Faculty Profile Inside Physics Final Final

Faculty Profile Inside Physics Final Final

IISER Pune: A New Initiative in Science Education and Research in India India of the 21st Century is headed towards knowledge economy, which is expected to bring changes in the economic scenario. In this context, we are ushering a new education system in science and technology. Amongst the many initiatives of the country is the establishment of the Indian Institutes of Science Education and Research (IISERs). These autonomous research institutes have been set up at five locations across India, one of them in Pune, by the Ministry of Human Resource Development, Govt. of India with the primary goal of integrating high quality research with undergraduate teaching to improve science education in India and to enhance the number and quality of future academic as well as industrial researchers of the country. The model of education at IISER Pune (http://www.iiserpune.ac.in) is concept-based and inquiry-driven, as opposed to the more traditional content-based models. IISER Pune offers a 5-year BS MS dual degree program, Integrated-PhD programs for bachelor level students, and PhD programs for Master's level students. In the shortest time possible, we have set up one of the best-equipped research facilities in the country at IISER Pune. Faculty members are carefully chosen for their research accomplishments, promise and teaching proficiency. While the identity of individual disciplines is maintained, we have physicists, chemists, biologists and mathematicians working shoulder to shoulder without any departmental (or compartmental) structure. One of the greatest strengths of IISER Pune is this interdisciplinary ambiance. At IISER Pune, we also aim to integrate natural sciences with social sciences and humanities in knowledge production and education. The whole ambiance is very academic and energy levels are high. There is a great enthusiasm amongst faculty members and students to pursue high quality research: together, they investigate questions in science that lie beyond the boundaries of conventional thinking. Scanning Electron Microscopy image of cadmium sulphide nanotubes (Image: Shouvik Datta's Group) G AMBIKA Professor [email protected] G Ambika received her PhD in Nonlinear Dynamics from Cochin University of Science & Technology, Cochin, India. She worked as a Research Associate for five years and then as Reader in Physics in Maharajas College, Cochin before joining IISER Pune in August 2006. NONLINEAR DYNAMICS AND COMPLEX SYSTEMS Natural systems are highly complex since their dynamics involve a large number of units with highly nonlinear interactions among themselves and with the environment. We analyze how the dynamics of such connected systems can be suppressed due to interaction with environment. We propose that this mechanism provides for the first time a physical model for Alzheimer's disease, where due to the induced activity on certain proteins called amyloid beta, the normal neuronal activity will be suppressed. We have recently introduced a novel coupling scheme for synchronizing nonlinear chaotic systems where the delay in coupling is varied within a reset interval. This has lead to a novel error dynamics and Lyapunov exponent computations. This introduces a new method for synchronizing time delay systems and has relevance in applications like secure communication. We have developed methods for quantifying complexity with relevant measures computed from the observed time series. A few parameters identified to characterize the Multifractal spectrum serve as better quantifiers for diagnostic purposes for data like EEG and ECG. A complete analysis of the light curves from all the states of the black hole system, GRS States of GRS 1915+105 1915+105 is done using these quantifiers. black hole system SELECTED PUBLICATIONS Harikrishnan, K.P., Mishra, R. and Ambika, G. (2012). Revisiting the box counting algorithm for the correlation dimension analysis of hyperchaotic time series. Communications in Nonlinear Science & Numerical Simulation 17:263-276. Harikrishnan, K.P., Mishra, R. and Ambika, G. (2011). Nonlinear time series analysis of the light curves from the black hole system GRS 1915+105-. Research in Astronomy & Astrophysics 11:71-90. Ambika, G. and Amritkar, R.E. (2011). Synchronizing time delay systems using variable delay in coupling. Chaos, Solitons & Fractals 44:1035-1042. Resmi, V., Ambika, G. and Amritkar, R.E. (2011). General mechanism for amplitude death in coupled systems. Physical Review E 84:046212. Harikrishnan, K.P., Misra, R., Ambika, G. and Amritkar, R.E. (2010). Parametric characterisation of a chaotic attractor using two scale Cantor measure. Physica D D239:420-427. Resmi, V., Ambika, G. and Amritkar, R.E. (2010). Synchronized states in chaotic systems coupled indirectly through a dynamic environment. Physical Review E 81:046216. Ambika, G. and Amritkar, R.E. (2009). Anticipatory synchronization with variable time delay and reset. Physical Review E 79:056206. Harikrishnan, K.P., Misra, R., Ambika, G. and Amritkar, R.E. (2009). Computing the multifractal spectrum from time series: An algorithmic approach. Chaos 19:043129. 