activities of the university of nebraska-lincoln (unl) high energy physics group in cms

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NSF reverse site visit, March 14, 2007 1 Activities of the University of Nebraska-Lincoln (UNL) High Energy Physics Group in CMS Overview of Group Involvements HEP Group Personnel and Their Affiliations Areas of Involvement in CMS Physics Directions Leadership Roles CMS effort and cost breakdown for upcoming year NSF Proposal PHY-0653592 “Experimental High Energy Physics”

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Activities of the University of Nebraska-Lincoln (UNL) High Energy Physics Group in CMS. NSF Proposal PHY-0653592 “Experimental High Energy Physics”. Overview of Group Involvements HEP Group Personnel and Their Affiliations Areas of Involvement in CMS Physics Directions - PowerPoint PPT Presentation

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Page 1: Activities of the University of Nebraska-Lincoln (UNL) High Energy Physics Group in CMS

NSF reverse site visit, March 14, 2007

1

Activities of theUniversity of Nebraska-Lincoln (UNL)

High Energy Physics Groupin CMS

• Overview of Group Involvements• HEP Group Personnel and Their Affiliations

• Areas of Involvement in CMS • Physics Directions

• Leadership Roles

• CMS effort and cost breakdown for upcoming year

NSF Proposal PHY-0653592“Experimental High Energy Physics”

Page 2: Activities of the University of Nebraska-Lincoln (UNL) High Energy Physics Group in CMS

NSF reverse site visit, March 14, 2007

2

Who is on the phone with you today?

Dan Claes Greg Snow

Ken Bloom

Aaron Dominguez

Page 3: Activities of the University of Nebraska-Lincoln (UNL) High Energy Physics Group in CMS

NSF reverse site visit, March 14, 2007

3

UNL High Energy Physics GroupOverview

For the duration of the 3-year base-funding proposal (June 2007 – June 2010), the UNL HEP group will be pursuing frontier physicsresearch through its collaboration in Fermilab’s DZERO and CERN’s CMS Experiments.

The anticipated breakdown of commitment, averaged over the group,for the 3 years isYear One (2007-2008): 50% CMS, 50% DZEROYear Two (2008-2009): 60% CMS, 40% DZEROYear Three (2009-2010): 75% CMS, 25% DZERO

The group also leads a nationally recognized education/outreachexperiment, CROP – the Cosmic Ray Observatory Project, that,along with other outreach efforts, makes it a leading groupin physics education/outreach at many levels.

Page 4: Activities of the University of Nebraska-Lincoln (UNL) High Energy Physics Group in CMS

NSF reverse site visit, March 14, 2007

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UNL HEP Personnel and Their Project Affiliations

Faculty members:

G. Snow (1993): CMS and DZERO Experiments, CROP,Pierre Auger Observatory

D. Claes (1996): CMS and DZERO Experiments, CROP,DUSEL/UNO Experiments

K. Bloom (2004): CMS and DZERO Experiments,NSF Career outreach (Rural Nebraska)

A. Dominguez (2004): CMS and DZERO Experiments, NSF Career outreach (Bilingual English/Spanish Tutors – BEST)

Tenured Associate Prof.

Tenured Associate Prof.

Tenure-track AssistantProfessor

Tenure-track AssistantProfessor

Page 5: Activities of the University of Nebraska-Lincoln (UNL) High Energy Physics Group in CMS

NSF reverse site visit, March 14, 2007

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UNL HEP Personnel and Their Project Affiliations

Postdoctoral Research Physicists:

A.Bellavance*: DZERO

A. Sobol*: CMS

M. Eads: CMS and DZERO

S. Malik: CMS and DZERO

Senior Research Associate, left group in January 2007 for Fermilab Computing Division

Postdoctoral Research Associate, to leave group imminently to resume position in Russia

Research Assistant Professor

Postdoctoral Research Associate

Bellavance

Eads

Malik

*Supported by present Claes/Snow base funding grant

Page 6: Activities of the University of Nebraska-Lincoln (UNL) High Energy Physics Group in CMS

NSF reverse site visit, March 14, 2007

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UNL HEP Personnel and Their Project Affiliations

Postdoctoral Research Physicists:

A.Bellavance: DZERO

A. Sobol: CMSPostdoctoral Research Associate, to leave group imminently to resume position in Russia

Senior Research Associate, left group in January 2007 for Fermilab Computing Division

• Replacing these two positions is crucial to the group’s strength in CMS• Bellavance replacement is foreseen to transition DZERO to CMS over the course of proposed 3-year program• Ideal candidate: DZERO graduating Ph.D. aiming for LHC involvement. Several top candidates exist.

