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Physics Opportunities in the Near DUNE Detector hall (POND 2 ) Review Peter B. Denton BNL’s HET Lunch Seminar December 14, 2018

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Page 1: Physics Opportunities in the Near DUNE Detector hall (POND2) … · 2018-12-14 · I Solar capture I Up scattered towards the Earth I Angular information in detector I Nuclear e ects

Physics Opportunities in the Near DUNEDetector hall (POND2) Review

Peter B. Denton

BNL’s HET Lunch Seminar

December 14, 2018

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Discussion Outline

I What is the DUNE Near Detector?

I What does the ND need to do?

I What kind of physics can it probe?

Lots of discussion!

“Not building the near detector correctly is like buying aLamborghini and instead of putting high octane fuel in, puttingin diesel.” - Stephen Parke

http://indico.fnal.gov/e/PONDD2018

Peter B. Denton (BNL) BNL’s HET Lunch Seminar: December 14, 2018 2/28

Page 3: Physics Opportunities in the Near DUNE Detector hall (POND2) … · 2018-12-14 · I Solar capture I Up scattered towards the Earth I Angular information in detector I Nuclear e ects

Discussion Outline

I What is the DUNE Near Detector?

I What does the ND need to do?

I What kind of physics can it probe?

Lots of discussion!

“Not building the near detector correctly is like buying aLamborghini and instead of putting high octane fuel in, puttingin diesel.” - Stephen Parke

http://indico.fnal.gov/e/PONDD2018

Peter B. Denton (BNL) BNL’s HET Lunch Seminar: December 14, 2018 2/28

Page 4: Physics Opportunities in the Near DUNE Detector hall (POND2) … · 2018-12-14 · I Solar capture I Up scattered towards the Earth I Angular information in detector I Nuclear e ects

Near Detector Physics Program

1. Aid DUNE FD in measuring δCP

I θ23 octantI Mass orderingI BSM oscillation physics

2. Measure beam properties

3. Measure ν-Ar cross sections

4. DM? MiniBooNE’s anomaly? New physics? Other things?

Peter B. Denton (BNL) BNL’s HET Lunch Seminar: December 14, 2018 3/28

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CPV Sensitivity

A. Bross

Peter B. Denton (BNL) BNL’s HET Lunch Seminar: December 14, 2018 4/28

Page 6: Physics Opportunities in the Near DUNE Detector hall (POND2) … · 2018-12-14 · I Solar capture I Up scattered towards the Earth I Angular information in detector I Nuclear e ects

C. Marshall

Peter B. Denton (BNL) BNL’s HET Lunch Seminar: December 14, 2018 5/28

Page 7: Physics Opportunities in the Near DUNE Detector hall (POND2) … · 2018-12-14 · I Solar capture I Up scattered towards the Earth I Angular information in detector I Nuclear e ects

C. Marshall

Peter B. Denton (BNL) BNL’s HET Lunch Seminar: December 14, 2018 6/28

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Multi-purpose detector design, akin to CMS

R. Harnik

Peter B. Denton (BNL) BNL’s HET Lunch Seminar: December 14, 2018 7/28

Page 9: Physics Opportunities in the Near DUNE Detector hall (POND2) … · 2018-12-14 · I Solar capture I Up scattered towards the Earth I Angular information in detector I Nuclear e ects

∼ 75t fiducial LAr ND

A. Bross

Peter B. Denton (BNL) BNL’s HET Lunch Seminar: December 14, 2018 8/28

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LAr: 3m (tall) x 5m (beam) x 4(7?)m (wide)

J. Sinclair

Peter B. Denton (BNL) BNL’s HET Lunch Seminar: December 14, 2018 9/28

Page 11: Physics Opportunities in the Near DUNE Detector hall (POND2) … · 2018-12-14 · I Solar capture I Up scattered towards the Earth I Angular information in detector I Nuclear e ects

High Pressure gas Time Projection Chamber(HPgTPC): Properties1. High pressure gaseous Ar

I Possibly others, maybe H2?

