Academic Report 2008–09
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Self-Study Report
Presidency University Self-Study RepoRt For Submission to the National Assessment and Accreditation Council Presidency University Kolkata 2016 (www.presiuniv.ac.in) Volume-3 Self-Study Report (Volume-3) Departmental Inputs 1 Faculty of Natural and Mathematical Sciences Self-Study RepoRt For Submission to the National Assessment and Accreditation Council Presidency University Kolkata 2016 (www.presiuniv.ac.in) Volume-3 Departmental Inputs Faculty of Natural and Mathematical Sciences Table of Contents Volume-3 Departmental Inputs Faculty of Natural and Mathematical Sciences 1. Biological Sciences 1 2. Chemistry 52 3. Economics 96 4. Geography 199 5. Geology 144 6. Mathematics 178 7. Physics 193 8. Statistics 218 Presidency University Evaluative Report of the Department : Biological Sciences 1. Name of the Department : Biological Sciences 2. Year of establishment : 2013 3. Is the Department part of a School/Faculty of the university? Faculty of Natural and Mathematical Sciences 4. Names of programmes offered (UG, PG, M.Phil., Ph.D., Integrated Masters; Integrated Ph.D., D.Sc., D.Litt., etc.) : B.Sc (Hons) in Biological Sciences, M.sc. in Biological Sciences, PhD. 5. Interdisciplinary programmes and de partments involved: ● The Biological Sciences Department is an interdisciplinary department created by merging the Botany, Zoology and Physiology of the erstwhile Presidency College. The newly introduced UG (Hons) and PG degree courses Biological Sciences cut across the disciplines of life science and also amalgamated the elements of Biochemistry, Statistics and Physics in the curricula. ● The UG elective General Education or ‘GenEd’ programmes, replace the earlier system of taking ‘pass course’ subjects and introduce students to a broad range of topics from across the disiplines. -
IUCAA Bulletin 2016
Editor : Editorial Assistant : Somak Raychaudhury Manjiri Mahabal ([email protected]) ([email protected]) A quarterly bulletin of the Inter-University Centre for Astronomy and Astrophysics ISSN 0972-7647 (An autonomous institution of the University Grants Commission) Available online at http://ojs.iucaa.ernet.in/ 27th IUCAA Foundation Day Lecture Introduction A Natural History of The 27th IUCAA Foundation Day Knowledge Lecture was delivered by the eminent A naturalist lives today in a world of Indian ecologist, Professor Madhav wounds, but for a connoisseur of Gadgil on December 29, 2015. Over a knowledge, ours is a golden age; the career spanning more than four decades, challenge before us is to deploy the strengths Professor Gadgil has championed the of our age to heal the wounds. Life is an effort towards the preservation of information-based, progressive and ecology in India, which includes cooperative enterprise, evolving organisms establishing the Centre for Ecological capable of handling greater and greater Sciences under the aegis of the Indian quantities, of increasingly more complex Institute of Science, Bengaluru in 1983 information, ever more effectively. Social and serving as the Head of the Western animals have taken this to new heights, with be unhappy in this as well as the nether Ghats Ecology Expert Panel of 2010, humans surpassing them, all thanks to the world. The ruling classes have always tried popularly known as the Gadgil language abilities, and the greatly enhanced to keep the populace ignorant as preached Commission. An alumnus of Harvard capacity to learn, teach, and to elaborate by Laozi, a contemporary of Buddha: The University, he is a recipient of the Padma memes, including mythologies and people are hard to rule when they have too Shri and Padma Bhushan from the scientific knowledge. -
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. -
Probing the Universe at Low Radio Frequencies Using the GMRT
