Doctor of Philosophy

Total Page:16

File Type:pdf, Size:1020Kb

Doctor of Philosophy Study of Scalars and Fermions in Models Beyond the Standard Model Deepanjali Goswami A thesis submitted for the degree of Doctor of Philosophy Department of Physics Indian Institute of Technology Guwahati Guwahati 781039, India June 2019 TH-2130_136121013 TH-2130_136121013 Study of Scalars and Fermions in Models Beyond the Standard Model Deepanjali Goswami A thesis submitted for the degree of Doctor of Philosophy Supervisor: Prof. Poulose Poulose Department of Physics Indian Institute of Technology Guwahati Guwahati 781039, India June 2019 TH-2130_136121013 TH-2130_136121013 Declaration The work contained in the thesis entitled \Study of Scalars and Fermions in Models Beyond the Standard Model" has been carried out at the Department of Physics, Indian Institute of Technology Guwahati, India by me under the supervision of Prof. Poulose Poulose. The material of this thesis has not been submitted elsewhere for any other degree. Works presented in the thesis are all my own unless referenced to the contrary in the thesis. Date: (Deepanjali Goswami) June, 2019 Department of Physics Indian Institute of Technology Guwahati Guwahati - 781039, India v TH-2130_136121013 TH-2130_136121013 Disclaimer The bibliography included in this thesis is, by no means complete but contains the ones which are consulted thoroughly by me. I apologize for inadvertently missing out some of the research papers, review articles and other scientific documents pertaining to the focus of this thesis which should also have been cited. vii TH-2130_136121013 TH-2130_136121013 Prof. Poulose Poulose Department of Physics Indian Institute of Technology Guwahati Guwahati-781039, INDIA Email: [email protected] Certificate It is to certify that the work contained in the thesis entitled \Study of Scalars and Fermions in Models Beyond the Standard Model " by Ms. Deepanjali Goswami (Roll No -136121013), a PhD student in the Department of Physics, Indian Institute of Technology Guwahati is carried out under my supervision and has not been submitted elsewhere for the award of any degree. Date: Poulose Poulose (Professor) TH-2130_136121013 TH-2130_136121013 Dedicated to My parents and motherland... TH-2130_136121013 TH-2130_136121013 Acknowledgements I would like to express my gratitude, respect and appreciation to the Almighty before writing this page! This page takes me to the onset of my deep involvement of pursuing PhD degree which begins from the picturesque and the utmost naturally beautiful campus, my beloved institution, to whom I would like to thank for giving me an opportunity to be a part of it with one of the most prestigious affiliations, the Indian Institute of Technology Guwahati. I feel myself very fortunate and honoured to get such an institute to spend couple of years with wonderful people around, surrounded by scenic beauty of mother nature. The presence of mighty Brahmaputra, the beautiful hills around the campus, with its lakes inside and flowers serve as a splendid feat to make it even more exquisite. Its collective contribution has inculcated in me slowly and silently, and immensely helped me in my learning process throughout this journey. Having said that, now firstly and foremost, I would like to express my indebtful grat- itude toward my thesis supervisor Prof. Poulose Poulose for giving me an opportunity to work under his esteemed and profound guidance. His continuous support, inspiration, constant motivation, encouragement and his immense knowledge have contributed towards successful completion of my PhD research work. He has always been motivating me to learn the deeper aspects of physics and his inspirational words immensely helped me to get the high spirit to do the research and to be able to move over all the ups and downs of research life. Alongwith, I would like to thank Ms. Stavelin Ma'am for her inspirational words and their two adorable kids Hasvid and Onella for sharing many beautiful moments with me. xiii TH-2130_136121013 xiv Acknowledgements I would also like to express my sincere gratitude to my doctoral committee members: Dr. Arunansu Sil (Chairman), Dr. Udit Raha, and Dr. Soumitra Nandi, for reviewing my yearly progress with their valuable suggestions and for giving me their insightful comments and encouragement, and also for their positive critics which aspired in me to widen my research process from various prospectives. I would also like to thank, all former and current, Head of Department of Physics (Prof. Saurabh Basu, Prof. Poulose Poulose and Prof. Subhradip Ghosh), for their support and providing me various departmental facilities. It is my pleasure to thank all the faculty members of the Department of Physics, IIT Guwahati for their support and help during this journey. Specially, I would like to express my grateful thanks to Dr. Subhaditya Bhattacharya, Dr. Tarak Nath Dey, Prof. Sunil K Khijwania, Dr. Debaprasad Maity, Dr. Malay Kumar Nandy, Prof. Perumal