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Subir Sarkar

Researcher at University of Oxford

Publications -  1566
Citations -  158344

Subir Sarkar is an academic researcher from University of Oxford. The author has contributed to research in topics: Neutrino & Large Hadron Collider. The author has an hindex of 149, co-authored 1542 publications receiving 144614 citations. Previous affiliations of Subir Sarkar include Inter-University Centre for Astronomy and Astrophysics & Max Planck Society.

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Measurement of electroweak production of two jets in association with a Z boson in proton–proton collisions at s=8TeV

Vardan Khachatryan, +2141 more
TL;DR: In this article, the electroweak cross section for the production of two jets in association with a Z boson, in proton-proton collisions at sqrt(s) = 8 TeV, is measured using data recorded by the CMS experiment at the CERN LHC, corresponding to an integrated luminosity of 19.7 inverse femtobarns.
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Search for long-lived particles with displaced vertices in multijet events in proton-proton collisions at s =13 TeV

Albert M. Sirunyan, +2268 more
- 16 Nov 2018 - 
TL;DR: In this paper, a search for long-lived particles in proton-proton collisions at √s = 13 TeV delivered by the CERN LHC and collected by the CMS experiment is reported.
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Search for Sources of Astrophysical Neutrinos Using Seven Years of IceCube Cascade Events

M. G. Aartsen, +355 more
TL;DR: Low-background searches for astrophysical neutrino sources anywhere in the sky can be performed using cascade events induced by neutrinos of all flavors interacting in IceCube with energies as low as 0.
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Transverse momentum spectra of inclusive b jets in pPb collisions at √sNN=5.02 TeV

Vardan Khachatryan, +2291 more
- 10 Mar 2016 - 
TL;DR: In this paper, a measurement of b jet transverse momentum spectra in proton-lead (pPb) collisions using a dataset corresponding to about 35 inverse nanobarns collected with the CMS detector at the LHC is presented.
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Cosmogenic photons as a test of ultra-high energy cosmic ray composition

TL;DR: In this article, it was shown that if the ultra-high energy cosmic rays are dominated by heavy nuclei, the flux of these photons is suppressed by approximately an order of magnitude relative to the proton-dominated case.