dependence of light-quark sea in the SeaQuest experiment · SeaQuest data collection completed July...

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Status of the measurement of the flavor dependence of light-quark sea in the SeaQuest experiment XXVII International Workshop on Deep Inelastic Scattering and Related Subjects April 8 th -12 th 2019 Jason Dove University of Illinois at Urbana-Champaign Representing the SeaQuest Collaboration

Transcript of dependence of light-quark sea in the SeaQuest experiment · SeaQuest data collection completed July...

Page 1: dependence of light-quark sea in the SeaQuest experiment · SeaQuest data collection completed July 2017 New extraction of D-Y D 2/H 2 as a function of x from 0.1 to 0.45 New cross

Status of the measurement of the flavordependence of light-quark sea in the

SeaQuest experiment

XXVII International Workshop on Deep InelasticScattering and Related Subjects

April 8th-12th 2019

Jason DoveUniversity of Illinois at Urbana-ChampaignRepresenting the SeaQuest Collaboration

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Outline

● The Drell-Yan process

● Flavor asymmetry of the nucleon sea

● SeaQuest experiment

● Status of D2/H2 cross section ratio (new!)

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Drell-Yan process

● Related to DIS via crossingsymmetry

● Provides informationcomplementary to DIS

● Directly probes antiquarks

Deep InelasticScattering

Drell-Yan

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Drell-Yan process

● Related to DIS via crossingsymmetry

● Provides informationcomplementary to DIS

● Directly probes antiquarks

Deep InelasticScattering

Drell-Yan

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Observation of flavor asymmetry of nucleon sea

● Significant deviation of from 1

● Asymmetry has a strongdependence on x

● Can x dependence be explained?

Using 800 GeV proton beam

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Possible explanations● Pion Cloud model

● Chiral Quark model

● Statistical Model

● Rise at low x wellexplained

● None explain drop athigh x

● Need more accuratemeasurement at high x

Meson Cloud Model with physical pion mass and floating pion mass (dashed)

J. Alwall and G. Ingelman. PRD, 71:094015, 2005.

Bourrely, Soffer, Buccella. Eur. Phys. J. C 23, 487–501 (2002)

Statistical model

Dashed line: global fit to data

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● 120 GeV protonbeam

● Completely newdetector apparatus

● ~10x instantaneousintensity

Tevatron

800 GeV

Main Injector120 GeV

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Fermilab E906/SeaQuestCollaboration

● Abilene Christian University

● Academia Sinica

● Argonne National Laboratory

● University of Colorado

● Fermi National Accelerator Laboratory

● University of Illinois

● KEK

● Los Alamos National Laboratory

● Mississippi State University

● University of Maryland

● University of Michigan

● National Kaohsiung Normal University

● RIKEN

● Rutgers, The State University of NewJersey

● Tokyo Tech

● Yamagata University

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E906 Apparatus● 120 GeV proton beam on LH

2,

LD2 targets

● New beamline

● New apparatus

● Forward spectrometer (xF > 0)

● Focusing magnet to bendtracks to spectrometer

● Spectrometer magnet tomeasure momentum of tracks

Target

104 cm

500 cm

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Timeline

● After extensive efforts from 2012,data collection finished in July2017

● Analysis based on run2 and run3data

Firstprotonbeam

2012 2013 2014 2015 2016 2017 2018

MI upgrade run2

Newchambers

run3 run4 run5 run6

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Dimuon mass distribution afterevent selection

● Analysis cuts designed toselect dimuons originatingfrom the target

● Able to resolve and

● By applying a cut of mass> 4.2 GeV we caneffectively removeand

Drell-Yan

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Accidental background

● To get high statistics we run at high intensity ~1e12protons/ second

● Accidental events: from coincidence of two singlemuons such as from pion or kaon decay

● Signal event rate: proportional to intensity linearly

● Accidental event rate: proportional to intensity squaredor higher

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D2/H

2 cross section ratio from intensity

extrapolation method● By extrapolating the

normalized D2/H2 D-Y

yields ratio to zerointensity, all forms ofrate dependence can beremoved

● The intercept gives theD2/H2 cross section ratio

Proton Intensity

D2/H

2

D2/H

2 Drell-Yan yield ratio

vs proton intensity

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Splitting the data into x2

bins

xBeam

xTarget

xTarg

et (x

2)

xBeam (x1)

0 0.5 1

0 0.5 1

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D2/H

2 cross section ratio from intensity

extrapolation method

● The intercept gives the D2/H2 cross section ratio

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Systematics● Extrapolation functional fit

● Negligible

– Choice of intensity binning and range

– Target contamination

– Empty flask subtraction

– Target length

– Beam intensity

– tail contamination

– Event selection cuts

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Drell-Yan cross section ratio

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Cross check withthe mass fit

● Performing a component fitto the mass spectrum

● Use Monte Carlo for signalevents

● Use mixed single trackevents for accidentalbackground

● Compute D-Y cross sectionfor individual targets

● Preliminary D-Y resultsshow consistent D2/H2 ratios

LD2

Preliminary

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Summary● SeaQuest data collection completed July 2017

● New extraction of D-Y D2/H2 as a function of x from 0.1 to 0.45

● New cross section ratio result includes removal of accidentalbackground

● Independent mass-fit method shows consistent D2/H2 ratio

● Extraction of ratio from D2/H2 ratio is underway

● Inclusion of data from after 2016 is underway

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Backup slides

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Fit functional form

● For each x2 bin I, the fit function is of the form

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PDFs

● Q between 4.2 and 8.7 GeV

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E906 vsE866

● E866 and E906have different

– Beam energy (800vs 120 GeV)

– Acceptance

– x1 distributions

● E886 systematics<1% and not shown