Alagarsamy, Prof. Girish Sampath Setlur. I thank all scientific officers of Department of Physics, IITG, specially Dr. Sidananda Sarma for his motivational words and Mr. Basab Bijoy Purkayastha for his continuous support and all time help at any emergency situation with all my technical issues. I would also like to acknowledge my department office staff members for their kind help. It is my honour to reserve my special thanks to Prof. Benjamin Fuks, Dr. Debasish Borah for providing me an opportunity to work and having wonderful experience of learning while collaborating with them, I have learned several analysis techniques of my research work from Prof Fuks and my knowledge treasure has been benefitted immensely with the discussions I had with Dr. Debasish Borah. I greatly owe a lot to Prof Daniel Jeans for providing me valuable opportunity to work with him at KEK, Japan. I would like to sincerely thank him, as with him I learned the basics of the ILC study. It is my privilege to thank all my teachers, starting from my school days, whose efforts and blessings have helped me in reaching to the current position. The person who holds a special place in my heart is my father cum my teacher Prof D. D. Goswami, for teaching me motivational lesson of life and to pursue my carrier in physics. I would remain in- debted for his uncountable contribution in my life as a result of which I could achieve upto this stage. I also express my grateful thanks to my brother cum teacher Dr. Umananda Dev Goswami, for his help in making me wade through the challenging times of my life TH-2130_136121013 Acknowledgements and pursue the research. I am also highly thankful to Prof Bipul Bhuyan for his help and providing me a working space in a conducive ambience of his High Energy Physics Laboratory. He was also very kind to allow me to access his HEP cluster to carry out the necessary high speed computation for my research work. I am also thankful to him for having several insightful discussions about current physics scenarios in experimental high energy physics. I extend my acknowledgement to DAE-BRNS, Govt of India for the research fellow- ship, International Travel Support under DST, Govt. of India for presenting a paper at the APS April Meeting 2016 held at Utah, USA. I also acknowledge Govt. of Japan, for selecting me for the Invitation Fellowship Program for Young Women Researchers in Asia Pacific Countries under Athena Program to visit KEK, Japan in January 2019. I thank my research group friends: Dr. Satendra Kumar, Dr. Biswaranjan Das, Dr. Shibananda Sahoo, Subhasish Behera, Dr. Rashidul Islam, Suresh Chand and Sreemanti Chakraborti for their help and many fruitful discussions. I would also like to thank my senior research fellow members Dr. Deepanwita Dutta, Dr. Biswajit Karmakar and lab mates and friends Dr. Kamal Jyoti Nath, Maharnab, Dibyajyoti, Devender, Jyotirmoi, Shubhangi, Sunayana and Pulak for their kind help. A special thanks goes to my beloved friends Dr. Chandita Baruah, Dr. Prahlad Baruah, Niharika Baruah, Biju Bharali and Dr. Sushma Chityala for sharing the beautiful moments in the lovely IITG campus and always staying by my side in all my sad and happy times. The memories collected with them are as precious as they are. This acknowledgement would remain incomplete without the mention of the love, the care, the hard work and the sacrifice of my ancestors, my grandparents, my beloved parents, my relatives and Guruji in bringing me up and also the utmost affection, given by my entire family, specially my sister Dr. Rupanjali Goswami and brother in law Mr. Nripen Mahanta for their constant support and keeping the faith in me to allow me to do what I like. I feel myself to be extremely fortunate to gain such unimaginable strength from Mummyji, my sisters Dr. Neelima Yadav, Teshma Di and Anamika, for supporting me unconditionally, and any degree of acknowledgment to the God's gifts: Dr. Nitin Yadav, TH-2130_136121013 xvi Acknowledgements Krishna, Raj, Ruchi, Lucky, Kanha, Dolcy, would somewhere, definitely, leave in me a void of ungratefulness. June, 2019 Deepanjali Goswami TH-2130_136121013 Abstract The Standard Model (SM) of particle physics is well established with the discovery of the Higgs boson by the independent experiments, ATLAS and CMS at LHC in 2012. The properties of the discovered Higgs boson is very similar to the proposed one in the SM and the discovery is considered as a remarkable success of this model. Inspite of this success, many experimental evidences provide hints of some fundamental issues; mainly absence of dark matter (DM), non-zero neutrino mass and hierarchy problem, which shows that the SM is not a complete theory. A possible way out of this situation is to look beyond the SM(BSM) to resolve these issues by accommodating new particles in the spectrum or extending the gauge sector of the SM. Out of many attractive proposals of BSM, models governing seesaw mechanism could explain the non-zero masses of neutrinos.