1 SUDARSHAN ANANTH Associate Professor Head, Max Planck Partner Group [email protected] Sudarshan Ananth received his BSc degree from Loyola College and MSc from Indian Institute of Technology (IIT) Madras, India. He obtained PhD from the University of Florida, USA in 2005. Dr Ananth was subsequently a Junior Scientist at the Max Planck Institute for Gravitational Physics for two years before moving to IISER Pune in 2008. THEORETICAL PARTICLE PHYSICS According to our current understanding, there are four fundamental forces in Nature. Quantum Yang-Mills theory provides a remarkably accurate description of three – electromagnetic, weak and strong – of these four forces. The fourth force, gravity, is classically well understood thanks to the general theory of relativity. However, we still lack a consistent quantum mechanical description of the gravitational force. My research is aimed at understanding this apparent incompatibility between general relativity and quantum mechanics. Themes of current interest include 1. Efficient methods to compute correlation functions in conformal field theories. 2. Origin of divergences in quantum field theories. 3. Perturbative relations between gravity and gauge theory: using perturbative ties between gravity and Yang-Mills theory to understand ultra-violet behavior in gravity theories. 4. Ultra-violet properties of N=8 supergravity. SELECTED PUBLICATIONS Ananth, S., Kovacs, S. and Parikh, S. (2012). Gauge-invariant correlation functions in light-cone superspace. Journal of High Energy Physics, 1205:096. Ananth, S., Kovacs, S. and Parikh, S. (2011). A manifestly MHV Lagrangian for N=4 Yang-Mills. Journal of High Energy Physics (JHEP) 1105:051. Ananth, S. (2010). LC_2 formulation of supergravity. Journal of High Energy Physics (JHEP) 1002:001. Ananth, S. (2010). Gravity and Yang-Mills theory, Special Issue (GRF) - International Journal of Modern Physics D 19:2379. Ananth, S. (2008). The quintic interaction vertex in light-cone gravity. Physics Letters B 664:219. Ananth, S., Kovacs, S. and Shimada, H. (2007). Proof of ultra-violet finiteness for a planar non-supersymmetric Yang-Mills theory. Nuclear Physics B 783:227. 2 RAMANA MANU ATHREYA Associate Professor [email protected] Ramana Athreya obtained PhD from the National Centre for Radio Astrophysics (NCRA, TIFR), Pune, India in 1996. Following postdoctoral fellowships at the Institute of Astrophysics, Paris (1998) and the European Southern Observatory, Chile (1999), and a faculty position at NCRA, Pune (2003), he joined IISER Pune in 2009. He is a Trustee of two conservation NGOs: Kaati Trust (Pune) and Eco-Systems India (Guwahati), and is a member of the Arunachal Pradesh State Wildlife Advisory Board. 1. ASTROPHYSICS AT LOW RADIO FREQUENCIES I focus on astrophysical phenomena which are best studied at low radio frequencies, largely with the Giant Metre- wave Radio Telescope (GMRT) near Pune. These include an eclectic mixture of radio halos and relics in galaxy clusters, AGN feedback in galaxy clusters, absorption line spectra of quasars and other objects in the early Universe, steep spectrum radio sources, pulsars, etc. In the past I have worked on gravitational lensing, and radio galaxies and Lyman alpha galaxies at high redshift. Recently, I developed a technique to excise man-made radio frequency interference from radio telescope data which has resulted in a significant improvement in the quality of imaging. SELECTED PUBLICATIONS Curran, S.J., Tzanavaris, P., Darling, J.K., Whiting, M.T., Webb, J.K., Bignell, C., Athreya, R. and Murphy, M.T. (2010). New searches for HI 21 cm in damped Lyman α absorption systems. Monthly Notices of the Royal Astronomical Society 402:35-45. Athreya, R.M. (2009). A new approach to mitigation of radio frequency interference in interferometric data. Astrophysical Journal 696:885. Giacintucci, S., Venturi, T., Macario, G., Dallacasa, D., Brunetti, G., Markevitch, M., Cassano, R., Bardelli, S. and Athreya, R. (2008). Shock acceleration as origin of the radio relic in A 521? Astronomy & Astrophysics 486:347-358. 2. BIOLOGICAL DIVERSITY: RESEARCH AND CONSERVATION I am interested in research on and conservation of the rich biological diversity in India. I initiated and lead the Eaglenest Biodiversity Project, which is inventorying the fauna of Eaglenest sanctuary in Arunachal Pradesh and helping in its conservation. My research in this field involves

View Full Text

Details

  • File Type
    pdf
  • Upload Time
    -
  • Content Languages
    English
  • Upload User
    Anonymous/Not logged-in
  • File Pages
    119 Page
  • File Size
    -

Download

Channel Download Status
Express Download Enable

Copyright

We respect the copyrights and intellectual property rights of all users. All uploaded documents are either original works of the uploader or authorized works of the rightful owners.

  • Not to be reproduced or distributed without explicit permission.
  • Not used for commercial purposes outside of approved use cases.
  • Not used to infringe on the rights of the original creators.
  • If you believe any content infringes your copyright, please contact us immediately.

Support

For help with questions, suggestions, or problems, please contact us