The GMRT : a look at the Past, Present and Future Yashwant Gupta & Govind Swarup National Centre for Radio Astrophysics Pune India URSI GASS Montreal 2017 The GMRT : a look at the Past, Present and Future Yashwant Gupta & Govind Swarup National Centre for Radio Astrophysics Pune India URSI GASS Montreal 2017 Overview of today’s talk . Part I : the GMRT -- a historical perspective . Part II : the GMRT -- current status . Part III : future -- the upgraded GMRT Some history . It is the early 1980s… the VLA has recently become operational . Radio astronomy has shifted from the low frequencies, where it was born, to higher frequencies (cm and higher wavelengths) -- obvious reasons . Note, however, techniques like self-cal have been shown to work . In India, the radio astronomy group at the Tata Institute, under the leadership of Govind Swarup, is looking for the next big challenge… They have already : . Built the Ooty Radio Telescope in the late 1960s – still operational & producing international quality results (in fact, currently being upgraded with new receiver system!) . Built the Ooty Synthesis Radio Telescope (1980s) – short-lived but valuable learnings . Built up considerable experience in low frequencies (metre wavelengths) Birth of the GMRT . Motivation : bridge the gap in radio astronomy facilities at low frequencies and address science problems best studied at metre wavelengths . First concept : 1984 (started with large cylinders); evolved to 34 dishes of 45 metres by 1986 . Project cleared and funding secured by 1987 . Construction started : 1990; first antenna erected : 1992 . First light observations : 1997 – 1998 . Released for world-wide use : 2002 The GMRT : turning it ON Jan 1997 : First fringes with the prototype GMRT correlator Dec 1998 : first light pulsar observation with the GMRT Dedication of the GMRT The Giant Metrewave Radio Telescope was dedicated to the World Scientific Community by the Chairman of TIFR Council, Shri Ratan Tata. -
Academic Report ( 2019–20 )
Academic Report ( 2019–20 ) Harish - Chandra Research Institute Chhatnag Road, Jhunsi Prayagraj (Allahabad), India 211019 Contents 1. About the Institute 2 2. Director’s Report 4 3. List of Governing Council Members 5 4. Staff List 7 5. Academic Report - Mathematics 15 6. Academic Report - Physics 100 7. HRI Colloquia 215 8. Mathematics Talks and Seminars 216 9. Physics Talks and Seminars 218 10. Recent Graduates 222 11. Publications 224 12. Preprints 233 13. About the Computer Section 240 14. Library 242 15. Construction Activity 245 1 About The Institute History The Harish-Chandra Research Institute is one of the premier research institutes in the country. It is an autonomous institution fully funded by the Department of Atomic En- ergy (DAE), Government of India. The Institute was founded as the Mehta Research Institute of Mathematics and Mathematical Physics (MRI). On 10th Oct 2000 the In- stitute was renamed as Harish-Chandra Research Institute (HRI) after the acclaimed mathematician, the late Prof Harish-Chandra. MRI started with the efforts of Dr. B. N. Prasad, a mathematician at the University of Allahabad, with initial support from the B. S. Mehta Trust, Kolkata. Dr. Prasad was succeeded in January 1966 by Dr. S. R. Sinha, also of Allahabad University. He was followed by Prof. P. L. Bhatnagar as the first formal Director. After an interim period, in January 1983 Prof. S. S. Shrikhande joined as the next Director of the Institute. During his tenure the dialogue with the DAE entered into decisive stage and a review committee was constituted by the DAE to examine the Institute’s future. -
Prime Minister Dr Manmohan Singh Gives Away