2. Clear PID: µ, π, e, K, p, D, . . .

3. Magnetic field

4. Charge identification

5. Surrounded by ECAL, µ tagger

6. Hardware is from ALICE

7. Prototype exists at FNAL:Gaseous-Argon Operation of theALICE TPC

T. Mohayai

Peter B. Denton (BNL) BNL’s HET Lunch Seminar: December 14, 2018 10/28

Page 12: Physics Opportunities in the Near DUNE Detector hall (POND2) … · 2018-12-14 · I Solar capture I Up scattered towards the Earth I Angular information in detector I Nuclear e ects

High Pressure gas Time Projection Chamber(HPgTPC): Properties1. High pressure gaseous Ar

I Possibly others, maybe H2?

2. Clear PID: µ, π, e, K, p, D, . . .

3. Magnetic field

4. Charge identification

5. Surrounded by ECAL, µ tagger

6. Hardware is from ALICE

7. Prototype exists at FNAL:Gaseous-Argon Operation of theALICE TPC

T. Mohayai

Peter B. Denton (BNL) BNL’s HET Lunch Seminar: December 14, 2018 10/28

Page 13: Physics Opportunities in the Near DUNE Detector hall (POND2) … · 2018-12-14 · I Solar capture I Up scattered towards the Earth I Angular information in detector I Nuclear e ects

3DST

What it is

I 3D Scintillator Tracker

I Connect with other scintillators(T2K, NOvA, MINERvA, . . . )

I Charge identification (B-field)

I External tracking and ECAL

What it is good for

I Multi-nucleon interactions

I 4π angular coverage

I Neutrons

I ν-e− scattering

C. McGrew

Peter B. Denton (BNL) BNL’s HET Lunch Seminar: December 14, 2018 11/28

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ND Hall

A. Bross

Peter B. Denton (BNL) BNL’s HET Lunch Seminar: December 14, 2018 12/28

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DUNE PRISM

Move the LAr detector horizontally on rails

C. VilelaPeter B. Denton (BNL) BNL’s HET Lunch Seminar: December 14, 2018 13/28

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DUNE PRISM

C. Vilela

Peter B. Denton (BNL) BNL’s HET Lunch Seminar: December 14, 2018 14/28

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DUNE PRISM

C. Vilela

Peter B. Denton (BNL) BNL’s HET Lunch Seminar: December 14, 2018 14/28

Page 18: Physics Opportunities in the Near DUNE Detector hall (POND2) … · 2018-12-14 · I Solar capture I Up scattered towards the Earth I Angular information in detector I Nuclear e ects

C. Marshall

Peter B. Denton (BNL) BNL’s HET Lunch Seminar: December 14, 2018 15/28

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C. Marshall

Peter B. Denton (BNL) BNL’s HET Lunch Seminar: December 14, 2018 16/28

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Generators

I GENIE is widely used at FNALI It is wrong in many waysI Knobs and dials that are not internally consistent

I GiBUU is an alternativeI Less wrongI More physicsI Fewer free parameters

U. Mosel

Peter B. Denton (BNL) BNL’s HET Lunch Seminar: December 14, 2018 17/28

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Other Ideas: Straw Tube Tracker

H. Duyang

Get a ν-H cross section measurement

Peter B. Denton (BNL) BNL’s HET Lunch Seminar: December 14, 2018 18/28

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Other Ideas: Flux Measurement: EMPHATIC

Peter B. Denton (BNL) BNL’s HET Lunch Seminar: December 14, 2018 19/28

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New Physics at theNear Detector

Peter B. Denton (BNL) BNL’s HET Lunch Seminar: December 14, 2018 20/28

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Neutrino Trident

ν +A→ ν + `+ + `− +A

µ+µ− measured by:

I CHARM II (1.58± 0.57)

I CCFR (0.82± 0.28)

I NuTeV (0.67± 0.27)

Constrains Z ′, h±, . . . models:

M. Hostert

Y. Perez-Gonzalez

Peter B. Denton (BNL) BNL’s HET Lunch Seminar: December 14, 2018 21/28

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Trident Rates

Peter B. Denton (BNL) BNL’s HET Lunch Seminar: December 14, 2018 22/28

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NSI with Zero-Distance Effect

I NSIs provide a new matter-like effect

I Generally their effects grow with E and L

I Can be a CC component, affects production, detection

I Can lead to an effect at L = 0 ⇒ ND

I In general DUNE FD can constrain many NSI models

B. Dev

Also generalized NSI’s with S, P, V, A, T interactions

I Systematics crucial to disentangle new interactions frombeam uncertainties

I. Bischer

Peter B. Denton (BNL) BNL’s HET Lunch Seminar: December 14, 2018 23/28

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Some DM Models

I Boosted DM:I Solar captureI Up scattered towards the EarthI Angular information in detectorI Nuclear effects important

J. Berger

I Lepton Number Charged Scalar (LeNCS) for B − LI New scalar φ with B − L = +2I Neutrinos are DiracI Leads to: Higgs/Z invisible, meson decays, 0νββI ND (statistics, charge) is sensitive to mφ ∼ 0.5− 2 GeVI Can add a DM candidate

J. Berryman

Lots of parameter space probed by the ND,probably is much more to do!

