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The OPERA experiment 1 CERN LNGS 730 km OPERA Neutrinos 1400 m Designed in 2000 to search for Neutrino Oscillations via the detection of tau neutrinos First neutrinos from CERN detected in 2006

The OPERA experiment

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The OPERA experiment. CERN. 730 km. LNGS. 1400 m. Neutrinos. OPERA. Designed in 2000 to search for Neutrino Oscillations via the detection of tau neutrinos First neutrinos from CERN detected in 2006. CERN. 730 km. LNGS. Neutrino velocity measurement Neutrinos production time (CERN) - PowerPoint PPT Presentation

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Page 1: The OPERA experiment

The OPERA experiment

1

CERN

LNGS

730 km

OPERA

Neutrinos

1400 m

Designed in 2000 to search for Neutrino Oscillations via the detection of tau neutrinos

First neutrinos from CERN detected in 2006

Page 2: The OPERA experiment

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• High neutrino energy - high statistics ~15000 events• Precise measurement of neutrino time distribution at CERN through proton

waveforms• Sophisticated timing system: ~1 ns CNGS-OPERA synchronization• Calibrations techniques of CNGS and OPERA timing chains: ~ 1 ns level • Measurement of baseline by global geodesy: 20 cm accuracy over 730 km (longest neutrino baseline actually available)

Result: ~10 ns overall accuracy on TOF with similar stat. and sys. errors

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Neutrino velocity measurement

Neutrinos production time (CERN)Neutrinos interaction time (OPERA detector)

Accurate determination of the distance (Geodesy)

Dedicated upgrade in 2008Largest application of metrology techniques in HEP

2009-2011 measurement with standard CNGS beam Blind analysis: “box” opened after assessment of delays (previously fixed to arbitrary values):

Time

Space

CERN

LNGS

730 km

Page 3: The OPERA experiment

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Summary of the principle for the TOF measurement

Measure t =TOFc - TOF 3

z

y x

3

Page 4: The OPERA experiment

Protons timing

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Beam CurrentTransformer

Recorded waveform of a pulse of protons10.5 s

2 km

Page 5: The OPERA experiment

CERN

Atomic clock Cs 4000

GPSPolaRx2e

LNGS

ESAT 2000

5

CERN

GPSPolaRx2e

Atomic clock Cs 4000

Page 6: The OPERA experiment

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GPS

GPS

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Geodesy at LNGS

Dedicated measurements at LNGS: July-Sept. 2010

2 new GPS benchmarks on each side of the 10 km highway tunnel ported underground to OPERA

CERN and LNGS measurements combined in ETRF2000

(731278.0 ± 0.2) m (731278.0 ± 0.2) m

Distance CERN BCT-OPERA

Monitor continental drift and important geological events (e.g. 2009 earthquake)

Page 7: The OPERA experiment

Neutrino data vs protons: after delay determination (2009-2011) ~15000 neutrinos

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BLIND: t = TOFc-TOF =(1043.4 ± 7.8) ns

Dots: neutrino eventsRed line: protons

Blind cross-checks: Accuracy of analysis method Stability in the 3 years Day/night Warm/cold External interactions Running conditions

Page 8: The OPERA experiment

OPENING OF THE BOX

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• The OPERA detector at LNGS in the CERN CNGS muon neutrino beam has allowed the most sensitive terrestrial measurement of the neutrino velocity over a baseline of about 730 km.

• Despite the large significance of the measurement reported here and the stability of the analysis, the potentially great impact of the result motivates the continuation of our studies in order to identify any still unknown systematic effect.

• We do not attempt any theoretical or phenomenological interpretation of the results.

March 2011 very surprising result neutrinos anticipate light by 60 ns (20 m over 730 km) 6 months of verifications campaign: synchronization, geodesy, detector, accelerator, each aspect of the measurement cross-checked with at least two independent techniques UNBLIND: t = (57.8 ± 7.8 (stat.) -5.9 +8.3 (sys.)) ns

September 2011, anomaly still alive involve the rest of the physics community in order to help in understanding its nature, speed up the investigation and try to replicate the effect under different conditions

Seminar at CERN (23/9/2011) and simultaneous publication of all the elements of the measurement:

Page 9: The OPERA experiment

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Measurement with a dedicated beam (November 2011)

t = TOFc-TOF= (62.1 ± 3.7 (stat.)) ns

10.5 s

A beam of very short pulses (3ns) separated by long empty intervals

Time of flight individually measured for 20 neutrinos in one week

1 s

Page 10: The OPERA experiment

1010

Further investigations since November 2011 Discussion of a new bunched beam campaign (indicative date May 2012) with improved beam performance (100 ns bunch spacing, a factor 3 more intensity). More accurate study for possible energy dependence and measurement with anti-neutrinos. Other LNGS experiments (ICARUS, BOREXINO, LVD) involved.

Development of a new time-transfer system at CERN and LNGS based on the White-Rabbit protocol (self-calibrating continuous delay measurement)

Developments for DAQ upgrade for May 2012 run by including TDCs at the level of the Master clock (±25 ns jitter) and FE sensors (± 5 ns jitter)

Additional checks on the Geodesy at CERN on the underground transport of external GPS measurements

Additional checks on GPS timing with a two-way satellite transfer measurement and possible time-transfer via optical fibers

Additional measurements at LNGS (winter 2011 shutdown): identified two unknown sources of bias on TOF, going in opposite directions (22 Feb. 2012)

Page 11: The OPERA experiment

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New direct measurement campaign of 10-24 May 2012:

1) Improvements in OPERA timingNew OPERA master clock installed a)Better timing time resolution twice betterb)Better local oscillator, small frequency offset 5ns/s (124 ns/s old oscillator)c)Continuous monitoring of the local oscillator frequency and fiber transmission delay using the “White Rabbit” systemd) Better stability of Master Clock delay response with respect to light input from the fiber

2) Improvements in the CNGS beam timing structureNovember 2011: 4 short bunches separated by 524 nsMay 2012: 64 short bunches separated by 100 ns

3) Improvements in timing equipment systematicsa)Double GPS systemb)White Rabbit monitoring of all time transfer delays at CERN and LNGSc)Beam Current Transformer (BCT) calibration redone. Before: BCT systematic error of 5 ns (the largest sys. error affecting the measurement). Now: only 1 ns !

106 events collected59 events selected by the analysis cuts (factor 3 better statistics, factor 2 better resolution, redundancy)

Page 12: The OPERA experiment

The CNGS neutrino beam

• 40000 billions of protons accelerated to 400 GeV energy

• Every 6 s two pulses of 10.5 s (50 ms gap)

• Almost pure beam (average energy = 17 GeV) 12

Page 13: The OPERA experiment

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“INTERNAL”EVENTS

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CC

NC

from external interaction

Neutrinos seen by the OPERA detector

“EXTERNAL”EVENTS

(interactions in the rock)

Page 14: The OPERA experiment

Standard GPS receiver:

finds x, y, z, t of the observer with ≥ 4 satellite observations, by solving 4 equations in 4 unknowns

If x, y, z are fixed one satellite enough to measure t

Common-view mode:

same satellite seen at the two sites

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The GPS “a marvelous tool”

Special GPS receiver + atomic clock Time-transfer (~1 ns accuracy )

Used in the definition of TAI (International Atomic Time)