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Greetings to Veljko from Fermilab December 9, 2010

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Page 1: Greetings to Veljko from Fermilab December 9, 2010

Greetings to Veljko from Fermilab

December 9, 2010

Page 2: Greetings to Veljko from Fermilab December 9, 2010

Veljko Radeka Symposium, December 9, 20102

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Frontiers of particle physics

• Question: Why have we not seen all the particle physics phenomena yet?

1. The phenomena involve objects that are hard to make (e.g. black holes, heavy gluinos)

2. The phenomena involve interactions that are fundamentally weak – thus very rare

3. The phenomena involve interactions that are very short range – thus very rare

• In case #1, proceed to Energy or Cosmic Frontiers

• In cases #2 and #3, we can use high intensities to observe rare phenomena

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Gaps and roles: intensity frontier

• Two principal approaches: 1) proton super-beams to study neutrinos and rare decays and 2) quark factories: in e+e- and LHCb

• Principal gap is the understanding of neutrinos and the observation of rare decays coupled to new physics processes

• Fermilab strategy: develop the most powerful set of facilities in the world for the study of neutrinos and rare processes, way beyond the present state of the art. Complementary to LHC and with discovery potential beyond LHC. DOE has the central role.

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Roles: intensity frontier

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MINOSMiniBooNEMINERvASeaQuest

NOvAMicroBooNEg-2?SeaQuest

Now 2016

LBNEMu2e

Project X+LBNEm, K, nuclear, …n Factory ??

2013 2019 2022

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Project X Reference Design

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Project X Siting

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Project X Capabilities

• > 2 MW delivered to a neutrino target at any energy between 60 – 120 GeV

• Simultaneous delivery of ~3 MW of high duty factor beam power to the 3 GeV program Variable beam formats to multiple users CW beam at time scales >1 msec 10% duty factor on time scales < 1 msec

• Potential for development of additional programs at: 1 GeV for nuclear energy experimentation 8 GeV for neutrino or muon experimentation

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Project X is central to the strategy

• Unique facility for rare decays: a continuous wave (CW), very high power, superconducting 3 GeV linac. Will not exist anywhere else

• CW linac greatly enhances the capability for rare decays of kaons, muons

• CW linac is the ideal machine for other uses: Standard Model tests with nuclei (ISOL targets), possible energy and transmutation applications, cold neutrons

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Project X is central to the strategy

• Coupled to an 8 GeV pulsed LINAC and to the Recycler and Main Injector, gives the most intense beams of neutrinos at high energy (LBNE) and low energy (for the successors to Mini and MicroBooNE)

• Makes use of modern accelerators at Fermilab (Recycler and Main Injector) and its scope would be difficult to reproduce elsewhere without this established base

• Eliminates proton economics as the major limitation: all experiments run simultaneously

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Project X and other projects

• Project X benefits from the word-wide ILC R&D: SCRF and photo-e cloud. SCRF R&D positions the US to play a leading role in ILC.

• Capabilities and infrastructure developed for Project X will be useful for other domestic non HEP projects.

• Project X with upgrades can be the front end of a neutrino factory or a muon collider, opening paths for development of the intensity frontier and a road back to the energy frontier

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LBNE and DUSEL

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JPARC

Intensity Frontier: Neutrino Beams

Fermilab Soudan (735km) CERN Gran Sasso (732km) J-PARC Kamioka (295km) Ash river(810km) 300 kW 700 kW 50 kW 100 kW ( 750 kW)

MINOS, MINERvA, MiniBooNE OPERA T2K NOvA

Fermilab CERNKEK

Fermilab

CERN

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Comparative situation: Asia

J-PARC

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Requires upgrade to JPARC, new detectors

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MEMPHYS 450 Ktons

LENA 50 ktons

GLACIER 100 ktons

LAGUNA

Comparative situation: Europe

CERN

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Reuires Project X and new synchrotron at CERN

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US: Long Baseline Neutrino ExperimentCD 0: January 2010

1300 km

Collaboration:288 members from 54 institutions (India, Italy, Japan, UK, US)

Continue to grow!

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DUSEL Lab Layout

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Far detector: Water Cherenkov at 4850L

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DUSEL 4850L Campus

Proton decay limit > 6x1034 years for e+p final state in 10 years

Fiducial mass for each: 100 kton

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Far detector: LAr TPC at 800L

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LAr TPC in 800L facility with cosmic ray veto to enable proton decay (K+n) search.

Proton decay limit > 3x1034 years for K+n final state in 10 years

(Fiducial mass for each: 17 kton)

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Facility Overview: LAr TPCs

South Portal (new)Cryogenics building

Kirk Drift (existing)At 300 level

North Portal (new)Access to cavern

300’ elevation

Ross Headframe

Yates Headframe

Kirk Road

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Various configurations: scorecard

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LAr TPC is a great choice

Need extremely good LAr purity, low convective flow

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Time Projection Chamber (TPC)

168 APAs (each 250kg, 3840 chan)224 CPAs (each 100kg, HV @125 kV)Field cageCryogenic ASIC electronicsPower, signal cables, feedthroughs, HV

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Detector Overview

2.5m

168 Anode Plane Ass’y (APA) 656k channels

Standard wire chamber construction

225 Cathode Plane Ass’y (CPA) - SS mesh

2016 PMT Ass’y

Membrane cryostat

2.5m

Field cage wraps detector

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LAr20 Front-End Electronics: Veljko next career!LAr20 Front-End Electronics: Veljko next career!

Collaboration• BNL• FNAL• Georgia Tech.• SMU

Functionality and multiplexing ratios will depend on chosen readout architecture

16 channel mixed-signal

digital

Copper or Optical

Driver

Veljko !

Veljko !

Veljko !

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Neutrino physics sensitivities

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With Project X