Page 7: Activities of the University of Nebraska-Lincoln (UNL) High Energy Physics Group in CMS

NSF reverse site visit, March 14, 2007

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UNL HEP Personnel and Their Project Affiliations

Current Graduate Students: K. DeVaughan: DZERO ExperimentD. Johnston: DZERO ExperimentM. Voutilainen: DZERO Experiment

X. Xu: CROP

First year students:J. Keller: CMS candidateT. Kelly: CMS candidateE. Petermann: CMS candidate

1-2 HEP students may join thegroup in fall 2007

UNL Visiting Scholar from Helsinki, Ph.D. 2007 on Inclusive jets

Department of Statistics, Masters Degree 2006

Page 8: Activities of the University of Nebraska-Lincoln (UNL) High Energy Physics Group in CMS

NSF reverse site visit, March 14, 2007

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UNL HEP Personnel and Their Project Affiliations

Other Affiliated Staff: Brian Bockelman: CMS Tier2, CSE graduate student

Makoto Furukawa: CMS Tier2 administrator, CSE Dept.

Carl Lundstedt: CMS Tier2 administrator, CSE Dept.

David Swanson: CMS Tier2 Principal Investigator, CSE Department

Plus undergraduate physics majors contributing toDZERO, CMS, and our outreach efforts

Page 9: Activities of the University of Nebraska-Lincoln (UNL) High Energy Physics Group in CMS

NSF reverse site visit, March 14, 2007

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The DZERO Experiment

DZERO is a mature facility in data-taking and physicspublication mode, with data-taking continuing until 2009 and analysis extending through 2010

UNL involvements in: Level-2 and -3 trigger electronicsand software, track reconstruction software, physicsanalysis (QCD, Electroweak, Top Quark, Higgs Searches,and New Phenomena), internal Editorial Boards, luminositymeasurement, data-taking shifts, other servicework, Speaker’s Bureau, Public Tour Area

Present leadership roles:G. Snow: Co-convener of Luminosity Working GroupM. Eads: Co-convener of Muon ID Working Group

Page 10: Activities of the University of Nebraska-Lincoln (UNL) High Energy Physics Group in CMS

NSF reverse site visit, March 14, 2007

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HEP Group Education and Outreach

Summary of initiatives• The Cosmic Ray Observatory Project (CROP)

• $1.34 Million NSF grant• Snow serves as task leader for Education/Outreach

for the Pierre Auger Observatory in Argentina and Colorado

• Claes serves as Education/Outreach for the emerging DUSEL and UNO initiatives in Colorado

• Bloom and Dominguez have important outreach initiatives funded by their NSF Career grants

The UNL HEP group faculty members are leadersnationally known HEP education and outreach initiatives

Page 11: Activities of the University of Nebraska-Lincoln (UNL) High Energy Physics Group in CMS

NSF reverse site visit, March 14, 2007

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The UNL group in the CMS Experiment

UNL joined the CMS experiment in 1994• Preparation of the Technical Proposal• Luminosity Measurement• Forward and Diffractive Physics simulations• CMS Ph.D. Thesis Award Program

Major new initiatives over the last 3 years:Forward Pixel Detector – U.S. based project A. Dominguez is coordinator of Forward Pixel moduletesting

Tier-2 Computing Center at UNL – very high visibilityOne of 7 in the United StatesK. Bloom is project manager for all US Tier-2 centers

Page 12: Activities of the University of Nebraska-Lincoln (UNL) High Energy Physics Group in CMS

NSF reverse site visit, March 14, 2007

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Wilson Hall

DØCDF

Fermilab in Batavia, Illinois

TheDZEROExpt.

ProtonAnti-

protoncollisions

“Sidet”Silicon

DetectorFacility

“LPC”: LHCPhysicsCenter

and “ROC”:Remote

OperationsCenter

The UNL group has and will rely on FNAL resources forCMS, making it convenient to split effort with DZERO

involvements

Page 13: Activities of the University of Nebraska-Lincoln (UNL) High Energy Physics Group in CMS

NSF reverse site visit, March 14, 2007

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CMS accomplishments, past 12 months

• Hosted annual US-CMS collaboration meeting, April 2006 (Snow and full group)

• Forward and Diffractive Physics contribution to CMS-TOTEM Letter of Intent (CERN/LHCC 2006-039/G-124) (Snow, Sobol)

• CMS Thesis Awards Program (Snow)

• UNL CMS Tier-2 computing center progress and data challenge (Bloom, Dominguez, Tier-2 affiliated staff)

• Forward Pixel Detector progress (Dominguez, Eads, Malik)

