Physics Department Lancaster University Cavity development Rebecca Seviour.
DIS from EMC to H1 T.Sloan, University of Lancaster. QCDN-06 Rome 2006
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Transcript of DIS from EMC to H1 T.Sloan, University of Lancaster. QCDN-06 Rome 2006
DIS from EMC to H1T.Sloan, University of Lancaster.
QCDN-06 Rome 2006
• EMC proposal ’72-74• Build 1974-1978• Run 1978-1985• NMC (3rd generation)• SMC (4th generation)• Compass (5th gen)
• H1 proposal 1985; Build 1985-1992 Run 1992 - 2007
DIS discovered at SLAC in 1960s – 1990 Nobel Prize
This led to - later generations of νN and μ(e)N experiments
The Crowning Glory of the Work
EMC Spin Effect.
Proved that only a small fraction of nucleon’s spin is carried by the quarks.
Incredible – we all thought we understood the quark-parton model.
Is it ΔG or is the nucleon a Skyrmion ? Or is it something else ?
NMC
Unexpected Effect (EMC Effect)
H1 How long will F2 Rise ?
EMC BSMSearch for free quarks
Search for D→μμObserve J/ψ peakCharm cross section order of magnitude bigger
Set limit on BR D→μμ of < 3.4 10-4 (A. Staiano’s thesis - 1984)
Sociology – one senior physicist commentedon the draft paper Why have you done this analysis ? This is a very quiet paper.
Was he correct ? There are 8 citations for the paper on Spires.
Look at quality of the citations
1. Particle data group (paper still there)
2. The experiment which copied us using a pion beam (bigger luminosity)
3. Others
If we had found a signal for D→μμ the standard model would have needed modification
Conclusion
We were right to do the analysis.
The Collaborations
• EMC and H1 Work divided into several sub groups
• Structure Functions, Heavy flavour, hadronic final states (EMC and H1)
• Diffraction, BSM (H1) – diffraction and the standard model not part of vocabulary in EMC days
Heavy Flavour Physics• EMC discovered via multimuons that boson gluon fusion was
responsible for charm production – among first evidence for gluons
Contribution of b and c to F2 - F2cc and F2 bb
Hadronic Final States• Programme in EMC (NA2, NA9)
• Lund Model developed for e+e- and μp data (ca1980). Much work was done to tune up the parameters of the model.
• H1 works in Breit frame, studies jets etc. Jets give insight into production of primary quarks and gluons.
EMC Inclusive Identified Hadrons - 1983
EMC Seagull plot – gluon radiation (1983)
H1 Scaling violations in fragmentation functions
in Breit Frame compared to e+e- data.
αs versus Q from event shapes
Using dijets to constrain gluon distribution
EW PhysicsFirst BCDMS measurement from μ+p μ-p differences
BCDMS data
H1 from e+p e-p differences
Are there right handed currents ?
Diffraction
• Not known in EMC days except for exclusive ρ, φ, J/ψ …
• Discovered in rapidity gap data at HERA.
• Now also being studied in forward leading proton and neutron data.
• Diffraction important for cosmic ray shower generation.
Cosmic Ray shower simulation
• Energy flow into forward region is very important for simulation of cosmic ray air showers.
• Estimate ~x% of events have a leading proton and ~y% have a leading neutron.
• Hence diffraction is important.
ZEUS Leading neutrons
Zeus Leading protons
ISR leadingphotons
ISR leading Neutrons(Flauger and Monnig
Leading neutron data – ISRIs the bump at high x one pion exchange ?
Holtmann,Szczurek,Speth
Dashed ps meson exch
Dotted vec meson exch
Solid total
Conclusions
EMC and H1 have been great places to work.
Plenty of outstanding questions – where is the spin of the proton ?
What will limit the rise of F2 ?
Is diffraction telling us something about the nuclear force ?
Many questions for the workshop
F2 Accuracy Now and 1996 Expected
• Wider x range expected to be covered
• (down to 1.4 10-5 compared to 6.510-5)
• Improved systematic errors expected in 1996 compared to now. Eg 0.5% electron energy calibration backward and 1% central and forward (compared to 1% backward and 0.7%-3% central-forward).
• Some work is needed here.
–Projected final accuracy is much better at x=0.65 than we actually have now.
PDF Accuracy
1996 Suggested to use jets to determinePDF by G.Lobo – fit made by ZEUS
The ZEUS fit already approaches the accuracy expected in 1996.
Measurement of xF3 from e+ e- differences
Based on 16 pb-1 of e- data – so improvement expected.
FL - 1996
Black points from extrapolation Measurement .Open from 4 protonEnergies 10pb-1 at each
Diffraction
• In 1995/6 rapidity gaps had not been known for too long – so plans at workshop were primitive.
• We have done much more than was considered at the workshop.
• E.g.F2D3,F2
D4, diffractive charm, vector meson production, dijets, DVCS…
Correlations between quarks studied by DVCS i.e. scatter highly virtual photon and detect a real one (NB e,γ, proton in final state).
Several new structure functions are needed to describe such correlations. It is not yet known how to measure them – hence can only compare with models.
Jets and High ET Group
• I could not find anything on this topic in the 1995-96 workshop that we have not done.
• Some things extra – odderon searches, anti-deuterons …
• However, we still have not published the fragmentation functions for identified particles (except π0).
Flagship Plot
αS=0.1198±0.0013(exp) +0.0056-0.0043(theor) L=106pb-1
EW Plot – Status with 21 pb-1 L and 27 pb-1 R
Classic plot demonstrating directly the left handedness of the W – this plot will end up in the text books. Must check with e- which should have negative slope.
Poor fit to SM – New physics ?
Current limit on ΔσR/σL is 7%
In 1996 projected to achieve 0.4%With L=500pb-1 and 70% polarisation.Use this to set limit on mass of WR
Conclusions
• Not much in the 1996 workshop to help us today• H1 has done great work – I have shown my
ideas of the flagship plots which we should leave for future generations.
• Each sub-group should identify its flagship plots.• These should be made before we stop analysing
HERA data with the smallest errors possible.