Recommended publications
  • Year 2016-17
    110 108.97 96 90 70 60.91 DST 50 WB Govt. 30.23 30 20.93 24.39 Project 10 2.96 4.01 4.13 -10 Grant - 2014-15 Grant - 2015-16 Grant - 2016-17 Budget in 2016-17 : DST – 108.97 crores; WB Government – 4.13 crores Web of Science Citation Report (On 19th July, 2017) Result found 1983-2017 No. of Publications : 9939 H Index : 115 Sum of the times cited : 158271 Average citations per item : 15.92 Average citations per year : 4522.03 Performance during the year (2016-17) Publication : 444 Average Impact Factor : 4.4 Ph.D. Degree Awarded : 58 Patent Awarded : 04 Patent Filed : 14 I A C S ANNUAL REPORT 2016 - 2017 INDIAN ASSOCIATION FOR THE CULTIVATION OF SCIENCE Contents From the Director’s Desk ....................................................................... 004 The Past Glory ....................................................................................... 006 The Laurels - Faculty Members ............................................................. 012 The Laurels - Research Fellows ............................................................. 013 Key Committees .................................................................................... 014 Executive Summary ............................................................................... 017 Biological Chemistry .............................................................................. 022 Centre For Advance Materials ............................................................... 031 Director’s Research Unit .......................................................................
    [Show full text]
  • 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.
    [Show full text]
  • 2017 Progress Report
    PROGRESS REPORT Report covering the period from Nov 2016 to Sep 2017 INFRE HEPNET INDOFRENCH HIGH ENERGY PHYSICS NETWORK 2 Table of Contents I GENERAL INFORMATION ............................................................................................................................. 3 A. Highlights of the previous report presented in Nov 2016. ...................................................................... 6 B. Main highlights of this report .................................................................................................................. 7 II WORK REPORT ............................................................................................................................................. 8 A. Summary of the project ........................................................................................................................... 8 1. Original objectives ............................................................................................................................... 8 2. Report on the project work done ........................................................................................................ 9 3. Budgetary Matters and Issues ........................................................................................................... 16 4. References/Publications of the Network ........................................................................................... 18 B. Plan of work for the remaining period of the project ...........................................................................
