Download Neutrino Mass, Dark Matter, Gravitational Waves, Monopole by Behram N. Kursunoglu (auth.), Behram N. Kursunoglu, Stephan PDF

By Behram N. Kursunoglu (auth.), Behram N. Kursunoglu, Stephan L. Mintz, Arnold Perlmutter (eds.)

The foreign convention, Orbis Scientiae 1996, desirous about the themes: The Neutrino Mass, mild Cone Quantization, Monopole Condensation, darkish topic, and Gravitational Waves which we have now followed because the identify of those court cases. was once there any intriguing information on the convention? might be, it is determined by who solutions the query. there has been a nearly unanimous contract at the total luck of the convention as used to be evidenced via the truth that within the after-dinner feedback by way of considered one of us (BNK) the advice of organizing the convention on a biannual foundation used to be offered yet no longer authorized: the members sought after the continuation of the culture to convene each year. we will, in fact, comply. the predicted remark of gravitational waves will represent the main intriguing vindication of Einstein's basic relativity. This topic is attracting the eye of the experimentalists and theorists alike. we are hoping that via the 1st decade of the 3rd millennium or past, gravitational waves might be detected, starting the way in which for a look for gravitons someplace within the universe, most likely during the observations within the CMBR. The theoretical foundation of the graviton seek will take us to quantum gravity and finally to the amendment of common relativity to incorporate the Planck scale habit of gravity -at energies 19 of the order of 10 Ge V.

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Extra resources for Neutrino Mass, Dark Matter, Gravitational Waves, Monopole Condensation, and Light Cone Quantization

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By combining the Ward-Takahashi identities with the LSZ reduction formula we can show that color confinement is realized provided that successive applications of the BRS and anti-BRS transformations annihilate the second term in the asymptotic gluon field. This is indeed a sufficient condition to be referred to as the condition A. Since the asymptotic field is a rather complicated object, we shall express this condition in terms of Heisenberg operators. For this purpose let us consider a two-point function defined as the vacuum expectation value (VEV) of the time-ordered product of the gauge field and the current corresponding to the deviation from the Maxwell equation.

_ Similarly, the B-violating coupling >'~33 leads to tR --t bRsR, bRsR decays, with partial widths r(t --t bs) = r(t --t bs) = (~~~2 mt (1 - m~/m;)2 , (41) neglecting mb and m. and assuming a common squark mass mb = m. = m q. 16 (>'~33? (for mq = 150 GeV) . (39)), giving altogether t --t (bs,sb) --t bsX~ --t (cbbbs,cbbbs). (43) This all-hadronic mode could in principle be identified experimentally, through the multiple b-jets plus the t --t 5-jet and X~ --t 3-jet invariant mass constraints. However, it would not be readily mistaken for the SM hadronic mode t --t bW --t 3-jet, and would simply reduce all the SM top signal rates.

Assuming, as we do, that only the RPV couplings A233, A;33 or A~33 are nonzero, it turns out 12 that the one-loop RGE for mixing angles and the C P-violation parameter J = Im(v"d v". v,,*. 1 2 or J. Nevertheless the evolution of CKM angles differs from the MSSM because the evolution of the Yukawa couplings on the right hand side is altered by the RPV couplings. 3. NUMERICAL RGE STUDIES It is instructive to supplement our algebraic arguments above with explicit numerical solutions of the RGE. Figure 1 shows the fixed-point behaviour of the three RPV couplings considered in this paper, (A~33' A;33, A233) along with the corresponding fixed point behaviour for At, assuming that tan,8 is small so that Ab and AT are negligible.

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