• Tracking and Vertex Reconstruction (Dominguez, Lundstedt, graduate students)

Page 14: Activities of the University of Nebraska-Lincoln (UNL) High Energy Physics Group in CMS

NSF reverse site visit, March 14, 2007

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The CMS Thesis Award Program

• Unique to CMS at CERN• Initiated by G. Snow in 2000, served as Secretary of the 8-member Committee for 7 years• Committee has dealt with 49 nominated theses in 7 years• Recipients receive plaque and expenses to an int’l conference to present thesis results• Work concentrated Sept.-Dec. when nominated theses are critiqued and ranked by Committee• Secretary’s work extends throughout the year• Most of the Thesis Award recipients have continued on CMS as postdocs and are in leadership positions

Page 15: Activities of the University of Nebraska-Lincoln (UNL) High Energy Physics Group in CMS

NSF reverse site visit, March 14, 2007

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The CMS Thesis Award Program

Web page

Ivica Puljak2001 recipient

Large plaquein Building 40

Page 16: Activities of the University of Nebraska-Lincoln (UNL) High Energy Physics Group in CMS

NSF reverse site visit, March 14, 2007

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Nebraska’s Tier-2 Computing Center for CMS

Bloom, Dominguez with Tier-2PI David Swanson (UNL CSE Dept., Director Research Computing Facility)with Tier-2 CPU cluster

Major commitment to CMS computingand analysis for many years

Generous University support

Bloom serves as US-CMS Tier-2Program Manager (7 sites)

Last 12 months:• Successful fall 2006 data challenge

• Transition to final software (CMSSW) and data management frameworks

Page 17: Activities of the University of Nebraska-Lincoln (UNL) High Energy Physics Group in CMS

NSF reverse site visit, March 14, 2007

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Fall 2006 Computing, Software, AnalysisChallenge (CSA06)

Nebraska’sTier-2

Data transferred (Tbyes) to the 7 U.S. Tier-2 sites

Page 18: Activities of the University of Nebraska-Lincoln (UNL) High Energy Physics Group in CMS

NSF reverse site visit, March 14, 2007

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Fall 2006 Computing, Software, AnalysisChallenge (CSA06)

Nebraska’sTier-2

CPU hours generating Monte Carlo for the challenge

Page 19: Activities of the University of Nebraska-Lincoln (UNL) High Energy Physics Group in CMS

NSF reverse site visit, March 14, 2007

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~ 0.3m

• Consists of Barrel and Forward Disks

• USA responsible for Forward Disks

• 100 × 150 µm2 pixel size excellent spatial resolution 10-20 µm

– Charge sharing promoted by 4T B field and 200 tilt in FPix

• 4 Forward disks (FPix) – Each Disk made of two ½-disks

– Z=34.5 and 46.5 cm ( 6 cm above beam line)

– 96 blades, 192 panels, 672 plaquettes– Plaquettes = Sensor + Readout Chips +

Flex Circuits– 4320 Readout Chips – 18 million pixels– 0.45 m2 silicon

• Nebraska responsible for testing and grading all plaquettes and panels

The Pixel Detector for CMS

Barrel

~ 1mDisks

Panel (4 types)

Plaquette (7 types)

Disk

IR

Page 20: Activities of the University of Nebraska-Lincoln (UNL) High Energy Physics Group in CMS

NSF reverse site visit, March 14, 2007

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Nebraska’s Responsibility

Testing Area

Test Stand

• Operate and maintain testing area at Sidet (FNAL)

• Hardware, software, shifts

• Test all plaquettes and panels

• 8 plaquettes/day (672 needed)

• 2 panels/day (192 needed)

• Grade plaquettes and panels

Burn-in Box

Modules under test

Plaquette Panel

Page 21: Activities of the University of Nebraska-Lincoln (UNL) High Energy Physics Group in CMS

NSF reverse site visit, March 14, 2007

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Plaquettes/Panels Tested

• Need EIGHT ½-disks

• ½-disk needs 84 plaquettes of SEVEN types on 24 panels of FOUR types

Plaquettes tested and assembled on panels: ½ - disk equivalent

http://fpixserv.fnal.gov:8081/production/

Page 22: Activities of the University of Nebraska-Lincoln (UNL) High Energy Physics Group in CMS

NSF reverse site visit, March 14, 2007

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½-Disk and ½-Cylinder

First Production ½-Cylinder

Pilot Run Detector• Tested modules for 2007 CMS Pilot Run FPix Detector (8 panels)

• Invaluable learning tool for the “real” run

• Shipped to CERN in January 07

• First Production ½-disk now in making

• First Production ½- cylinder now being instrumented

• Ship 8 ½-disks and

4 ½-cylinders by summer 2008

Panels on First Production ½-Disk

Page 23: Activities of the University of Nebraska-Lincoln (UNL) High Energy Physics Group in CMS