    [Show full text]
  • Cumulative Author Index
    PHYSICAL REVIEW D VOLUME 64, NUMBER 12 15 DECEMBER 2001 Cumulative Author Index All authors of papers published in this volume are listed alphabetically. Full titles are included in each ®rst author's entry. The letters (R), (BR), (C), or (E) following the article number indicate that a paper is a Rapid Communication, a Brief Report, a Comment, or an Erratum, respectively. Aarts, Gert and JuÈrgen Berges Ð Nonequilibrium time evolution of and A. A. Kozhevnikov Ð Erratum: Measuring the ®nite width the spectral function in quantum ®eld theory. D 64, 105010͑15͒ and unitarity corrections to the ␾␻ mixing amplitude ͓Phys. Rev. Abada, A., Ph. Boucaud, G. Herdoiza, J. P. Leroy, J. Micheli, O. D 61, 054005 ͑2000͔͒.D64, 019901͑E͒͑1͒ PeÁne, and J. RodrõÂguez-Quintero Ð Preliminaries on a Adachi, I. Ð ͑see Abe, K.͒ D 64, 071101͑R͒͑1͒ lattice analysis of the pion light-cone wave function: A partonic ͑see Abe, K.͒ D 64, 072001͑1͒ signal? D 64, 074511͑1͒ Adamov, Anatoly and Gary R. Goldstein Ð Excited state contributions Abazajian, Kevork, George M. Fuller, and Mitesh Patel Ð Sterile to the heavy baryon fragmentation functions in a quark-diquark neutrino hot, warm, and cold dark matter. D 64, 023501͑15͒ model. D 64, 014021͑1͒ ͑see Pruet, Jason͒ D 64, 063002͑15͒ Adams, Allan and Eva Silverstein Ð Closed string tachyons, AdS/CFT, Abazov, V. M. et al. ͑DO” Collaboration͒ Ð Quasi-model-independent and large N QCD. D 64, 086001͑15͒ search for new physics at large transverse momentum. Adams, D. L. Ð ͑see Abazov, V. M.͒ D 64, 012004͑1͒ D 64, 012004͑1͒ ͑see Abazov, V.
    [Show full text]
  • Studies of Supersymmetry Models for the ATLAS Experiment at the Large Hadron Collider
    Studies of supersymmetry models for the ATLAS experiment at the Large Hadron Collider Alan James Barr Churchill College A dissertation submitted to the University of Cambridge for the degree of Doctor of Philosophy November 2002 ii Studies of supersymmetry models for the ATLAS experiment at the Large Hadron Collider Alan James Barr Abstract This thesis demonstrates that supersymmetry can be discovered with the ATLAS experiment even if nature conspires to choose one of two rather difficult cases. In the first case where baryon-number is weakly violated, the lightest supersym- metric particle decays into three quarks. This leads to events with a very large multiplicity of jets which presents a difficult combinatorical problem at a hadronic collider. The distinctive property of the second class of model { anomaly-mediation { is the near degeneracy of the super-partners of the SU(2) weak bosons. The heavier charged wino decays producing its invisible neutral partner, the presence of which must be inferred from the apparent non-conservation of transverse momen- tum, as well as secondary particle(s) with low transverse momentum which must be extracted from a large background. Monte-Carlo simulations are employed to show that for the models examined not only can the distinctive signature of the model can be extracted, but that a variety of measurements (such as of sparticle masses) can also be made. The final two chapters present an investigation into part of the experimental hard- ware which will be vital for these analyses. Beam tests of ATLAS semiconductor tracker modules demonstrate that this sub-detector can be expected to perform to its specification, providing the good spatial resolution and efficiency with low noise, even after the equivalent of ten years of irradiation.
    [Show full text]
  • Biswarup Mukhopadhyaya
    Biswarup Mukhopadhyaya Research Summary: (a)Different aspects of supersymmetric (SUSY) theories have been studied, with special reference to collider signals at the Large Hadron Collider (LHC). One of the important outcomes of this investigations is the identification of novel signals for scenarios with a right sneutrino as the lightest supersymmetric particle, which are being used by the experimentalists at the LHC. (Sudhir Kumar Gupta, Santosh Kumar Rai, Biswarup Mukhopadhyaya) (b)The implications of supersymmetric models in the neutrino have been inves- tigated. One area of study is the identification of viable regions in the SUSY pa- rameter space which correspond to the observed neutrino mass pattern and bi- large mixing, using flavour-dependent behaviour in the hidden sector of a broken SUSY model. (R. Srikanth Hundi, Biswarup Mukhopadhyaya). Another aspect of the above study is the identification of SUSY models where lepton number can be violated by two units (thereby allowing Majorana masses for neutrinos) but violation by one unit is heavily suppressed (thereby ensuring a SUSY dark matter candidate). It was shown how a supergravity framework can lead to such a possibility. (R. Srikanth Hundi, Biswarup Mukhopadhyaya, Soumitra SenGupta). (c) It was shown that Little Higgs theories with broken T-parity can lead to sit- uations where the Higgs boson may have dominantly invisible decay modes. It could act as a distinctive signal of such theories in certain regions of the parame- ter space. (R. Srikanth Hundi, Biswarup Mukhopadhyaya, Andreas Nyffeler). (d) Implications of a degenerate neutrino scenario was studied, where the Majo- rana neutrino phases can lead to certain conclusions about the 1-3 mixing angle in the neutrino sector.