Peter B. Denton (BNL) BNL’s HET Lunch Seminar: December 14, 2018 24/28

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Milicharged Particles

I Fractional charges allowed

I Even with integer charges can get mCP via 1-loop εFµνF′µν

I Production: from meson decays → very high rate

I Detection: think dE/dx but much slower ⇒ soft hits

I If two soft hits line up, then mCP

I ArgoNeut analysis (with data) en route, DUNE ND next

I Good parameter space sensitivity improvement

Peter B. Denton (BNL) BNL’s HET Lunch Seminar: December 14, 2018 25/28

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Neutrino Theory Network (NTN)

I FNAL got leftover money (∼$300k) from the DOE

I Has been assigned for neutrino theory

I Initial struggles managing the money

I Awards go for things promoting the US neutrino effort

I Can be spent:I To go somewhere for a time O(weeks to months)I To host a workshopI To pay a grad student for O(months)

I Has been renewed

I Expect two calls per year, next should be in January

I http://ntn.fnal.gov

See also the NPC, IF, URA which provide for to travel toFermilabPlease ask if you have questions1!

1Disclaimer: I am not affiliated with the NTN.Peter B. Denton (BNL) BNL’s HET Lunch Seminar: December 14, 2018 26/28

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Zenodo

I Conference proceedings:I Time inefficientI Either aren’t read (theory) or not representative of the

conference (experiment)I Treated (roughly) the same as an article by inspire

I Alternative: upload slides to https://zenodo.orgI Permanent record of what was discussedI Get a DOI so is citableI Working with inspire to track them

I This was done from Neutrino 2018 Heidelberg

I This is being done for PONDD

I Talk to Stephen Parke about how to do this for futureconferences/workshops

Peter B. Denton (BNL) BNL’s HET Lunch Seminar: December 14, 2018 27/28

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Key Points

I Near detector design is coming along: 3+ detectors and PRISM

I Flux and cross section uncertainties are/will be always concerning

I The ND alone will be an excellent probe of SM and NP, more to do

I Lots of other good talks on:

I MiniBooNE

I Global fits

I LAr backgrounds

I Solar neutrinos with DUNE

I HNL and long-lived particles

I Machine learning

I Many other topics

Peter B. Denton (BNL) BNL’s HET Lunch Seminar: December 14, 2018 28/28

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Backups

Peter B. Denton (BNL) BNL’s HET Lunch Seminar: December 14, 2018 29/28

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A Theorist’s Long-Baseline Picture

ExperimentsMeasure dN

dEDUNE, T2HK, . . .

Near Detector

ProbabilitiesP (να → νβ)

in matter

Oscillation Parametersθ23 octant, δCP,

mass ordering, . . .

UnderstandingLeptogenesis, flavor

structure, new physics, . . .

BSM ParametersSterile, NSI, decay,

decoherence, unitarity, . . .

PBDPeter B. Denton (BNL) BNL’s HET Lunch Seminar: December 14, 2018 30/28

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θ23, δ

θ13

θ12

α13|α23

α23|α13

α12|α12

...

1st

order

2nd

order

...

1st

order

...

VacuumRot.

MatterRot.

ν|ν

Pert.

MP15DMP16DPZ18

Required toremovelevel crossings

Correctionsare O(ε′)

Correctionsare O(ε′2)

Correctionsare O(ε′3)

|ε′| < 0.015and

ε′ = 0 invacuum

Rotations, Perturbations

PBD

Peter B. Denton (BNL) BNL’s HET Lunch Seminar: December 14, 2018 31/28

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Extend to new physics such as steriles

X. Zhang

Peter B. Denton (BNL) BNL’s HET Lunch Seminar: December 14, 2018 32/28