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Institution

Tata Institute of Fundamental Research

EducationMumbai, Maharashtra, India
About: Tata Institute of Fundamental Research is a education organization based out in Mumbai, Maharashtra, India. It is known for research contribution in the topics: Magnetization & Large Hadron Collider. The organization has 7786 authors who have published 21742 publications receiving 622368 citations. The organization is also known as: TIFR.


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Journal ArticleDOI
TL;DR: This study demonstrates near-100% light absorption and increased x-ray emission from dense plasmas created on solid surfaces with a periodic sub-lambda structure and offers a definite, quantitative way forward for optimizing and understanding the absorption process.
Abstract: We demonstrate near-100% light absorption and increased x-ray emission from dense plasmas created on solid surfaces with a periodic sub-lambda structure. The efficacy of the structure-induced surface plasmon resonance, responsible for enhanced absorption, is directly tested at the highest intensities to date (3 x 10{15} W cm{-2}) via systematic, correlated measurements of absorption and x-ray emission. An analytical grating model as well as 2D particle-in-cell simulations conclusively explain our observations. Our study offers a definite, quantitative way forward for optimizing and understanding the absorption process.

116 citations

Journal ArticleDOI
A. Kumar1, A M Vinod Kumar2, Abhik Jash3, Abhik Jash4, Ajit Kumar Mohanty5, Ajit Kumar Mohanty3, Aleena Chacko6, Ali Ajmi3, Ali Ajmi7, Ambar Ghosal3, Ambar Ghosal4, Amina Khatun3, Amitava Raychaudhuri8, Amol Dighe9, Animesh Chatterjee3, Animesh Chatterjee10, Ankit Gaur11, Anushree Ghosh10, Anushree Ghosh3, Ashok Kumar11, A. Redij9, B. Satyanarayana9, B. S. Acharya9, Brajesh C Choudhary11, C. Ranganathaiah12, C. D. Ravikumar2, Chandan Gupta13, Chandan Gupta3, D. Indumathi3, Daljeet Kaur11, Debasish Majumdar4, Debasish Majumdar3, D. Samuel9, Deepak Tiwari3, Deepak Tiwari10, G Rajasekaran3, Gautam Gangopadhyay8, Gobinda Majumder9, H. B. Ravikumar12, Jasvinder A. Singh1, J. Shahi1, J. Libby6, Jyotsna Singh14, K. Raveendrababu3, K. Raveendrababu6, K K Meghna3, K. R. Rebin6, Kamalesh Kar3, Kamalesh Kar4, K. Bhattacharya9, Lalit Mohan Pant3, Lalit Mohan Pant5, M. Sajjad Athar15, M. V. N. Murthy3, Manzoor A. Malik16, Naimuddin11, Mohammad Salim15, Monojit Ghosh13, Moon Moon Devi9, Moon Moon Devi3, N.K. Mondal9, Nayana Majumdar4, Nayana Majumdar3, N Sinha3, N. Dash5, N. Dash3, Pomita Ghoshal13, Poonam Mehta17, Prafulla Kumar Behera6, R. Kanishka1, R. Gandhi3, R. Gandhi10, Rajesh Ganai18, Rajesh Ganai3, Rashid Hasan15, S. Krishnaveni12, S. M. Lakshmi3, S. K. Singh15, S.S.R. Inbanathan19, S. Uma Sankar7, Sadiq Jafer6, Saikat Biswas18, Saikat Biswas3, Sanjeev Kumar11, Sanjib Kumar Agarwalla3, Sandhya Choubey3, Sandhya Choubey10, Satyajit Saha3, Satyajit Saha4, Shakeel Ahmed15, S. P. Behera3, S. P. Behera5, Srubabati Goswami13, Subhasis Chattopadhyay3, Subhasis Chattopadhyay18, Sudeb Bhattacharya3, Sudeb Bhattacharya4, Sw. Banerjee9, Sudeshna Dasgupta9, Sumanta Pal3, Supratik Mukhopadhyay4, Supratik Mukhopadhyay3, Sushant K. Raut13, S. Bose3, S. Bose4, Swapna Mahapatra20, T.K. Ghosh3, T.K. Ghosh18, Tarak Thakore9, V K S Kashyap3, V K S Kashyap5, V. S. Subrahmanyam21, V. Singh21, V.B. Chandratre3, V.B. Chandratre5, Vipin Bhatnagar1, V. M. Datar5, V. M. Datar9, W. Bari16, Y. P. Viyogi3, Y. P. Viyogi18 
26 Apr 2017-Pramana
TL;DR: In this paper, the authors presented the physics potential of the ICAL detector as obtained from realistic detector simulations and gave the expected physics reach of the detector with 10 years of runtime.
Abstract: The upcoming 50 kt magnetized iron calorimeter (ICAL) detector at the India-based Neutrino Observatory (INO) is designed to study the atmospheric neutrinos and antineutrinos separately over a wide range of energies and path lengths. The primary focus of this experiment is to explore the Earth matter effects by observing the energy and zenith angle dependence of the atmospheric neutrinos in the multi-GeV range. This study will be crucial to address some of the outstanding issues in neutrino oscillation physics, including the fundamental issue of neutrino mass hierarchy. In this document, we present the physics potential of the detector as obtained from realistic detector simulations. We describe the simulation framework, the neutrino interactions in the detector, and the expected response of the detector to particles traversing it. The ICAL detector can determine the energy and direction of the muons to a high precision, and in addition, its sensitivity to multi-GeV hadrons increases its physics reach substantially. Its charge identification capability, and hence its ability to distinguish neutrinos from antineutrinos, makes it an efficient detector for determining the neutrino mass hierarchy. In this report, we outline the analyses carried out for the determination of neutrino mass hierarchy and precision measurements of atmospheric neutrino mixing parameters at ICAL, and give the expected physics reach of the detector with 10 years of runtime. We also explore the potential of ICAL for probing new physics scenarios like CPT violation and the presence of magnetic monopoles.

