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Institution

Indian Institute of Technology Guwahati

EducationGuwahati, Assam, India
About: Indian Institute of Technology Guwahati is a education organization based out in Guwahati, Assam, India. It is known for research contribution in the topics: Adsorption & Catalysis. The organization has 6933 authors who have published 17102 publications receiving 257351 citations.


Papers
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Journal ArticleDOI
TL;DR: Mild reaction conditions, shorter reaction times, high efficiencies, cost-effectiveness, and facile isolation of the desired products make the present methodology a practical alternative.

164 citations

Journal ArticleDOI
TL;DR: In this paper, the sign and magnitude of the third-order nonlinearity from the closed aperture Z-scan data were evaluated while the nonlinear absorption properties were assessed using the open aperture data.

164 citations

Journal ArticleDOI
TL;DR: In this article, the authors presented the Futoshiki puzzle pattern for the arrangement of the modules of a PV array under partial shading condition, ensuring the enhancement of the power generation with respect to totally crossed tired (TCT) structure.
Abstract: As per energy efficiency of a photovoltaic (PV) system is concerned, partial shading is an important issue. Under partial shading condition, the modules of a PV array receive different levels of solar irradiation, so the power generation of a PV system decreases. The power–voltage characteristic of a partially shaded PV array contains multiple local maxima, and the global maximum power point is one of them. The losses in a PV array depend on the shading pattern and the physical location of shaded modules. This paper presents the Futoshiki puzzle pattern for the arrangement of the modules of a PV array under partial shading condition, ensuring the enhancement of the power generation with respect to totally crossed tired (TCT) structure. In this method, the physical locations of modules in a TCT structure PV array are rearranged without changing the electrical connection of the modules. A comparison between the power generation in TCT and Futoshiki puzzle pattern configuration is presented. It is demonstrated that the power generated by a PV array in the Futoshiki configuration method is enhanced, and mismatch loss (ML) is minimized under different shading patterns by theoretical, simulation, and experimental results.

