'Theoretical uncertainty' presentation slideshows

Theoretical uncertainty - PowerPoint PPT Presentation

Uncertainties and Consistency (?) in pQCD and AdS /CFT Jet Physics

Uncertainties and Consistency (?) in pQCD and AdS /CFT Jet Physics

Uncertainties and Consistency (?) in pQCD and AdS /CFT Jet Physics. W. A. Horowitz The Ohio State University March 17, 2010. With many thanks to Brian Cole, Miklos Gyulassy , Ulrich Heinz, and Yuri Kovchegov. Why High- p T Particles?. and even more with multiple probes.

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285 views • 28 slides
Brief update of Muon Collider Higgs Physics studies

Brief update of Muon Collider Higgs Physics studies

1. Brief update of Muon Collider Higgs Physics studies. Higgs & 4th Family Physics Studies 3/21/2012 https:// indico.fnal.gov/conferenceDisplay.py?confId=5398 Higgs Observation by CMS, Atlas, LHC 7/4/2012 This update. G P Yeh 8/1/2012. 2. 3.

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349 views • 26 slides
B Ricci* Helioseismology and solar models

B Ricci* Helioseismology and solar models

LNGS 12 March 2001. B Ricci* Helioseismology and solar models. Helioseismic observables SSMs and helioseismology 2000+ Solar physics metal abundance, age, mixing.... Plasma physics Diffusion, Statistics, Screening Nuclear Physics S pp , S 33 & S 34 Subnuclear Physics

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251 views • 24 slides
Energy Loss in the Hot QCD Brick I

Energy Loss in the Hot QCD Brick I

Energy Loss in the Hot QCD Brick I. W. A. Horowitz The Ohio State University December 16, 2009. With many thanks to Brian Cole, Miklos Gyulassy , Yuri Kovchegov , and TECHQM Collab. Outline. High- p T motivation Differences seen in parameters OK

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204 views • 20 slides
Status Report

Status Report

Status Report. 14.05.2014. Overview. note editing PDF theoretical uncertainties. Note editing. extended the fit to the muon final state case tried multiple fitting PDFs for every case asymmetric Gauss convolution of Gauss into Breit -Wigner Crystal-Ball

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225 views • 4 slides
Flux of Atmospheric Neutrinos T. Gaisser and M. Honda

Flux of Atmospheric Neutrinos T. Gaisser and M. Honda

Uncertainty in Primary Spectrum +-20% below 100 GeV +-30% above 100 GeV. Flux of Atmospheric Neutrinos T. Gaisser and M. Honda Annu. Rev. Nucl. Part. Sci. 2002, 52: 153-199. Figure 6. Uncertainty from Hadronic Interactions +-20%-25% (even when Lundy data is excluded).

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144 views • 3 slides

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