116 citations

Journal ArticleDOI
TL;DR: In this paper, the authors used the Hubble Space Telescope Cosmic Origins Spectrograph and Wide-Field Camera 3 observations of SN 1993J from 2012, at which point the flux from the SN had faded sufficiently to potentially measure the UV continuum properties from the putative companion.
Abstract: The Type IIb supernova (SN) 1993J is one of only a few stripped-envelope SNe with a progenitor star identified in pre-explosion images. SN IIb models typically invoke H envelope stripping by mass transfer in a binary system. For the case of SN 1993J, the models suggest that the companion grew to 22 solar mass and became a source of ultraviolet (UV) excess. Located in M81, at a distance of only 3.6 Mpc, SN 1993J offers one of the best opportunities to detect the putative companion and test the progenitor model. Previously published near-UV spectra in 2004 showed evidence for absorption lines consistent with a hot (B2 Ia) star, but the field was crowded and dominated by flux from the SN. Here we present Hubble Space Telescope Cosmic Origins Spectrograph and Wide-Field Camera 3 observations of SN 1993J from 2012, at which point the flux from the SN had faded sufficiently to potentially measure the UV continuum properties from the putative companion. The resulting UV spectrum is consistent with contributions from both a hot B star and the SN, although we cannot rule out line-of-sight coincidences.

