search for dark photons at na62 - institut national de...

23
Search for dark photons at NA62 Marco Mirra Universitร  degli studi di Napoli Federico II and Sezione INFN Napoli o n behalf of NA62 collaboration Rencontres de Moriond QCD and High Energy Interactions 21 March 2018, La Thuile, Italia

Upload: others

Post on 30-Jun-2020

1 views

Category:

Documents


0 download

TRANSCRIPT

Page 1: Search for dark photons at NA62 - Institut national de ...moriond.in2p3.fr/QCD/2018/WednesdayMorning/Mirra.pdf21/03/2018 M. Mirra Search for dark photons at NA62 2 Hidden sector motivations

Search for dark photons at NA62

Marco Mirra

Universitร  degli studi di Napoli Federico II and Sezione INFN Napoli

on behalf of NA62 collaboration

Rencontres de Moriond QCD and High Energy Interactions

21 March 2018, La Thuile, Italia

Page 2: Search for dark photons at NA62 - Institut national de ...moriond.in2p3.fr/QCD/2018/WednesdayMorning/Mirra.pdf21/03/2018 M. Mirra Search for dark photons at NA62 2 Hidden sector motivations

M. Mirra Search for dark photons at NA6221/03/2018 2

Hidden sector motivations

If DM is a thermal relic from hot early universe, can hunt for it in particle-physics: search for

non-gravitational interactions DM-SM

A mediator of a hidden sector might exist, inducing DM-SM field (feeble) interactions; many

possible dynamics: vector (Aโ€™ dark photon), neutrino (HNL), axial (ALP a), scalar..

Various experimental hints for hidden sector at MeV-GeV, e.g., aฮผ 3.5-ฯƒ discrepancy:

Feeble interaction: ultra-suppressed production rate, very long-lived states.

E.g.: 1-GeV mass HNL, ฯ„ ~ 10-5-10-2 s, decay length ~ 10-10000 Km at SPS energies,

suppression at production 10-7-10-10

Might be due to a

dark photon Aโ€™...

โ€ฆor to an ALP a

enhancing light-by-light?

Aโ€™

a

[Okun, Holdom] [Marciano et al. arXiv:1607.01022]

Page 3: Search for dark photons at NA62 - Institut national de ...moriond.in2p3.fr/QCD/2018/WednesdayMorning/Mirra.pdf21/03/2018 M. Mirra Search for dark photons at NA62 2 Hidden sector motivations

M. Mirra Search for dark photons at NA6221/03/2018 3

NA62 experiment

Kaon physics at CERN:

Fixed target experiments at

CERN SPS

Kaon decay-in-flight

Currently in NA62:

~200 participants

29 institutions from 13 countries

NA62

Page 4: Search for dark photons at NA62 - Institut national de ...moriond.in2p3.fr/QCD/2018/WednesdayMorning/Mirra.pdf21/03/2018 M. Mirra Search for dark photons at NA62 2 Hidden sector motivations

M. Mirra Search for dark photons at NA6221/03/2018 4

NA62 layout

[NA62 Detector Paper, JINST 12 (2017), P05025]

SPS protons:

400 GeV/c

๐Ÿ๐ŸŽ๐Ÿ๐Ÿ Proton on target(PoT)/sec on spill

3.5 sec spill

Page 5: Search for dark photons at NA62 - Institut national de ...moriond.in2p3.fr/QCD/2018/WednesdayMorning/Mirra.pdf21/03/2018 M. Mirra Search for dark photons at NA62 2 Hidden sector motivations

M. Mirra Search for dark photons at NA6221/03/2018 5

NA62 layout

SPS protons:

400 GeV/c

๐Ÿ๐ŸŽ๐Ÿ๐Ÿ PoT/sec on spill

3.5 sec spill

Secondary beam:

75 GeV/c, 1% bite

100 ฮผrad

60 ร— 30 mm2

๐‘ฒ+(6%)/๐…+(70%)/p(24%)

750 MHz at GTK3

[NA62 Detector Paper, JINST 12 (2017), P05025]

Page 6: Search for dark photons at NA62 - Institut national de ...moriond.in2p3.fr/QCD/2018/WednesdayMorning/Mirra.pdf21/03/2018 M. Mirra Search for dark photons at NA62 2 Hidden sector motivations