ISSN 0409-7467 VOL 59 NO 1 15 JANUARY 2009 Prime Minister Dr Manmohan Singh gives away Shanti Swarup Bhatnagar Prizes for 2007 & 2008, CSIR Diamond Jubilee Technology Award for 2007 and CSIR Award for S&T Innovation for Rural Development for 2007 & 2008 Seen on the dais at the CSIR Award Presentation Function: Prime Minister Dr Manmohan Singh (centre), Minister for Science & Technology and Earth Sciences and Vice President, CSIR, Shri Kapil Sibal (left ) and Director General, CSIR, Prof. Samir K. Brahmachari Prime Minister of India and President, CSIR, Dr Manmohan Singh, gave away Shanti Swarup Bhatnagar Prizes for 2007 & 2008. CSIR Diamond Jubilee Technology Award for 2007 and CSIR Award for S&T Innovation for Rural Development for 2007 & 2008, at a glittering function held on 20 December 2008 in the Dr D.S. Kothari Auditorium, DRDO Bhawan, New Delhi. Attended by a galaxy of S&T personnel, the function was presided over by Shri Kapil Sibal, Minister for Science & Technology and Earth Sciences and Vice President, CSIR. Prof Samir K. Brahmachari, Director General, CSIR, proposed a vote of thanks. We bring in this issue, speeches of Dr Manmohan Singh, Shri Kapil Sibal and Prof. Brahmachari on the occasion along with the citations of the prize-winners. 15 JANUARY 2009 1 CSIR Award Function Speech of Prime Minister Dr Manmohan Singh am very pleased to be here in laboratories.” Iyour midst today to give away the It is this energy and this Shanti Swarup Bhatnagar Prizes for enthusiasm of our scientists that we the years 2007 & 2008. I honour and celebrate each year on congratulate each one of the award such events. -
Calcutta University Physics Alumni Association (CUPAA) Registered Alumni Members Please Check Your Serial Number from the List Below Name Year Sl
Calcutta University Physics Alumni Association (CUPAA) Registered Alumni Members Please check your serial number from the list below Name Year Sl. Dr. Joydeep Chowdhury 1993 45 Dr. Abhijit Chakraborty 1990 128 Mr. Jyoti Prasad Banerjee 2010 152 Mr. Abir Sarkar 2010 150 Dr. Kalpana Das 1988 215 Dr. Amal Kumar Das 1991 15 Mr. Kartick Malik 2008 205 Ms. Ambalika Biswas 2010 176 Prof. Kartik C Ghosh 1987 109 Mr. Amit Chakraborty 2007 77 Dr. Kartik Chandra Das 1960 210 Mr. Amit Kumar Pal 2006 136 Dr. Keya Bose 1986 25 Mr. Amit Roy Chowdhury 1979 47 Ms. Keya Chanda 2006 148 Dr. Amit Tribedi 2002 228 Mr. Krishnendu Nandy 2009 209 Ms. Amrita Mandal 2005 4 Mr. Mainak Chakraborty 2007 153 Mrs. Anamika Manna Majumder 2004 95 Dr. Maitree Bhattacharyya 1983 16 Dr. Anasuya Barman 2000 84 Prof. Maitreyee Saha Sarkar 1982 48 Dr. Anima Sen 1968 212 Ms. Mala Mukhopadhyay 2008 225 Dr. Animesh Kuley 2003 29 Dr. Malay Purkait 1992 144 Dr. Anindya Biswas 2002 188 Mr. Manabendra Kuiri 2010 155 Ms. Anindya Roy Chowdhury 2003 63 Mr. Manas Saha 2010 160 Dr. Anirban Guha 2000 57 Dr. Manasi Das 1974 117 Dr. Anirban Saha 2003 51 Dr. Manik Pradhan 1998 129 Dr. Anjan Barman 1990 66 Ms. Manjari Gupta 2006 189 Dr. Anjan Kumar Chandra 1999 98 Dr. Manjusha Sinha (Bera) 1970 89 Dr. Ankan Das 2000 224 Prof. Manoj Kumar Pal 1951 218 Mrs. Ankita Bose 2003 52 Mr. Manoj Marik 2005 81 Dr. Ansuman Lahiri 1982 39 Dr. Manorama Chatterjee 1982 44 Mr. Anup Kumar Bera 2004 3 Mr. -
Annual Report 2007 - 2008 Indian Academy
ACADEMY OF SCIENCES BANGALORE ANNUAL REPORT 2007 - 2008 INDIAN ACADEMY ANNUAL REPORT 2007-2008 INDIAN ACADEMY OF SCIENCES BANGALORE Address Indian Academy of Sciences C.V. Raman Avenue Post Box No. 8005 Sadashivanagar P.O. Bangalore 560 080 Telephone 80-2361 2546, 80-2361 4592, (EPABX) 80-2361 2943, 80-2361 1034 Fax 91-80-2361 6094 Email [email protected] Website www.ias.ac.in Contents 1. Introduction 5 2. Council 6 3. Fellowship 6 4. Associates 10 5. Publications 10 6. Academy Discussion Meetings 18 7. Academy Public Lectures 22 8. Raman Chair 24 9. Mid-Year Meeting 2007 24 10. Annual Meeting 2007 – Thiruvananthapuram 26 11. Science Education Programme 28 12. Finances 44 13. Acknowledgements 44 14. Tables 45 15. Annexures 47 16. Statement of Accounts 55 INDIAN