    [Show full text]
  • The Year Book 2019
    THE YEAR BOOK 2019 INDIAN ACADEMY OF SCIENCES Bengaluru Postal Address: Indian Academy of Sciences Post Box No. 8005 C.V. Raman Avenue Sadashivanagar Post, Raman Research Institute Campus Bengaluru 560 080 India Telephone : +91-80-2266 1200, +91-80-2266 1203 Fax : +91-80-2361 6094 Email : [email protected], [email protected] Website : www.ias.ac.in © 2019 Indian Academy of Sciences Information in this Year Book is updated up to 22 February 2019. Editorial & Production Team: Nalini, B.R. Thirumalai, N. Vanitha, M. Venugopal, M.S. Published by: Executive Secretary, Indian Academy of Sciences Text formatted by WINTECS Typesetters, Bengaluru (Ph. +91-80-2332 7311) Printed by Lotus Printers Pvt. Ltd., Bengaluru CONTENTS Page Section A: Indian Academy of Sciences Memorandum of Association ................................................... 2 Role of the Academy ............................................................... 4 Statutes .................................................................................. 7 Council for the period 2019–2021 ............................................ 18 Office Bearers ......................................................................... 19 Former Presidents ................................................................... 20 Activities – a profile ................................................................. 21 Academy Document on Scientific Values ................................. 25 The Academy Trust ................................................................. 33 Section B: Professorships
    [Show full text]
  • Fostering Partnerships
    Indo-US Science and Technology Forum Joint R & D Centers Fostering Partnerships The Indo-US Science and Technology Forum (IUSSTF) established under an agreement between the Governments of India and the United States of America in March 2000, is an autonomous, not- for-profit-society that promotes science, technology, engineering and biomedical research through substantive interaction among government, media and industry. Joint R & D Centers Fostering Partnerships Indo-US Science and Technology Forum Indo-US Science and Technology Forum Contents Chemical Sciences 7 • Integrated Study of Correlated Electrons in Organic and Inorganic Materials 9 • Development of Metal-Ceramic Composites through Microwave Processing 12 • Theoretical Physics of Ultra-Cold Atoms in Optical Lattices 16 • Thin-Films and Nanostructured Emerging Coating Technologies 22 • Dynamics of Dislocations in Solid Helium and its Role in Supersolid Behavior 25 • Rational Control of Functional Oxides 29 • 3-D Engineered Electrodes for Electrochemical Energy Storage 33 • Elastohydrodynamic Lubrication Studies 37 • From Fundamentals to Applications of Nanoparticle Assemblies 40 • Crystallization at Interfaces 43 • Theoretical Studies of the Correlated Electronic Structure of Graphene 45 Engineering Sciences 49 • Highway and Airport Pavement Engineering 51 • Intelligent Transportation Systems Technologies 55 • Intelligent Structural Health Monitoring 59 • Design of Sustainable Products, Services and Manufacturing Systems 65 • Fire Center for Advancing Research and Education in
    [Show full text]
  • Arxiv:2006.07854V2 [Hep-Ph] 9 Jan 2021