M. Mirra Search for dark photons at NA6221/03/2018 6

NA62 layout

SPS protons:

400 GeV/c

๐Ÿ๐ŸŽ๐Ÿ๐Ÿ PoT/sec on spill

3.5 sec spill

Secondary beam:

75 GeV/c, 1% bite

100 ฮผrad

60 ร— 30 mm2

๐‘ฒ+(6%)/๐…+(70%)/p(24%)

750 MHz at GTK3

Kaon decay region:

60 m

~5 MHz

๐“ž(10-6) mbar

[NA62 Detector Paper, JINST 12 (2017), P05025]

Page 7: Search for dark photons at NA62 - Institut national de ...moriond.in2p3.fr/QCD/2018/WednesdayMorning/Mirra.pdf21/03/2018 M. Mirra Search for dark photons at NA62 2 Hidden sector motivations

M. Mirra Search for dark photons at NA6221/03/2018 7

NA62 layout

Performances

Excellent time resolution ๐“ž(100 ps) to match beam and daughter particle

information

Kinematics: rejection of main ๐‘ฒ modes 104 via kinematics reconstruction

PID capability: ๐ vs ๐… rejection of O(107) for 15 < p(๐…+) < 35 GeV

High-efficiency veto: 108 rejection of ๐…๐ŸŽ for E(๐…๐ŸŽ) > 40 GeV

[NA62 Detector Paper, JINST 12 (2017), P05025]

Page 8: Search for dark photons at NA62 - Institut national de ...moriond.in2p3.fr/QCD/2018/WednesdayMorning/Mirra.pdf21/03/2018 M. Mirra Search for dark photons at NA62 2 Hidden sector motivations

M. Mirra Search for dark photons at NA6221/03/2018 8

NA62 timescale for ๐‘ฒ+ โ†’ ๐…+๐‚เดค๐‚

Run in 2014: pilot run

Run in 2015: commissioning run

โ€ข commissioning of L0 trigger

โ€ข run up to nominal intensity,

โ€ข 33 ร— 1011 PoT/spill, 3.5 s effective-length spill

Run in 2016: detector commissioning + physics run

โ€ข L1 trigger/detector final commissioning

โ€ข stable run at 40% of the nominal beam intensity

Run in 2017-2018: physics run

โ€ข improve on present state of the art (BNL measurement) collecting ~ 20 SM ๐‘ฒ+ โ†’๐…+๐‚เดฅ๐‚ events before LS2

๐‘ฒ+ โ†’ ๐…+๐‚เดฅ๐‚ physics program

Current run

Page 9: Search for dark photons at NA62 - Institut national de ...moriond.in2p3.fr/QCD/2018/WednesdayMorning/Mirra.pdf21/03/2018 M. Mirra Search for dark photons at NA62 2 Hidden sector motivations

M. Mirra Search for dark photons at NA6221/03/2018 9

NA62 physics besides ๐‘ฒ+ โ†’ ๐…+๐‚เดค๐‚Such high-intensity, high-performance setup as NA62 might be suited for these NP searches:

โ€ข Lepton flavour violation (LFV) and lepton number violation (LNV) studies

โ€ข ultra-rare/forbidden ๐…๐ŸŽ decays

โ€ข chiral perturbation theory studies from kaon decays

โ€ข search for exotic states

Trigger bandwidth for final states other than โ€œ๐…++ Emissโ€ (used for the ๐‘ฒ+ โ†’ ๐…+๐‚เดฅ๐‚)

limited. Some LFV/LNV studies can be performed because involve low-bandwidth trigger

โ€ข 3 daughter tracks at SES ~ 10-11: ๐พ+ โ†’ ๐œ‹+๐œ‡ยฑ๐‘’โˆ“, ๐พ+ โ†’ ๐œ‹โˆ’๐œ‡+๐‘’+, ๐พ+ โ†’ ๐œ‹โˆ’๐‘’+๐‘’+,

๐พ+ โ†’ ๐œ‹ยฑ๐œ‡โˆ“๐œ‡+

others because can be made in parasitic mode with the main trigger:

