Institution
Tata Institute of Fundamental Research
Education•Mumbai, 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.
Topics: Magnetization, Large Hadron Collider, Galaxy, Higgs boson, Lepton
Papers published on a yearly basis
Papers
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TL;DR: A statistical combination of several searches for the electroweak production of charginos and neutralinos is presented in this article, where a targeted analysis requiring three or more charged leptons (electrons or muons) is presented, focusing on the challenging scenario in which the difference in mass between the two least massive neutralino is approximately equal to the mass of the Z boson.
Abstract: A statistical combination of several searches for the electroweak production of charginos and neutralinos is presented. All searches use proton-proton collision data at $ \sqrt{s}=13 $ TeV, recorded with the CMS detector at the LHC in 2016 and corresponding to an integrated luminosity of 35.9 fb$^{−1}$. In addition to the combination of previous searches, a targeted analysis requiring three or more charged leptons (electrons or muons) is presented, focusing on the challenging scenario in which the difference in mass between the two least massive neutralinos is approximately equal to the mass of the Z boson. The results are interpreted in simplified models of chargino-neutralino or neutralino pair production. For chargino-neutralino production, in the case when the lightest neutralino is massless, the combination yields an observed (expected) limit at the 95% confidence level on the chargino mass of up to 650 (570) GeV, improving upon the individual analysis limits by up to 40 GeV. If the mass difference between the two least massive neutralinos is approximately equal to the mass of the Z boson in the chargino-neutralino model, the targeted search requiring three or more leptons obtains observed and expected exclusion limits of around 225 GeV on the second neutralino mass and 125 GeV on the lightest neutralino mass, improving the observed limit by about 60 GeV in both masses compared to the previous CMS result. In the neutralino pair production model, the combined observed (expected) exclusion limit on the neutralino mass extends up to 650–750 (550–750) GeV, depending on the branching fraction assumed. This extends the observed exclusion achieved in the individual analyses by up to 200 GeV. The combined result additionally excludes some intermediate gaps in the mass coverage of the individual analyses.
167 citations
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Arizona State University1, University of Washington2, University of Melbourne3, Curtin University4, Brown University5, Rhodes University6, Harvard University7, Australian National University8, Massachusetts Institute of Technology9, University of California, Berkeley10, University of Sydney11, University of Toronto12, Victoria University of Wellington13, University of Wisconsin–Milwaukee14, University of Michigan15, Commonwealth Scientific and Industrial Research Organisation16, Tata Institute of Fundamental Research17, ASTRON18, Raman Research Institute19, National Radio Astronomy Observatory20, University of Western Australia21
TL;DR: In this article, the authors introduce several novel analysis techniques, such as cable reflection calibration, hyper-resolution gridding kernels, diffuse foreground model subtraction, and quality control methods, and incorporate the new techniques into a deep integration of 32 hours of MWA data.
Abstract: The Murchison Widefield Array (MWA) has collected hundreds of hours of Epoch of Reionization (EoR) data andnow faces the challenge of overcoming foreground and systematic contamination to reduce the data to acosmological measurement. We introduce several novel analysis techniques, such as cable reflection calibration,hyper-resolution gridding kernels, diffuse foreground model subtraction, and quality control methods. Each changeto the analysis pipeline is tested against a two-dimensional power spectrum figure of merit to demonstrateimprovement. We incorporate the new techniques into a deep integration of 32 hours of MWA data. This data set isused to place a systematic-limited upper limit on the cosmological power spectrum of Δ2 ≤ 2.7×104 mK2 at k =0.27 h Mpc-1 and z = 7.1, consistent with other published limits, and a modest improvement (factor of 1.4) overprevious MWA results. From this deep analysis, we have identified a list of improvements to be made to our EoRdata analysis strategies. These improvements will be implemented in the future and detailed in upcomingpublications.
167 citations
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TL;DR: In this paper, a method for classifying rational conformal field theories in terms of the differential equation satisfied by their characters is proposed, which is based on the notion of rational conformality.
167 citations
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TL;DR: In a globally supersymmetric gauge theory with two distinct mass scales, the possible limitation on the gauge hierarchy due to the structure of the loop-corrected Higgs potential is shown to be absent.
166 citations
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TL;DR: A search for exotic unstable neutral and charged heavy leptons was performed with the L3 detector at LEP as discussed by the authors, but no evidence for their existence was found and lower limits on their masses were set.
166 citations
Authors
Showing all 7857 results
Name | H-index | Papers | Citations |
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Pulickel M. Ajayan | 176 | 1223 | 136241 |
Suvadeep Bose | 154 | 960 | 129071 |
Subir Sarkar | 149 | 1542 | 144614 |
Sw. Banerjee | 146 | 1906 | 124364 |
Dipanwita Dutta | 143 | 1651 | 103866 |
Ajit Kumar Mohanty | 141 | 1124 | 93062 |
Tariq Aziz | 138 | 1646 | 96586 |
Andrew Mehta | 137 | 1444 | 101810 |
Suchandra Dutta | 134 | 1265 | 87709 |
Kajari Mazumdar | 134 | 1295 | 94253 |
Bobby Samir Acharya | 133 | 1121 | 100545 |
Gobinda Majumder | 133 | 1523 | 87732 |
Eric Conte | 132 | 1206 | 84593 |
Prashant Shukla | 131 | 1341 | 85287 |
Alessandro Montanari | 131 | 1387 | 93071 |