116 citations

Journal ArticleDOI
A. Bozek1, M. Rozanska1, I. Adachi, Hiroaki Aihara2, K. Arinstein3, K. Arinstein4, V.M. Aulchenko3, V.M. Aulchenko4, T. Aushev5, Tariq Aziz6, A. M. Bakich7, V. Bhardwaj8, M. Bischofberger9, A.E. Bondar3, A.E. Bondar4, M. Bračko10, T. E. Browder, Y. Chao11, A. Chen12, B. G. Cheon13, I. S. Cho14, K. S. Choi14, Y. Choi15, J. Dalseno16, Z. Doležal17, Z. Drasal17, A. Drutskoy18, W. Dungel19, S.I. Eidelman4, S.I. Eidelman3, P. Goldenzweig18, B. Golob20, H. Ha21, Kazuhiko Hara22, Yoji Hasegawa23, H. Hayashii9, T. Higuchi, Yasuyuki Horii24, Y. Hoshi25, W. S. Hou11, H. J. Hyun26, T. Iijima22, K. Inami22, M. Iwabuchi14, Y. Iwasaki, N. J. Joshi6, Ju Hwan Kang, P. Kapusta1, H. Kawai27, T. Kawasaki28, H. Kichimi, C. Kiesling16, H. O. Kim26, Jung-Hyun Kim29, M. J. Kim26, S. K. Kim30, Y. J. Kim31, B. R. Ko21, S. Korpar10, P. Krišan20, P. Krokovny, T. Kuhr32, T. Kumita33, A.S. Kuzmin4, A.S. Kuzmin3, Youngjoon Kwon, S. H. Kyeong14, M. J. Lee30, Soohyung Lee21, J. Li, D. Liventsev, R. Louvot5, A. Matyja1, S. McOnie7, H. Miyata28, Y. Miyazaki22, R. Mizuk, G. B. Mohanty6, E. Nakano34, M. Nakao, H. Nakazawa12, S. Neubauer32, S. Nishida, O. Nitoh35, T. Nozaki, S. Ogawa36, T. Ohshima22, S. Okuno37, S. L. Olsen30, W. Ostrowicz1, P. Pakhlov, G. Pakhlova, C. W. Park15, H. K. Park26, R. Pestotnik, Marko Petrič, L. E. Piilonen38, H. Sahoo, Y. Sakai, O. Schneider5, J. Schümann, C. Schwanda19, A. J. Schwartz18, K. Senyo22, J. G. Shiu11, B.A. Shwartz4, B.A. Shwartz3, R. Sinha, P. Smerkol, Andrey Sokolov, E. Solovieva, M. Starič, J. Stypula1, T. Sumiyoshi33, G. N. Taylor39, Y. Teramoto34, I. Tikhomirov, K. Trabelsi, S. Uehara, Yoshinobu Unno13, S. Uno, G. S. Varner, Kevin Varvell7, K. Vervink5, C. H. Wang40, M. Z. Wang11, P. Wang, Y. Watanabe37, Robin Wedd39, E. Won21, Bruce Yabsley7, Y. Yamashita, Vladimir Zhulanov3, Vladimir Zhulanov4, T. Zivko, A. Zupanc32 
TL;DR: In this article, the authors present measurements of B+ -> (D) over bar*(0)tau(+) v(tau) and B+ → (D), over bar (0) tau(+ v(Tau) v( tau) decays in a data sample of 657 x 10(6) B (B) over bars collected with the Belle detector at the KEKB asymmetric-energy e(+)e(-) collider.
Abstract: We present measurements of B+ -> (D) over bar*(0)tau(+) v(tau) and B+ -> (D) over bar (0)tau(+) v(tau) decays in a data sample of 657 x 10(6) B (B) over bar pairs collected with the Belle detector at the KEKB asymmetric-energy e(+)e(-) collider. We find 446(-56)(+58) B+ -> (D) over bar*(0)tau(+) v(tau) events with a significance of 8.1 standard deviations, and 146(-41)(+42) B+ -> (D) over bar (0)tau(+) v(tau) events with a significance of 3.5 standard deviations. The latter signal provides the first evidence for this decay mode. The measured branching fractions are B(B+ -> (D) over bar*(0)tau(+) v(tau)) = (2.12(-0.27)(+0.28) (stat) +/- 0.29(syst))% and B(B+ -> (D) over bar (0)tau(+) v(tau) ) = (0.77 +/- 0.22(stat) +/- 0.12(syst))%.

115 citations

Journal ArticleDOI
TL;DR: The two-state model for equilibrium unfolding has been critically evaluated in barstar by estimating the intramolecular distance distribution by time-resolved fluorescence resonance energy transfer (TR-FRET) methods, in which fluorescence decay kinetics are analyzed by the maximum entropy method (MEM).
Abstract: Coincidental equilibrium unfolding transitions observed by multiple structural probes are taken to justify the modeling of protein unfolding as a two-state, N ⇌ U, cooperative process. However, for many of the large number of proteins that undergo apparently two-state equilibrium unfolding reactions, folding intermediates are detected in kinetic experiments. The small protein barstar is one such protein. Here the two-state model for equilibrium unfolding has been critically evaluated in barstar by estimating the intramolecular distance distribution by time-resolved fluorescence resonance energy transfer (TR-FRET) methods, in which fluorescence decay kinetics are analyzed by the maximum entropy method (MEM). Using a mutant form of barstar containing only Trp 53 as the fluorescence donor and a thionitrobenzoic acid moiety attached to Cys 82 as the fluorescence acceptor, the distance between the donor and acceptor has been shown to increase incrementally with increasing denaturant concentration. Although other probes, such as circular dichroism and fluorescence intensity, suggest that the labeled protein undergoes two-state equilibrium unfolding, the TR-FRET probe clearly indicates multistate equilibrium unfolding. Native protein expands progressively through a continuum of native-like forms that achieve the dimensions of a molten globule, whose heterogeneity increases with increasing denaturant concentration and which appears to be separated from the unfolded ensemble by a free energy barrier.

115 citations


Authors

Showing all 7857 results

NameH-indexPapersCitations
Pulickel M. Ajayan1761223136241
Suvadeep Bose154960129071
Subir Sarkar1491542144614
Sw. Banerjee1461906124364
Dipanwita Dutta1431651103866
Ajit Kumar Mohanty141112493062
Tariq Aziz138164696586
Andrew Mehta1371444101810
Suchandra Dutta134126587709
Kajari Mazumdar134129594253
Bobby Samir Acharya1331121100545
Gobinda Majumder133152387732
Eric Conte132120684593
Prashant Shukla131134185287
Alessandro Montanari131138793071
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Performance
Metrics
No. of papers from the Institution in previous years
YearPapers
202322
2022128
2021939
20201,085
20191,100
20181,040