    Current bounds and future prospects of light neutralino dark matter in NMSSM Rahool Kumar Barman∗ Indian Association for the cultivation of Science, Jadavpur, Kolkata 700032, India and Centre for High Energy Physics, Indian Institute of Science, Bangalore 560012, India Genevieve B´elangery LAPTh, Universit´eSavoie Mont Blanc, CNRS, B.P. 110, F-74941 Annecy Cedex, France Biplob Bhattacherjeez and Rohini Godbolex Centre for High Energy Physics, Indian Institute of Science, Bangalore 560012, India Dipan Sengupta{ Department of Physics and Astronomy, University of California, San Diego, 9500 Gilman Drive, La Jolla, USA Xerxes Tata∗∗ Department of Physics and Astronomy, University of Hawaii, Honolulu, HI 96822, USA Abstract Unlike its minimal counterpart, the Next to Minimal supersymmetric Standard Model (NMSSM) allows the possibility that the lightest neutralino could have a mass as small as ∼ 1 GeV while still providing a significant component of relic dark matter (DM). Such a neutralino can provide an invisible decay mode to the Higgs as well. Further, the observed SM-like Higgs boson (H125) could also have an invisible branching fraction as high as ∼ 19%. Led by these facts, we first delineate the region of parameter space of the NMSSM with a light neutralino (M 0 < 62:5 GeV) that yields a thermal neutralino relic density smaller than the χe1 measured relic density of cold dark matter, and is also compatible with constraints from collider searches, searches for dark matter, and from flavour physics. We then examine the prospects for probing the NMSSM with a light neutralino via direct DM detection searches, via invisible Higgs boson width experiments at arXiv:2006.07854v2 [hep-ph] 9 Jan 2021 future e+e− colliders, via searches for a light singlet Higgs boson in 2b2µ, 2b2τ and 2µ2τ channels and via pair production of winos or doublet higgsinos at the high luminosity LHC and its proposed energy upgrade.
    [Show full text]
  • List of Fellows
    The abbreviations that follow the name and affiliation of the scientist-guides are explained below: 1. S — Willing to accept students (undergraduate/graduate/postgraduate). 2. T — Willing to accept teachers (doctoral/post-doctoral). 3. AA — Accommodation may be available to the student/teacher (subject to confirmation). 4. ANA — Accommodation not available, and has to be taken care of by the student/teacher concerned. 5. The entry in brackets after the name indicates the fields of specialization of the guide. LIST OF FELLOWS 1. Abbasi, Prof. Shahid A. (sp. Environmental Engineering, Energy Studies, Limnology), Pondicherry University, Pondicherry. S, AA. 2. Acharya, Prof. B.D. (sp. Graph Theory), Bangalore. S, AA. 3. Adhya, Dr Samit (sp. Molecular Genetics of Parasites, Intracellular RNA Trafficking & DNA Diagnostics), Indian Institute of Chemical Technology, Kolkata. S, AA. 4. Adhya, Dr Tapan K. (sp. Agricultural Microorganisms), Central Rice Research Institute, Cuttack. S,T, AA. 5. Adimurthi, Prof. (sp. Nonlinear Differential Equations), TIFR Centre for Applicable Mathematics, Bangalore. S,T, AA. 6. Agarwal, Dr Avinash K. (sp. Alternative Fuels, Biodiesel Emissions, Oil Tribology, Sensors, Laser Diagnostics), Indian Institute of Technology, Kanpur. T, AA. 7. Ahmad, Prof. Talat (sp. Igneous Petrology, Geochemistry, Himalayan Geology), University of Delhi, Delhi. S, AA. 8. Ahuja, Dr Paramvir S. (sp. Plant Improvement), Institute of Himalayan Bioresource Technology, Palampur. S,T, AA. 9. Ajayaghosh, Dr A. (sp. Organic Functional Materials, Molecular Self-Assembly), National Institute for Interdisciplinary Science & Technology, Thiruvananthapuram. S, AA. 10. Amarnath, Prof. T. (sp. Fluid Mechanics), University of Hyderabad, Hyderabad. T, AA. 1033 11. Amla, Dr Devindra V. (sp. Plant Molecular Biology & Biotechnology), National Botanical Research Institute, Lucknow.