โ€ข search for heavy neutral leptons in ๐พ+ โ†’ ๐œ‡+๐œˆโ„Ž, ๐พ+ โ†’ ๐‘’+๐œˆโ„Žโ€ข search for ๐œ‹0 โ†’ ๐‘–๐‘›๐‘ฃ๐‘–๐‘ ๐‘–๐‘๐‘™๐‘’, NA62 sensitive at 10-8 , search for ๐œ‹0 โ†’ ๐ดโ€ฒ๐›พ

Page 10: Search for dark photons at NA62 - Institut national de ...moriond.in2p3.fr/QCD/2018/WednesdayMorning/Mirra.pdf21/03/2018 M. Mirra Search for dark photons at NA62 2 Hidden sector motivations

M. Mirra Search for dark photons at NA6221/03/2018 10

Dark photon at NA62

Several production modes / signals of Aโ€™ can be studied at NA62

Search for invisible decays (production in fiducial volume, missing mass signals):

From ๐พ+ beam: for ๐พ+ โ†’ ๐œ‹+๐ดโ€ฒ, by product of ๐‘ฒ+ โ†’ ๐…+๐‚๐‚ [Marciano et al.

PRD 892014]

From ๐พ+ decay daughters: ๐‘ฒ+ โ†’ ๐…+๐…๐ŸŽ, ๐…๐ŸŽ โ†’ ๐‘จโ€ฒ๐œธ

Rate scales with square of coupling

Up with intensity, if no background

limited, improve from above

| Aโ€™ coupling to

ordinary ฮณ|

Aโ€™ mass [GeV]

Page 11: Search for dark photons at NA62 - Institut national de ...moriond.in2p3.fr/QCD/2018/WednesdayMorning/Mirra.pdf21/03/2018 M. Mirra Search for dark photons at NA62 2 Hidden sector motivations

M. Mirra Search for dark photons at NA6221/03/2018 11

Dark photon at NA62

Several production modes / signals of Aโ€™ can be studied at NA62

Search for visible decays to SM particles (production at target/dump)

Production from primary beam secondaries: pN โ†’ ๐‘‹๐œ‹0, ๐œ‹0 โ†’ ๐ดโ€ฒ๐›พ, ๐ดโ€ฒ โ†’ ๐‘™+๐‘™โˆ’

Production from primary beam: pN โ†’ ๐‘‹๐ดโ€ฒ, ๐ดโ€ฒ โ†’ ๐‘™+๐‘™โˆ’

Rate scales with 4th power of coupling

Up with intensity, if no background

limited, improve from below

| Aโ€™ coupling to

ordinary ฮณ|

Aโ€™ mass [GeV]

Sensitivity region shape depends on:

minimum distance from production

point to decay volume (upper curve)

decay volume acceptance (lower curve)

Page 12: Search for dark photons at NA62 - Institut national de ...moriond.in2p3.fr/QCD/2018/WednesdayMorning/Mirra.pdf21/03/2018 M. Mirra Search for dark photons at NA62 2 Hidden sector motivations

M. Mirra Search for dark photons at NA6221/03/2018 12

TAX

NA62 in dump mode

A rich field to be explored with minimal upgrades to the present setup: run in โ€œbeam-

dumpโ€ mode with NP searches for MeV-GeV mass hidden-sector candidates like Dark

photons, Heavy neutral leptons (HNL), Axions/ALP, etc.

proton

High-intensity 400-GeV proton beam: boost charm/beauty, other meson production

1018 PoT / nominal year: 1012 PoT/sec on spill, 100 days/year, 60% run efficiency

1015 D(S), 1014 K, 1018 ๐œ‹0/ฮท/ฮทโ€™/ฮฆ/ฯ/ฯ‰ with ratios 6.4/0.68/0.07/0.03/0.94/0.95

Compact beam dump: ~ 11 I Cu-based

beam-defining collimator (TAX)

Page 13: Search for dark photons at NA62 - Institut national de ...moriond.in2p3.fr/QCD/2018/WednesdayMorning/Mirra.pdf21/03/2018 M. Mirra Search for dark photons at NA62 2 Hidden sector motivations

