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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.


Papers
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Journal ArticleDOI
S. Uehara, T. Aushev1, A. M. Bakich2, K. Belous, V. Bhardwaj3, M. Bischofberger4, M. Bračko5, T. E. Browder, P. Chang6, A. Chen7, Po-Hsun Chen6, Byung Gu Cheon8, C. C. Chiang6, I. S. Cho9, S. K. Choi10, Y. Choi11, J. Dalseno12, A. Drutskoy13, S.I. Eidelman14, S.I. Eidelman15, D. Epifanov15, D. Epifanov14, M. Feindt16, N. Gabyshev14, N. Gabyshev15, H. Ha17, J. Haba, K. Hayasaka18, H. Hayashii4, Y. Hoshi19, W. S. Hou6, Y. B. Hsiung6, H. J. Hyun20, K. Inami18, R. Itoh, M. Iwabuchi9, M. Iwasaki21, Y. Iwasaki, N. J. Joshi22, J. H. Kang9, T. Kawasaki23, C. Kiesling12, H. J. Kim20, Jung-Hyun Kim11, Y. I. Kim20, Y. J. Kim24, B. R. Ko17, Peter Kodys25, S. Korpar5, P. Križan26, P. Krokovny, T. Kumita27, A.S. Kuzmin15, A.S. Kuzmin14, Y. J. Kwon9, S. H. Kyeong9, J. S. Lange28, M. J. Lee29, Sang Hoon Lee17, J. Li, Chang Liu30, Yang Liu18, D. Liventsev, R. Louvot1, A. Matyja31, S. McOnie2, K. Miyabayashi4, H. Miyata23, Y. Miyazaki18, R. Mizuk, R. Mussa, E. Nakano32, M. Nakao, H. Nakazawa7, Z. Natkaniec31, S. Nishida, O. Nitoh33, S. Ogawa34, T. Ohshima18, S. Okuno35, S. L. Olsen29, P. Pakhlov, G. Pakhlova, C. W. Park11, H. Park20, H. K. Park20, R. Pestotnik, Marko Petrič, L. E. Piilonen36, M. Röhrken16, Sunmin Ryu29, H. Sahoo, Y. Sakai, O. Schneider1, C. Schwanda37, M. E. Sevior38, M. Shapkin, C. P. Shen, J. G. Shiu6, B.A. Shwartz15, B.A. Shwartz14, Jasvinder A. Singh3, P. Smerkol, E. Solovieva, M. Starič, Y. Teramoto32, K. Trabelsi, Yoshinobu Unno8, S. Uno, Phillip Urquijo38, G. S. Varner, K. Vervink1, C. H. Wang39, P. Wang, Y. Watanabe35, Robin Wedd38, E. Won17, Bruce Yabsley2, Y. Yamashita, C. Z. Yuan, C. C. Zhang, T. Zivko, O. Zyukova14, O. Zyukova15 
TL;DR: The results of a search for a charmonium-like state produced in the process gamma gamma + omega J/psi in the 3.9-4.2 GeV = c(2) mass region were reported in this article.
Abstract: We report the results of a search for a charmoniumlike state produced in the process gamma gamma -> omega J/psi in the 3.9-4.2 GeV = c(2) mass region. We observe a significant enhancement, which is well described by a resonant shape with mass M = (3915 +/- 3 +/- 2_ MeV/c(2) and total width Gamma = (17 +/- 10 +/- 3) MeV. This enhancement may be related to one or more of the three charmoniumlike states so far reported in the 3.90-3.95 GeV= c(2) mass region.

119 citations

Journal ArticleDOI
TL;DR: It is concluded that the conductivity of the graphene sheet is lowered by impurity atoms and especially by lattice defects, because they result in weak localization effects at low temperatures.
Abstract: We investigate the structural, electronic, and transport properties of substitutional defects in SiC-graphene by means of scanning tunneling microscopy and magnetotransport experiments. Using ion incorporation via ultralow energy ion implantation, the influence of different ion species (boron, nitrogen, and carbon) can directly be compared. While boron and nitrogen atoms lead to an effective doping of the graphene sheet and can reduce or raise the position of the Fermi level, respectively, (12)C(+) carbon ions are used to study possible defect creation by the bombardment. For low-temperature transport, the implantation leads to an increase in resistance and a decrease in mobility in contrast to undoped samples. For undoped samples, we observe in high magnetic fields a positive magnetoresistance that changes to negative for the doped samples, especially for (11)B(+)- and (12)C(+)-ions. We conclude that the conductivity of the graphene sheet is lowered by impurity atoms and especially by lattice defects, because they result in weak localization effects at low temperatures.

119 citations

Journal ArticleDOI
TL;DR: In this paper, a search for new physics is performed using isolated same-sign dileptons with at least two b-quark jets in the final state, based on a 4.98 inverse femtobarn sample of proton-proton collisions at a centre-of-mass energy of 7 TeV collected by the CMS detector.
Abstract: A search for new physics is performed using isolated same-sign dileptons with at least two b-quark jets in the final state. Results are based on a 4.98 inverse femtobarn sample of proton-proton collisions at a centre-of-mass energy of 7 TeV collected by the CMS detector. No excess above the standard model background is observed. Upper limits at 95% confidence level are set on the number of events from non-standard-model sources. These limits are used to set constraints on a number of new physics models. Information on acceptance and efficiencies are also provided so that the results can be used to confront additional models in an approximate way.

119 citations

Journal ArticleDOI
V. M. Abazov1, Brad Abbott2, M. Abolins3, B. S. Acharya4  +536 moreInstitutions (77)
TL;DR: In this paper, a data sample corresponding to an integrated luminosity of 2.1 fb-1 collected by the D0 detector at the Fermilab Tevatron Collider was analyzed to search for squarks and gluinos produced in ppbar collisions at a center-of-mass energy of 1.96 TeV.

119 citations

Journal ArticleDOI
B. P. Abbott1, Richard J. Abbott1, T. D. Abbott2, Fausto Acernese3  +1140 moreInstitutions (123)
TL;DR: Using data recorded by Advanced LIGO during its first observing run, no evidence for a background of any polarization is found, and the first direct bounds on the contributions of vector and scalar polarizations to the stochastic background are placed.
Abstract: The detection of gravitational waves with Advanced LIGO and Advanced Virgo has enabled novel tests of general relativity, including direct study of the polarization of gravitational waves. While general relativity allows for only two tensor gravitational-wave polarizations, general metric theories can additionally predict two vector and two scalar polarizations. The polarization of gravitational waves is encoded in the spectral shape of the stochastic gravitational-wave background, formed by the superposition of cosmological and individually unresolved astrophysical sources. Using data recorded by Advanced LIGO during its first observing run, we search for a stochastic background of generically polarized gravitational waves. We find no evidence for a background of any polarization, and place the first direct bounds on the contributions of vector and scalar polarizations to the stochastic background. Under log-uniform priors for the energy in each polarization, we limit the energy densities of tensor, vector, and scalar modes at 95% credibility to Ω_{0}^{T}<5.58×10^{-8}, Ω_{0}^{V}<6.35×10^{-8}, and Ω_{0}^{S}<1.08×10^{-7} at a reference frequency f_{0}=25 Hz.

119 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