    [Show full text]
  • Newest LIC Ids 15.11.19.Xlsx
    S.N. EIS Code Employee Name LIC ID 1 42735 BARRE SURYA KAMALA SULOCHANA B 5294 2 90003781 S N KATIYAR 21439 3 90003856 N. SINGH 18355 4 90004490 MANIK LAL BANERJEE 18208 5 90004862 S.B.CHAKRAVARTY 21477 6 90005042 AVTAR KRISHAN 18212 7 90005448 R.K.SINGH 18049 8 90005489 SHREE RAM SHARMA 21951 9 90006289 CHANDRA NATH MISHRA 18000 10 90006362 T K BANDYOPADHYAY 26144 11 90006586 K.K.TIWARI 20787 12 90006693 ASHOK SARKAR 8323 13 90006990 Y C SINHA 17980 14 90007261 BIKASH SAMANTA 18221 15 90007311 T.K.LAHIRI 18494 16 90007345 O.RAHMAN 26164 17 90007725 CHHABI SHANKER CHAWLEY 23846 18 90008004 MAINAK DUTTA 15968 19 90008012 ANOOP KUMAR SENGUPTA 8551 20 90008814 SHRI B.PRASAD 20202 21 90008822 GORA KOLEY 20916 22 90008863 SATYA NARAYAN SINGH 15900 23 90009093 JASWINDER PAL SINGH 21614 24 90009150 H.S.KHARE 18927 25 90009184 SUBIR GHOSH 20934 26 90009390 DINESH CHANDRA JHA 25050 27 90009614 SHEKHAR SARAN 11931 28 90009622 RAVINDRA KUMAR NIGAM 15189 29 90009788 GOPAL SINGH 17674 30 90009879 GANESH SHARMA 3398 31 90009911 PULAK BARAN CHAKRABARTY 18851 32 90010091 V.S.RAI 26957 33 90010141 BIBHASH CHANDRA MAJI 19314 34 90011289 NEELACHAL NAYAK 18227 35 90012071 R. P. SINHA 20793 36 90012261 AJAY KUMAR RAYGHATAK 18163 37 90013152 TEISONI SANGMA 8210 38 90013368 KAPIL DEO SINGH 17992 39 90014358 JAYANT V NAIK 23870 40 90016353 BIRENDRA KUMAR SINGH 18150 41 90016429 UTPAL ROY 11741 42 90016899 B.K.SINHA 26240 43 90017583 A.K.HAZARE 8498 44 90017641 BIBHUTI KUMAR SINGH 18053 45 90017682 ALOK KUMAR MUKHOPADHYAY 16459 46 90018060 THAKUR B.N.
    [Show full text]
  • List of All Publications by Rohini M. Godbole the Citation Index Quoted
    List of all publications by Rohini M. Godbole The citation index quoted for some of the publicationsis taken from the HEP data base INSPIRE and the url is: (http://inspirehep.net/search?ln=en&ln=en&p=find+a+godbole&of=hb&action search=Search &sf=earliestdate&so=d&rm=&rg=25&sc=0) and citation summary is available at (http://inspirehep.net/search?ln=en&p=find+a+godbole&of=hcs&action search=Search &sf=earliestdate&so=d) In particle physics the author list is alphabetical and first author has no special meaning. For information about list of publications available from INSPIRE- HEP data base, see at the end. A Full length research papers: 1. R. M. Godbole, A. Kaushik and A. Misra, \Transverse single-spin asymmetry in the low-virtuality leptoproduction of open charm as a probe of the gluon Sivers function," Phys. Rev. D 97, no. 7, 076001 (2018), [arXiv:1709.03074 [hep-ph]]. 2. S. Banerjee, G. Blanger, B. Bhattacherjee, F. Boudjema, R. M. Godbole and S. Mukher- jee, \Novel signatures for long-lived particles at the LHC," arXiv:1706.07407 [hep- ph]. 3. R. M. Godbole, A. Kaushik, A. Misra, V. Rawoot and B. Sonawane, \Transverse single spin asymmetry in p + p" ! J= + X," Phys. Rev. D 96 (2017) no.9, 096025, [arXiv:1703.01991 [hep-ph]]. 4. R. K. Barman, G. Belanger, B. Bhattacherjee, R. Godbole, G. Mendiratta and D. Sengupta, \Invisible decay of the Higgs boson in the context of a thermal and nonthermal relic in MSSM," Phys. Rev. D 95 (2017) no.9, 095018, [arXiv:1703.03838 [hep-ph]].
    [Show full text]