M. Mirra Search for dark photons at NA6221/03/2018 13

NA62: ๐‘ฒ+ โ†’ ๐…+๐‚เดฅ๐‚, LNV/LFV decays,

hidden sector searches in K decays

Current run

NA62 Run3 plan under discussion

โ€ข Present setup for ๐‘ฒ+ beam + dedicated triggers: LFV/LNV sensitivity studies based:

๐พ+ โ†’ ๐œ‹+๐œ‡ยฑ๐‘’โˆ“, ๐พ+ โ†’ ๐œ‹โˆ’๐œ‡+๐‘’+, ๐พ+ โ†’ ๐œ‹โˆ’๐‘’+๐‘’+, ๐พ+ โ†’ ๐œ‹โˆ’๐œ‡+๐œ‡+ (+ rad. modes)

๐œ‹0 โ†’ ฮผ๐‘’, 3ฮณ, 4ฮณ, ๐‘’๐‘’, ๐‘’๐‘’๐‘’๐‘’

LFV/LNV @ ultimate sensitivity,

hidden sector searches (beam dump)

Run 3

โ€ข 1018 POT in run in โ€œbeam-dumpโ€ mode, new program of NP searches for MeV-GeV mass

hidden-sector candidates: Dark photons, Heavy neutral leptons, Axions/ALPโ€™s, etc.

LS2 LS2

protonAny kind of feebly-interacting

long-lived particle

(put here your favored model)

Dark scalars

Aโ€™

HNLmuons

neutrinos

โ€ข If needed, run for refining ๐‘ฒ+ โ†’ ๐…+๐‚เดฅ๐‚

Page 14: Search for dark photons at NA62 - Institut national de ...moriond.in2p3.fr/QCD/2018/WednesdayMorning/Mirra.pdf21/03/2018 M. Mirra Search for dark photons at NA62 2 Hidden sector motivations

M. Mirra Search for dark photons at NA62

Minimum bias

data: 2 ฮณ on

LKr, simulate

1g loss

Data control

trigger: 2 ฮณ

on LKr,

simulate 1g

loss

MC:

- mAโ€™ = 60 MeV- mAโ€™ = 90 MeV- mAโ€™ = 120 MeV

21/03/2018 14

Mmiss2 (GeV2)

NA62 2016 data: dark photon from ๐…๐ŸŽ decay

Decay chain: ๐‘ฒ+ โ†’ ๐…+๐…๐ŸŽ, ๐…๐ŸŽ โ†’ ๐‘จโ€ฒ๐œธ, ๐‘จโ€ฒ โ†’ ๐’Š๐’๐’—๐’Š๐’”๐’Š๐’ƒ๐’๐’†

Signature:

โ€ข 1 photon + missing energy

Selection:

โ€ข ๐œ‹+ as in ๐พ+ โ†’ ๐œ‹+๐œˆ าง๐œˆโ€ข 15<๐‘๐œ‹+<35 GeV/c

โ€ข 1 ๐›พ in LKr

โ€ข Missing momentum in LKr

โ€ข Extra ๐›พ veto

Background:

โ€ข Negative tail of ๐‘€๐‘š๐‘–๐‘ ๐‘ 2

Normalization:

โ€ข ๐พ+ โ†’ ๐œ‹+๐œ‹0 from minimum bias

๐‘ด๐’Ž๐’Š๐’”๐’”๐Ÿ = ๐‘ท๐‘ฒ โˆ’ ๐‘ท๐… โˆ’ ๐‘ท๐œธ

๐Ÿ

NA62

Preliminary

Page 15: Search for dark photons at NA62 - Institut national de ...moriond.in2p3.fr/QCD/2018/WednesdayMorning/Mirra.pdf21/03/2018 M. Mirra Search for dark photons at NA62 2 Hidden sector motivations

M. Mirra Search for dark photons at NA6221/03/2018 15

MAโ€™

(MeV)

e

Limit found

1-s limit band

2-s limit band

NA62

NA62 2016 data: dark photon from ๐…๐ŸŽ decay

e

MAโ€™ (GeV)MAโ€™ (MeV)

NA62

Preliminary

NA62

Preliminary

Limits observed are statistically compatible with fluctuations from the background-only hypothesis

