09:00 to 09:30 |
A. Dhar, R. Gopakumar, S. Vishveshwara |
Inaugural talks |
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09:00 to 11:40 |
Rajesh Gopakumar (ICTS-TIFR, India) |
Session Chair |
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09:30 to 10:30 |
Michael Berry (University of Bristol, UK) |
Quantum chaology and the singing of the primes Although envisaged by Einstein in 1917, it was only in the 1970s that the implications for quantum mechanics of chaos in the classical limiting dynamics was recognised as a problem. The solution emerged from several directions. There is no sharp quantum-classical boundary; instead, rich borderland physics. I will concentrate on the arrangement of energy levels. Semiclassical asymptotics, in the form of Gutzwiller’s trace formula, gives the quantum spectral density as a sum over classical periodic orbits. Long periodic orbits enjoy a universal phase space democracy, leading to statistics between closelying levels described by random-matrix theory (RMT). Short orbits give nonuniversal correlations between more distant levels, and the failure of RMT. A bonus was the discovery that the Riemann zeros share the same statistics: RMT and its failure. If time permits, I will discuss wavefunctions, for which semiclassical asymptotics implies gaussian random functions with a particular spatial correlation, occasionally decorated by scars from unstable periodic orbits. For many-body quantum chaos, large dimension D will involve asymptotics additional to semiclassical, possibly clashing (cf P W Anderson, ‘More is different’).
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11:00 to 11:40 |
Ashoke Sen (ICTS-TIFR, India) |
Classical Gravitational Wave Tails from Quantum Soft Theorem If a set of massive objects collide in space and the fragments disperse, possibly forming black holes, then this process will emit gravitational waves. Computing the detailed gravitational wave-form associated with this process is a complicated problem, not only due to the non-linearity of gravity but also due to the fact that during the collision and subsequent fragmentation the objects could undergo complicated non-gravitational interactions. Nevertheless some results in quantum theory of gravity, known as soft graviton theorems, determine the power law fall-off of the wave-form at late and early times, including logarithmic corrections, in terms of only the momenta of the incoming and outgoing objects without any reference to what transpired during the collision. In this talk I shall explain the results and very briefly outline the derivation of these results.
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11:40 to 12:40 |
Peter Sarnak (Institute for Advanced Study and Princeton University, USA) |
Arithmetic Quantum Chaos (Infosys Science Foundation Lecture) Understanding the semiclassical limit of the quantization of even the simplest classically chaotic Hamiltonian, proved to be problematic from the inception of quantum mechanics 100 years ago. Arithmetically defined such systems provide instances for which this limit can be analyzed mathematically using central tools from number theory and homogeneous dynamics.As such these can be thought of as "solvable models ". We review some of the many developments for these quantizations.
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14:30 to 15:50 |
P Ajith (ICTS-TIFR, India) |
Session Chair |
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14:30 to 15:10 |
Nathaniel Craig (University of California, Santa Barbara, USA) |
The Quantum Frontiers of Particle Physics The 2012 discovery of the Higgs boson marked the completion of the Standard Model of particle physics, tempting many to echo Michelson’s 1894 declaration that "most of the grand underlying principles have been firmly established...the future truths of Physical Science are to be looked for in the sixth place of decimals.” But just as quantum mechanics upended Michelson’s dictum in the 20th century, so too does it promise to transform particle physics in the 21st century. In this talk, I’ll highlight two of the central questions facing particle physics — the origin of mass and the nature of matter in the universe — and emphasize the potential for quantum mechanics, quantum computation, and quantum sensing to provide the answers.
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15:10 to 15:50 |
Urbasi Sinha (Raman Research Institute, Bengaluru, India) |
Light, Camera, Action! Quantum mechanics is a cornerstone of modern physics. Just as the 19th century was called the Machine Age and the 20th century the Information Age, the 21st century promises to go down in history as the Quantum Age. Quantum Computing promises unprecedented speed in solving certain classes of problems while Quantum Cryptography promises information theoretically secure communications. In this talk, I will discuss the world of single and entangled photons and also discuss ongoing work towards secure quantum communications, quantum information and precision experimental tests of principles of quantum mechanics in our Quantum Information and Computing lab at the Raman Research Institute, Bengaluru, India. I will end with our broad vision for the future, which includes establishment of long distance secure quantum communications in India and beyond involving satellite based, fibre based as well as quantum memory and repeater network based approaches towards the global quantum internet.
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16:20 to 17:00 |
Herbert Spohn (Technische Universität München, Germany) |
Session Chair |
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16:20 to 17:00 |
G. Baskaran (IITMadras, Perimeter Institute, Matscience) |
Boson Bloom In 1924, Bose communicated a derivation of the Planck distribution, to Einstein, where Bose introduced a key notion of indistinguishability of photon quanta. This was a turning point in the history of quantum mechanics. Bose's article is considered the fourth most important article, in the development of quantum mechanics, following those of Planck, Einstein and Niels Bohr. It was Dirac, who coined the names Bosons and Fermions. We present a brief historical account of Bose’s discovery, followed by a bird’s eye view of the impacts of boson bloom and Bose-Einstein condensation in modern science and technology.
[1] Boson Bloom, G. Baskaran and A. May, J. Physics B, 57, 142001 (2024)
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17:00 to 18:00 |
S.N. Bose Corridor Dedication |
Screening of the film "Dear Master", interaction with Director - Ms. Subha Das Mollick |
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