ACADEMY OF SCIENCES BANGALORE 4 ANNUAL REPORT 2007 - 2008 1 Introduction The Academy was founded in 1934 by Sir C.V. Raman with the main objective of promoting the progress and upholding the cause of science (both pure and applied). It was registered as a Society under the Societies Registration Act on 24 April 1934. The Academy commenced functioning with 65 Fellows and the formal inauguration took place on 31 July 1934 at the Indian Institute of Science, Bangalore. On the afternoon of that day its first general meeting of Fellows was held where Sir C.V. Raman was elected its President and the draft constitution of the Academy was approved and adopted. The first issue of the Academy Proceedings was published in July 1934. The present report covering the period from April 2007 to March 2008 represents the seventy-fourth year of the Academy. -
Event Shape Discrimination of Supersymmetry from Large Extra Dimensions at a Linear Collider
Physics Letters B 634 (2006) 295–301 www.elsevier.com/locate/physletb Event shape discrimination of supersymmetry from large extra dimensions at a linear collider Partha Konar ∗,1, Probir Roy Department of Theoretical Physics, Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai 400 005, India Received 20 October 2005; received in revised form 12 January 2006; accepted 13 January 2006 Available online 3 February 2006 Editor: T. Yanagida Abstract The production of a charged lepton ( = e,μ) pair with a large missing energy at a linear collider is discussed as a means of distinguishing the minimal supersymmetry (MSSM) scenario from that with large extra dimensions (ADD) for parameter ranges where the total cross-sections are comparable for both. Analyses in terms of event shape variables, specifically sphericity and thrust, are shown to enable a clear discrimination in this regard. © 2006 Elsevier B.V. All rights reserved. PACS: 04.50.+h; 11.10.Kk; 11.25.Mj; 12.60.Jv; 13.66.Hk; 14.80.Ly Keywords: Linear collider; Beyond standard model; Supersymmetry phenomenology; Large extra dimensions; Event shape variable 1. Introduction fest itself at sub-TeV to TeV energies, its signals ought to show up at the upcoming Large Hadron Collider (LHC) at CERN. It A general expectation in high energy physics today is that is widely accepted, nonetheless, that the precise nature of the of physics beyond the standard model (BSM) emerging at TeV BSM physics responsible for such signals may not always be energies. Supersymmetry (SUSY) [1] and extra dimensions [2] easily gleaned from analyses of the corresponding data on ac- are two alternative possibilities in this direction that are the count of the complexity of the hadronic environment in any most exciting. -
Amitava Raychaudhuri
Amitava Raychaudhuri Research Summary: In 2007-08, research has been carried out in aspects of neutrino physics, particle physics models based on space-time with extra dimensions, and quark models. In continuing work on the prospects of the proposed Iron Calorimeter detector at INO being used as an end-detector for a very long baseline experiment in con- junction with a beta-beam source in Europe, it has been shown that this set-up has unmatched sensitivity for probing many of the remaining unknowns of the neutrino mass matrix. Related work on long baseline experiments with a beta- beam have (a) explored the possibility of using the survival probability Pee and (b) optimised the baseline, boost-factor, and luminosities for the best reach for probing the open issues of neutrino physics. The upper bound on the mass of the lightest neutral higgs scalar is shown to be considerably relaxed in models in which SUSY is embedded in space-time of more than four dimensions. Even though the observational evidence for the ‘pentaquark’ is currently not strong, such a bound state is a consequence of QCD. The group theory of the ‘triquark’ – which is a aconstitutent of the pentaquark – has been examined with a focus on the colour-spin SU(6) structure. Using these results, the masses of the different pentaquak states and their colour-spin excitations have been estimated. Publications: 1. Sanjib Kumar Agarwalla, Sandhya Choubey, Srubabati Goswami, and Ami- tava Raychaudhuri, Neutrino parameters from matter effects in Pee at long base- lines, Phys. Rev. D75, 097302 (2007) 2. Abhijit Samanta, Sudeb Bhattacharya, Ambar Ghosal, Kamales Kar, Deba- sish Majumdar, and Amitava Raychaudhuri, A GEANT-based study of atmo- spheric neutrino oscillation parameters at INO, Int. -
00224Notice 10212019.Pdf
District-Gorakhpur, College Name-MADAN MOHAN MALAVIYA UNIVERSITY OF TECHNOLOGY, GORAKHPUR, Postmatric 2019-20 (Fresh) ALL Application For Session 2019-20 as on 18- 10-2019 Serial No.Registration No Name Father Name Date Of Birth Caste Course Course Branch YearType Student TypeClaim FeesStatus 1 580380501901323 AASHISH KUMAR MISHRA RAVI PRAKASH MISHRA 21/01/2001 GEN B.TECH/B.E.Bachelor of Technology (Electrical1 Regular EngineeringD/s 80900 ) Forwd 2 580380501901096 AASTHA SHUKLA RANG NATH SHUKLA 12/04/1999 GEN M.SC M.Sc. in Mathematics and1 ComputingRegular D/s 41900 Forwd 3 580380501901048 AAYUSH SRIVASTAV JAI SHANKAR LAL SRIVASTAV 14/12/1999 GEN B.TECH/B.E.Bachelor of Technology (Electrical1 Regular EngineeringD/s 80900 ) Forwd 4 580380501900555 ABHAY RAJ SINGH SURYA PRATAP SINGH 02/04/2000 GEN B.TECH/B.E.Bachelor of Technology (Mechanical1 Regular Engineering)Host 25900 Forwd 5 580380501900038 ABHIJEET KUMAR SINGH RAJEEV RANJAN SINGH 01/03/1998 GEN B.TECH/B.E.Bachelor of Technology (Computer3 Regular ScienceHost &80900 Engineering)Forwd 6 580380501900942 ABHINAV PRAKASH PANDEY GIRISH CHANDRA PANDEY 27/07/2000 GEN B.TECH/B.E.Bachelor of Technology (Electrical1 Regular EngineeringHost 25900 ) Forwd 7 580380501900314 ABHINAY SINGH UDAY PRATAP SINGH 25/08/1997 GEN MCA Master in Computer Applications1 Regular D/s 55900 Forwd 8 580380501901425 ABHISHEK MISHRA GYANENDRA DHAR MISHRA 10/10/1998 GEN B.TECH/B.E.Bachelor of Technology (Electranics2 Regular &D/s Communication)90000 Forwd 9 580380501900571 ABHISHEK PANDEY RAKESH PANDEY 29/01/2001 -
Academic Report ( 2018–19 )
Academic Report ( 2018–19 ) Harish - Chandra Research Institute Chhatnag Road, Jhunsi Prayagraj (Allahabad), India 211019 Contents 1. About the Institute 2 2. Director’s Report 4 3. List of Governing Council Members 5 4. Staff list 6 5. Academic Report - Mathematics 15 6. Academic Report - Physics 100 7. HRI Colloquia 219 8. Mathematics Talks and Seminars 220 9. Physics Talks and Seminars 222 10. Recent Graduates 226 11. Publications 227 12. Preprints 236 13. About the Computer Section 242 14. Library 244 15. Construction Activity 247 1 About The Institute History: The Harish-Chandra Research Institute is one of the premier research in- stitutes in the country. It is an autonomous institution fully funded by the Department of Atomic Energy (DAE), Government of India. The Institute was founded as the Mehta Research Institute of Mathematics and Mathematical Physics (MRI). On 10th Oct 2000 the Institute was renamed as Harish-Chandra Research Institute (HRI) after the acclaimed mathematician, the late Prof Harish-Chandra. MRI started with the efforts of Dr. B. N. Prasad, a mathematician at the University of Allahabad, with initial support from the B. S. Mehta Trust, Kolkata. Dr. Prasad was succeeded in January 1966 by Dr. S. R. Sinha, also of Allahabad University. He was followed by Prof. P. L. Bhatnagar as the first formal Director. After an interim period, in January 1983 Prof. S. S. Shrikhande joined as the next Director of the Institute. During his tenure the dialogue with the DAE entered into decisive stage and a review committee was constituted by the DAE to examine the Institute’s future.