163 citations

Journal ArticleDOI
Rathin Adhikari1, Matteo Agostini, N. Anh Ky2, N. Anh Ky3, T. Araki4, Maria Archidiacono5, M. Bahr6, J. Baur7, J. Behrens8, Fedor Bezrukov9, P. S. Bhupal Dev10, Debasish Borah11, Alexey Boyarsky12, A. de Gouvea13, C. A. de S. Pires14, H. J. de Vega15, Alex G. Dias16, P. Di Bari17, Z. Djurcic18, Kai Dolde19, H. Dorrer20, M. Durero7, O. Dragoun, Marco Drewes21, Guido Drexlin19, Ch. E. Düllmann20, Klaus Eberhardt20, Sergey Eliseev22, Christian Enss23, Nick Evans, A. Faessler24, Pavel Filianin22, V. Fischer7, Andreas Fleischmann23, Joseph A. Formaggio25, Jeroen Franse12, F.M. Fraenkle19, Carlos S. Frenk26, George M. Fuller27, L. Gastaldo23, Antonella Garzilli12, Carlo Giunti, Ferenc Glück19, Maury Goodman18, M. C. Gonzalez-Garcia28, Dmitry Gorbunov29, Dmitry Gorbunov30, Jan Hamann31, Volker Hannen8, Steen Hannestad5, Steen Honoré Hansen32, C. Hassel23, Julian Heeck33, F. Hofmann22, T. Houdy34, T. Houdy7, A. Huber19, Dmytro Iakubovskyi35, Aldo Ianni36, Alejandro Ibarra21, Richard Jacobsson37, Tesla E. Jeltema38, Josef Jochum24, Sebastian Kempf23, T. Kieck20, M. Korzeczek7, M. Korzeczek19, V. N. Kornoukhov39, Tobias Lachenmaier24, Mikko Laine40, Paul Langacker41, Thierry Lasserre, J. Lesgourgues42, D. Lhuillier7, Yufeng Li43, W. Liao44, A.W. Long45, Michele Maltoni46, Gianpiero Mangano, Nick E. Mavromatos47, Nicola Menci48, Alexander Merle22, Susanne Mertens49, Susanne Mertens19, Alessandro Mirizzi50, Alessandro Mirizzi51, Benjamin Monreal6, A. A. Nozik29, A. A. Nozik30, Andrii Neronov52, V. Niro46, Yu. N. Novikov53, L. Oberauer21, Ernst W. Otten20, Nathalie Palanque-Delabrouille7, Marco Pallavicini54, V. S. Pantuev30, Emmanouil Papastergis55, Stephen J. Parke56, Silvia Pascoli26, Sergio Pastor57, Amol V. Patwardhan27, Apostolos Pilaftsis10, D. C. Radford58, P. C.-O. Ranitzsch8, O. Rest8, Dean J. Robinson59, P. S. Rodrigues da Silva14, Oleg Ruchayskiy35, Oleg Ruchayskiy60, Norma G. Sanchez61, Manami Sasaki24, Ninetta Saviano26, Ninetta Saviano20, Aurel Schneider62, F. Schneider20, T. Schwetz19, S. Schönert21, S. Scholl24, Francesco Shankar17, Robert Shrock28, N. Steinbrink8, Louis E. Strigari63, F. Suekane64, B. Suerfu65, R. Takahashi66, N. Thi Hong Van2, Igor Tkachev30, Maximilian Totzauer22, Y. Tsai67, Christopher George Tully65, Kathrin Valerius19, José W. F. Valle57, D. Vénos, Matteo Viel48, M. Vivier7, Mei-Yu Wang63, Ch. Weinheimer8, Klaus Wendt20, Lindley Winslow25, Joachim Wolf19, Michael Wurm20, Z. Xing43, Shun Zhou43, Kai Zuber68 
Jamia Millia Islamia1, Vietnam Academy of Science and Technology2, Hanoi University of Science3, Saitama University4, Aarhus University5, University of California, Santa Barbara6, Commissariat à l'énergie atomique et aux énergies alternatives7, University of Münster8, University of Connecticut9, University of Manchester10, Indian Institute of Technology Guwahati11, Leiden University12, Northwestern University13, Federal University of Paraíba14, Centre national de la recherche scientifique15, Universidade Federal do ABC16, University of Southampton17, Argonne National Laboratory18, Karlsruhe Institute of Technology19, University of Mainz20, Technische Universität München21, Max Planck Society22, Heidelberg University23, University of Tübingen24, Massachusetts Institute of Technology25, Durham University26, University of California, San Diego27, C. N. Yang Institute for Theoretical Physics28, Moscow Institute of Physics and Technology29, Russian Academy of Sciences30, University of Sydney31, University of Copenhagen32, Université libre de Bruxelles33, Paris Diderot University34, Niels Bohr Institute35, Estácio S.A.36, CERN37, University of California, Santa Cruz38, Institute on Taxation and Economic Policy39, University of Bern40, Institute for Advanced Study41, RWTH Aachen University42, Chinese Academy of Sciences43, East China University of Science and Technology44, University of Chicago45, Autonomous University of Madrid46, King's College London47, INAF48, Lawrence Berkeley National Laboratory49, Istituto Nazionale di Fisica Nucleare50, University of Bari51, University of Geneva52, Petersburg Nuclear Physics Institute53, University of Genoa54, Kapteyn Astronomical Institute55, Fermilab56, Spanish National Research Council57, Oak Ridge National Laboratory58, University of California, Berkeley59, École Polytechnique Fédérale de Lausanne60, University of Paris61, University of Zurich62, Mitchell Institute63, Tohoku University64, Princeton University65, Shimane University66, University of Maryland, College Park67, Dresden University of Technology68
TL;DR: A comprehensive review of keV-scale neutrino Dark Matter can be found in this paper, where the role of active neutrinos in particle physics, astrophysics, and cosmology is reviewed.
Abstract: We present a comprehensive review of keV-scale sterile neutrino Dark Matter, collecting views and insights from all disciplines involved - cosmology, astrophysics, nuclear, and particle physics - in each case viewed from both theoretical and experimental/observational perspectives. After reviewing the role of active neutrinos in particle physics, astrophysics, and cosmology, we focus on sterile neutrinos in the context of the Dark Matter puzzle. Here, we first review the physics motivation for sterile neutrino Dark Matter, based on challenges and tensions in purely cold Dark Matter scenarios. We then round out the discussion by critically summarizing all known constraints on sterile neutrino Dark Matter arising from astrophysical observations, laboratory experiments, and theoretical considerations. In this context, we provide a balanced discourse on the possibly positive signal from X-ray observations. Another focus of the paper concerns the construction of particle physics models, aiming to explain how sterile neutrinos of keV-scale masses could arise in concrete settings beyond the Standard Model of elementary particle physics. The paper ends with an extensive review of current and future astrophysical and laboratory searches, highlighting new ideas and their experimental challenges, as well as future perspectives for the discovery of sterile neutrinos.

163 citations

Journal ArticleDOI
TL;DR: In this paper, a nano-composite polymeric scaffolds with controllable pore size and mechanical strength was synthesized, which served dual functions of providing mechanical strength and antimicrobial activity.

162 citations


Authors

Showing all 7128 results

NameH-indexPapersCitations
Jasvinder A. Singh1762382223370
Dipanwita Dutta1431651103866
Sanjay Gupta9990235039
Santosh Kumar80119629391
Subrata Ghosh7884132147
Rishi Raj7856922423
B. Bhuyan7365821275
Ravi Shankar6667219326
Ashutosh Sharma6657016100
Gautam Biswas6372116146
Sam P. de Visser6225613820
Surendra Nadh Somala6114428273
Manish Kumar61142521762
Mihir Kumar Purkait572679812
Ajaikumar B. Kunnumakkara5720120025
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Performance
Metrics
No. of papers from the Institution in previous years
YearPapers
2023118
2022365
20212,032
20201,947
20191,866
20181,647