NA62 limits in an interesting

region; #๐‘ฒ decays ~ 1.5 ร— 1010

(4% 2016 statistics) used

Limit if

Nobs = Nbkg

Page 16: Search for dark photons at NA62 - Institut national de ...moriond.in2p3.fr/QCD/2018/WednesdayMorning/Mirra.pdf21/03/2018 M. Mirra Search for dark photons at NA62 2 Hidden sector motivations

M. Mirra Search for dark photons at NA6221/03/2018 16

Search for visible decays of long-lived Aโ€™

Assume 1018 400-GeV PoT:

โ€ข Aโ€™ produced (meson decays, bremsstrahlung) from interaction into target

โ€ข search for displaced, dilepton decays of dark photons, ๐ดโ€ฒ โ†’ ๐œ‡๐œ‡, ๐‘’๐‘’โ€ข include trigger/acceptance/selection efficiency

โ€ข assume zero-background, evaluate expected 90%-CL exclusion plot

Sensitivity expected

to be even higher

including direct QCD

production of Aโ€™ and

production in the

dump (only target

considered here)

| Aโ€™ coupling to

ordinary ฮณ|2

Aโ€™ mass [MeV]

3 ร— 1017 PoT acquired in 2016/17 with di-muon parasitic trigger, 5 ร— 1016 PoT with ee trigger

Page 17: Search for dark photons at NA62 - Institut national de ...moriond.in2p3.fr/QCD/2018/WednesdayMorning/Mirra.pdf21/03/2018 M. Mirra Search for dark photons at NA62 2 Hidden sector motivations

M. Mirra Search for dark photons at NA6221/03/2018 17

Zero background assumption: 2016 data

Statistics corresponds to ~1015 PoT, search for ๐‘จโ€ฒ โ†’ ๐๐

Track quality + acceptance cuts: forward detectors, CHOD, LKr, MUV3 associated to CHOD,

LKr hits in time

Vertex quality: two-track distance < 1 cm

Vertex position: 105 < Z < 165 m

Test if total momentum ๐‘ท๐’•๐’๐’• = ๐‘ท๐ + ๐‘ท๐stems from target

All two tracks vertices

Impact parameter of ๐‘ท๐’•๐’๐’• to beam

line [cm]

Z of closest approach of ๐‘ท๐’•๐’๐’• to beam line [m]

Signal

region

Background from ๐‘ฒ, ๐… decays

concentrated around beam after final

collimator

๐‘ท๐’•๐’๐’•๐‘ท๐

๐‘ท๐

NA62

Preliminary

0 40 80 120 160 200 240

Page 18: Search for dark photons at NA62 - Institut national de ...moriond.in2p3.fr/QCD/2018/WednesdayMorning/Mirra.pdf21/03/2018 M. Mirra Search for dark photons at NA62 2 Hidden sector motivations

M. Mirra Search for dark photons at NA6221/03/2018 18

Statistics corresponds to ~1015 PoT, search for ๐‘จโ€ฒ โ†’ ๐๐

Track quality + acceptance cuts: forward detectors, CHOD, LKr, MUV3 associated to CHOD,

LKr hits in time

Vertex quality: two-track distance < 1 cm

Vertex position: 105 < Z < 165 m

Test if total momentum stems from target

Further event-level veto conditions:

Additional energy in the LKr < 2 GeV

Veto on forward / large angle calorimeters

Veto on charged anti counter

No events selected in the signal region

(even with standard ๐‘ฒ+ beam)

All vetoes + 10 < ฯ (vertex) < 50 cm

Impact parameter of ๐‘ท๐’•๐’๐’• to beam

line [cm]

Z of closest approach of Ptot to beam line [m]

Signal

region

NA62

Preliminary

0 40 80 120 160 200 240

Zero background assumption: 2016 data

Page 19: Search for dark photons at NA62 - Institut national de ...moriond.in2p3.fr/QCD/2018/WednesdayMorning/Mirra.pdf21/03/2018 M. Mirra Search for dark photons at NA62 2 Hidden sector motivations