NSF reverse site visit, March 14, 2007

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CMS goals, next 12 months

• Complete Forward Pixel Detector, establish silicon R&D lab at UNL (Dominguez, Bloom, Claes, Eads, Malik, graduate students)• Commission Tier-2 cluster to full capacity, CSA07 challenge (Bloom, Dominguez, Tier-2 affiliated staff)• Forward and Diffractive Physics, publication-grade paper challenge (Snow, postdoc)• Primary vertexing (Dominguez, Claes)• CMS luminosity measurement (Snow, postdoc)• Physics Commissioning (Bloom, Claes, Dominguez, Snow, postdocs, graduate students)• CMS Thesis Award Program (Snow)

Page 24: Activities of the University of Nebraska-Lincoln (UNL) High Energy Physics Group in CMS

NSF reverse site visit, March 14, 2007

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CMS physics organizationPhysics

CoordinatorP.SphicasDeputy:

J.Incandela

MC generators

P.BartaliniF.Moortgat

HiggsA.Nikitenko

Y.Sirois

SUSY-BSMS.Eno

M.Spiropulu

EWKR.Tenchini

B physicsU.Langenegger

b-taggingT.Speer

I.Tomalin

Jets/MissETG.DissertoriN.Varelas

MuonsN.Amapane

N.Neumeister

e/D. FutyanP.Vanlaer

Onl Selection

S.DasuC.Leonidopoulo

s

ParticleFlow/

R.CavanaughP.Janot

DiffractionM.Groethe

Heavy IonsD.D’EnterriaB.Wyslouch

Super LHCD.Denegri

QCDK.Rabbertz

TopJ.D’Hondt J.Mnich

The UNL HEP group has expertise (Tevatron) in manyareas of CMS physics

Snow

Claes

Bloom

Dominguez

Page 25: Activities of the University of Nebraska-Lincoln (UNL) High Energy Physics Group in CMS

NSF reverse site visit, March 14, 2007

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2007 Physics Exercise: “Papers we wantto write in 2008”

Complete this slide

Hard single and double diffractive paper (diagram andplot)

Involvement in similar efforts by other group members

Meeting with physics conveners at FNAL in April

Page 26: Activities of the University of Nebraska-Lincoln (UNL) High Energy Physics Group in CMS

NSF reverse site visit, March 14, 2007

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CMS Leadership Summary

Snow• Secretary, CMS Thesis Award Committee• CMS and US-CMS Collaboration Board representative• Chair, Fermilab Board of Directors ES&H Committee (CMS safety issues for US-CMS collaborators)

Bloom• US-CMS Tier-2 Program Manager• Member of CMS ROC Advisory Committee• Senior Advisor in CMS Top Physics group

Dominguez• UNL representative on the Tracker Institution Board• Member of the US-CMS Institutional Advisory Board

Page 27: Activities of the University of Nebraska-Lincoln (UNL) High Energy Physics Group in CMS

NSF reverse site visit, March 14, 2007

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Projected CMS effort in 2007

Bloom Professor 75%

Claes Professor 25-50%

Dominguez Professor 75%

Snow Professor 50%

Eads Postdoc 50% Supervised by Bloom and Dominguez

MalikResearch

Asst. Prof.100% Supervised by Bloom and Dominguez

(Bellavance)Senior Rsrh.

Associate25% Replacement to begin mid-2007

(Sobol) Post doc 100% Replacement to begin mid-2007

Keller Student 20% (reflects mostly summer research time)

Kelly Student 20% (reflects mostly summer research time)

Page 28: Activities of the University of Nebraska-Lincoln (UNL) High Energy Physics Group in CMS

NSF reverse site visit, March 14, 2007

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Fraction of first-year proposal budgetdevoted to CMS

CMS commitment Amount Requested

Snow (50% of summer salary) 10,692 22,239

Claes (25% of summer salary) 4,396 17,585

Postdoc (at least 1 full-time CMS) 44,000 88,000

Benefits (28% of above salaries) 16545 35,551

Undergrads - 14,252

GRA (at least one committed to CMS) 18,600 37,200

Graduate Tuition Remission 5,952 11,904

Grad Student Health 750 1,500

Domestic Travel (~50% CMS) 16,100 32,200

Foreign Travel (~100% CMS) 12,000 12,000

Publications - 250

Materials & Supplies - 4,750

Subtotal 120,035 276,574

IDC 29,866 72,409

Total Request 149,901 345,388

43% CMS