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Dijet angular distr...
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Boelaert, NeleLund University,Lunds universitet,Partikel- och kärnfysik,Fysiska institutionen,Institutioner vid LTH,Lunds Tekniska Högskola,Particle and nuclear physics,Department of Physics,Departments at LTH,Faculty of Engineering, LTH
(author)
Dijet angular distributions at root s=14 TeV
- Article/chapterEnglish2010
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2010-02-19
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Springer Science and Business Media LLC,2010
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LIBRIS-ID:oai:lup.lub.lu.se:610b7a1e-5baa-49c0-8cfa-0242540b8773
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https://lup.lub.lu.se/record/1603932URI
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https://doi.org/10.1140/epjc/s10052-010-1268-8DOI
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Language:English
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Summary in:English
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We present a Monte Carlo study of dijet angular distributions at root s = 14 TeV. First we perform a next-to- leading order QCD study; we calculate the distributions in four different bins of dijet invariant mass using different Monte Carlo programs and different jet algorithms, and we also investigate the systematic uncertainties coming from the choice of the parton distribution functions and the renormalization and factorization scales. In the second part of this paper, we present the effects on the distributions coming from a model including gravitational scattering and black hole formation in a world with large extra dimensions. Assuming a 25% systematic uncertainty, we report a discovery potential for the mass bin 1 < M-jj < 2 TeV at 10 pb(-1) integrated luminosity.
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Åkesson, TorstenLund University,Lunds universitet,Partikel- och kärnfysik,Fysiska institutionen,Institutioner vid LTH,Lunds Tekniska Högskola,Particle and nuclear physics,Department of Physics,Departments at LTH,Faculty of Engineering, LTH(Swepub:lu)quar-tak
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Partikel- och kärnfysikFysiska institutionen
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In:European Physical Journal C. Particles and Fields: Springer Science and Business Media LLC66:3-4, s. 343-3571434-6044
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In:The European Physical Journal C: Springer Science and Business Media LLC66:3-4, s. 343-3571434-6052
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