M. Mirra Search for dark photons at NA6221/03/2018 19

Heavy neutrino invisible decay: 2015 dataNew result released in 2018 from minimum bias data equivalent to 3ร—108 ๐‘ฒ+ decays

analyzed in๐‘ฒ+ โ†’ ๐’†+๐‚ search and to 1ร—108 ๐‘ฒ+ decays analyzed in the ๐‘ฒ+ โ†’ ๐+๐‚ search

[NA62 coll. PL B778 137 (2018)]

HNL mass [MeV]

Squared missing

mass: ๐‘ท๐‘ฒ โˆ’ ๐‘ท๐’†๐Ÿ

[GeV2]

UL

on

๐‘ผ๐’๐Ÿ’

๐Ÿa

t

90

% C

L

No heavy neutrino signal observed;

improvement on ๐‘ผ๐’†๐Ÿ’๐Ÿ and ๐‘ผ๐๐Ÿ’

๐Ÿ

Major improvements with NA62

2016-2018 higher intensity data sets

and fully operational beam tracker

Squared missing mass:

๐‘ท๐‘ฒ โˆ’ ๐‘ท๐๐Ÿ

[GeV2]

Page 20: Search for dark photons at NA62 - Institut national de ...moriond.in2p3.fr/QCD/2018/WednesdayMorning/Mirra.pdf21/03/2018 M. Mirra Search for dark photons at NA62 2 Hidden sector motivations

M. Mirra Search for dark photons at NA6221/03/2018 20

Conclusions

NA62 is officially approved to run until LS2 with the main goal of

collecting ~ 20 SM ๐‘ฒ+ โ†’ ๐…+๐‚เดฅ๐‚ events before LS2.

Before LS2 (2018) many searches in the hidden sector will be performed

using the kaon beam (new limits on dark photon already investigated).

After LS2 (2020++) there is a window of opportunity to run NA62 in beam-

dump mode to search for hidden particles from charm and beauty decays

and pave the way for the next generation experiments.

The current NA62 run can be exploited to evaluate background rejection

capability up to ~1017-1018 POT. Preliminary studies with data taken in

beam and beam-dump modes show that the background can be kept under

control, further improvements in the setup are currently under study.

Page 21: Search for dark photons at NA62 - Institut national de ...moriond.in2p3.fr/QCD/2018/WednesdayMorning/Mirra.pdf21/03/2018 M. Mirra Search for dark photons at NA62 2 Hidden sector motivations

M. Mirra Search for dark photons at NA6221/03/2018 21

Backup slides

Page 22: Search for dark photons at NA62 - Institut national de ...moriond.in2p3.fr/QCD/2018/WednesdayMorning/Mirra.pdf21/03/2018 M. Mirra Search for dark photons at NA62 2 Hidden sector motivations

M. Mirra Search for dark photons at NA6221/03/2018 22

Search for visible decays of HNL

Assume 1018 400-GeV PoT:

โ€ข search for displaced, leptonic decays HNL โ†’ ฯ€e, ฯ€ฮผ, HNL production at the TAX

โ€ข include trigger/acceptance/selection efficiency

โ€ข separately address 3 extreme coupling scenarios [Shaposhnikov, Gorbunov

arXiv:0705.1729v2]

โ€ข assume zero-background, evaluate expected 90%-CL exclusion plot

1018 PoT acquired in 2016/17 with ฮผฯ€ parasitic trigger, few 1016 PoT with eฯ€ trigger

Page 23: Search for dark photons at NA62 - Institut national de ...moriond.in2p3.fr/QCD/2018/WednesdayMorning/Mirra.pdf21/03/2018 M. Mirra Search for dark photons at NA62 2 Hidden sector motivations

M. Mirra Search for dark photons at NA6221/03/2018 23

Search for visible decays of ALP

Assume 1018 400-GeV PoT:

โ€ข study ALP Primakoff production [JHEP 1602 (2016) 018] at target

โ€ข search for ALP-decay to ฮณฮณ in NA62 fiducial volume, account for geometrical acceptance

โ€ข assume zero-background, evaluate expected 90%-CL exclusion plot

ALP mass [GeV]

ALP-ฮณ coupling

[GeV-1]

Improvements expected already with 1 day of run (1.3 ร— 1016 POT)

Analysis of 2017 data for ~5 ร— 1015 PoT taken in dump mode in progress