International Advisory Committee Organizing Committee

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International Advisory Committee Organizing Committee

International Advisory Committee Hiroaki Aihara, Tokyo Arthur McDonald, Queen’s Ahmed Ali, DESY Joachim Mnich, DESY Guido Altarelli, CERN, Roma-III Naba Mondal, TIFR, India Barry Barish, Caltech Aleandro Nisati, ATLAS Allesandro Bettini, Padova-Canfranc Sandip Pakvasa, Hawaii Michel Davier, Orsay Gigi Rolandi, CMS Sally Dawson, BNL D P Roy, HBCSE, Mumbai, India Dmitri Denisov, Fermilab Probir Roy, SINP, Kolkata, India Rohini Godbole, IISc, India David Saltzberg, UCLA Maury Goodman, ANL Subir Sarkar, Oxford David Gross, KITP Ashoke Sen, HRI, Allahabad, India Chen Hesheng, IHEP Bikash Sinha, SINP, Kolkata, India Rolf-Dieter Heuer, CERN Christian Spiering, DESY JoAnne Hewett, SLAC Sheldon Stone, Syracuse Young-Kee Kim, Fermilab Atsuto Suzuki, KEK Michelangelo Mangano, CERN Yoichiro Suzuki, Tokyo Patricia McBride, Fermilab Geoffrey Taylor, Melbourne Organizing Committee B S Acharya, TIFR, India Kajari Mazumdar, TIFR, India Sudeshna Banerjee, TIFR, India Naba Mondal (Co-Chairperson), TIFR, India Sunanda Banerjee, SINP, India Sunil Mukhi, TIFR, India Rahul Basu, IMSc, India (since deceased) B Mukhopadhay, HRI, India Debjyoti Choudhury, Delhi University, India Nagaraj Panyam, TIFR, India Amol Dighe, TIFR, India Sudhir Raniwala, Rajastan University, India Rajiv Gavai, TIFR, India Sreerup Raychaudhuri, TIFR, India Rohini Godbole (Co-Chairperson), Amitava Raychoudhuri, HRI, India IISc/TIFR, India S D Rindani, PRL, India Manoranjan Guchait, TIFR, India B Satyanarayana, TIFR, India Kamales Kar, SINP, India Jasbir Singh, Panjab University, India Ramesh Koul, IMSc, India K Sridhar, TIFR, India Avinash Khare, IOP, India S Uma Sankar, IIT-B, India Gobinda Majumder, TIFR, India.

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IJP a Status of Weak-Scale Supersymmetry 1
Indian J. Phys. 72A (6), 479-494 (1998) IJP A — an international journal Status of weak-scale supersymmetry1 Probir Roy Tata Institute of Fundamental Research. Homi Bhabha Road. Colaba, Mumbai-400 005 V Abstract : This article includes discussions on : (i) Standard Model and motivation for supersymmetry, (ii) Supersymmetry and MSSM. (tii) CMSSM and the mass spectra of sparticles, (iv) Experimental constraints on CMSSM parameters and (v) Conclusions Keywords : Supersymmetry, Higgs, CMSSM FACS Nos. ; 14 80 Ly, 14 80 Gt 1. Standard Model and motivation for supersymmetry Supersymmetry, as a generalized spacetime invariance under which fermions and bosons Hailstorm into each other, is undoubtedly a beautiful idea. But why should particle physicists look for it—especially at or slightly above the weak scale? The answer is that solily broken supersymmetry with an intra-supermultiplet mass breaking < 0 (TeV) can ujic the Standard Model (SM) of particle physics of a serious theoretical deficiency, viz. the ladiative instability of the Higgs mass. Before I elaborate on the last point, let me first briefly review the impressive experimental successes 11] that SM has had—if only to underscore the absence of any phenomenological need at present to go beyond it. Table 1 below contains a "pull-plot”. Various measurables (on the Z-peak) of the standard electroweak theory have been listed in ihe first column. The second column contains the measured values (combining SLD and I-hP numbers) with la errors. The "pull", defined as the deviation (with sign) of the central ^iluc from the theoretical prediction divided by the laerror in the measurement, is given in the third column.
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