking of a class of grand unified theories including SO(10), we prove a theorem showing that the scale (MI) where the Pati–Salam gauge symmetry with parity breaks down to the standard gauge group, has vanish- ing corrections due to all sources emerging from higher scales (μ MI) such as the one–loop and all higher–loop effects, the GUT–threshold, gravitational smearing, and string threshold effects. Implications of such a scale for the unification of gauge couplings with small Majorana neutrino masses are dis- cussed. In string inspired SO(10), we show that MI ? 5× 10 12 GeV, needed for neutrino masses, with the GUT scale MU ? Mstr can be realized provided certain particle states in the predicted spectrum are light. 12.10.Dm, 12.60.Jv Typeset using REVTEX 1 I. INTRODUCTION Grand unified theories based upon SUSY SU(5), SO(10), nonSUSY SO(10) with inter- mediate symmetries, and those inspired by superstrings have been the subject of considerable interest over recent years. In order to solve the strong CP problem through Peccei–Quinn mechanism and achieve small neutrino masses [1] necessary to understand the solar neutrino flux [2] and/or the dark matter of the universe, an intermediate scale seems to be essential [3]. Such a scale might correspond to the spontaneous breaking of gauged B–L contained in intermediate gauge symmetries like SU(2)L × SU(2)R × U(1)B?L × SU(3)C(≡ G2213) and SU(2)L × SU(2)R × SU(4)C (≡ G224) with [3-6] or without [7] parity, or even others like SU(2)L × U(1)I3R × SU(4)C and SU(2)L × U(1)I3R × U(1)B?L × SU(3)C . But it is well known that the predictions

文档评论(0)

l215322 + 关注
实名认证
内容提供者

该用户很懒,什么也没介绍

1亿VIP精品文档

相关文档