Experimental Particle Physics at SLAC. John Jaros Stanford Graduate Student Orientation September 17, 2015

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Transcription:

Experimental Particle Physics at SLAC John Jaros Stanford Graduate Student Orientation September 17, 2015

The Best of Times We ve found the Higgs but have just scratched the surface of what a new, fundamental scalar means for particle physics The LHC is offering us our first glimpse of the highest energy collisions ever made on earth 13 TeV. What new physics is waiting to be discovered? Neutrinos have mass and mix! Pinning down masses, mixing angles, and CP violation in the neutrino sector could lead to understanding why baryons dominate anti-baryons in the universe. Dark Matter detection could be just around the corner! Will it be Wimps, Axions, Hidden Sector Particles, or something we haven t yet imagined? 2

Job Security 96% of the Mass and Energy in the Universe has yet to be accounted for. Particle Physics has just begun! Standard Model fits here! 3

Big Questions motivate SLAC s Experiments What exactly is the Higgs? Are there new particles, new forces, hidden sectors? ATLAS Experiment at the Large Hadron Collider (LHC) Heavy Photon Search at JLAB 4

Big Questions motivate SLAC s Experiments What is the nature of the neutrino? What can neutrino mixing reveal? Enriched Xenon Observatory (EXO200 and nexo) DUNE, MicroBooNE, and ICARUS 5

ATLAS Experiment at LHC World s most powerful particle accelerator Explorations at the energy frontier * Understanding the Higgs boson Does it give neutrinos mass? Does it couple to Dark Matter? Are there more Higgses? * Searching beyond the Standard Model Are there WIMPS at LHC? High mass SUSY? Unprecedented detector capabilities for a hadron collider: * Lives in a hostile radiation environment * Extremely high rate capability * Disentangles ~25 overlapping events 6

SLAC/ATLAS Physics Higgs SUSY Searches g b/ t b/ t b/ t LSP g b/ t LSP b/ t b/ t 7

Physics Event Reconstruction Pileup Jet substructure Tagging Machine learning 8

Research opportunities Detector activities: o State-of-the-art data acquisition concept for high luminosity upgrade o Pixel detector upgrade and sensors o Trigger algorithms and online infrastructure Physics analysis and development of physics tools: o Jet substructure techniques o Higgs bb and beyond the Standard Model Higgs searches o Super-symmetry searches o Searches for new phenomena Collaborate with Prof. Lauren Tompkins on Campus 9

SLAC ATLAS contact info Prof. Ariel Schwartzman sch@slac.stanford.edu Prof. Su Dong sudong@slac.stanford.edu Dr. Charlie Young young@slac.stanford.edu Detailed info on ATLAS@SLAC for students: http://www.slac.stanford.edu/exp/atlas/students/ 10

Heavy Photon Search Evidence for Dark Matter is compelling, but there s still no direct evidence for Dark Matter particles. The absence of SUSY at the LHC is stimulating non-wimp explanations for Dark Matter. Dark matter may reside in a hidden sector, carry an analogue of electric charge and couple to a heavy photon (A ). Heavy photons will mix with regular photons, so they can be produced by, and decay into electrons and positrons. The Heavy Photon Search looks for a new vector gauge boson (a heavy photon) radiated by electron beams, decaying to e + e -. 11

HPS Setup at JLAB Si Vertex Tracker PbWO 4 Electromagnetic Calorimeter e - The JLAB electron beam is directed onto a W foil target, producing heavy photons. They decay to e + e - pairs, which are measured by the Si vertex tracker inside an analyzing magnet. The PbWO 4 ECal provides a fast trigger. https://confluence.slac.stanford.edu/display/hpsg/heavy+photon+search+experiment 12

Beam s Eye View of SVT The beam goes here! 13

Status and plans HPS was installed, commissioned, and took its first data in an Engineering Run at JLAB this past Spring. Physics Running is planned for 2015-2016 and 2017-2018 HPS will search a large and unexplored region of the A mass/coupling plane 2015 Running (1 GeV) 2016 Running (2 & 4 GeV) 14

Opportunities for students Opportunities for new students 2015-16 Data taking, analysis, and planning upgrades 2016-17 Build and install HPS upgrades 2017-19 Data taking and analysis Learn the trade Data for theses Small Experiments provide training in all aspects of HEP experimentation Physics Analysis Experiment design State of the art hardware construction Running experiments Contact: Prof John Jaros (john@slac.stanford.edu) Rotation Projects are available on HPS this year: https://confluence.slac.stanford.edu/display/hpsg/stanford+rotation+projects+in+heavy+photon+search 15

Enriched Xenon Observatory half life neutrino mass Search for neutrino-less double beta decay of Xe-136 2 modes of ββdecay: o (2νββ): allowed in SM, but extremely rare process (halflife~10 20 years) o (0νββ): only 2 electrons are emitted Lepton number violation (not allowed in the SM) Only possible if neutrinos have mass and are Majorana particles (neutrino=anti-neutrino) EXO-200 discovered the (2νββ) decay mode in Xe, provides the most precise measurement of any (2νββ) rate and has demonstrated the best sensitivity to the (0νββ) decay mode 16

EXO-200 Experiment 500m underground in New Mexico TPC (Time Projection Chamber) measures energy (scintillation light in photo-detectors) and longitudinal position (from drift time) o o Signal reconstructed as single-cluster events Gamma-ray backgrounds produce multiple clusters 17

The Next Step: nexo R&D for a ton-scale experiment 5 tons of enriched 136 Xe Improved charge/light collection, spatial and energy resolution. Second phase may employ Ba daughter ion identification. 5-year reach in half life ~100 times EXO-200 performance 130 cm 46 cm 18

Opportunities for students Design and prototype the nexo TPC Conduct R&D for HV field cage design and LXE purity for nexo Signal pulse fitting Characterize photodetectors for LXe Develop detector electronics for operations at LXe temperature (165 K) to reduce noise Develop Ba ++ extraction and identification * Mechanical probe development EXO-200 event reconstruction/calibration * Improve efficiency and background rejection * Compare calibration source data with simulation There are many opportunities for rotation students which could lead into an EXO-200 thesis and provide a strong background in detector R&D 19

EXO Contact info Prof. Martin Breidenbach mib@slac.stanford.edu EXO-200 Prof. Giorgio Gratta gratta@stanford.edu EXO-200/nEXO Dr. Peter Rowson rowson@slac.stanford.edu EXO-200/nEXO 20

Beam Neutrino Experiments Address very fundamental questions o What is the nature of the neutrino? Is there CP in the lepton sector? SLAC group is working on three experiments, all based on Liquid Argon Time Projection Chambers (LArTPC) o Deep Underground Neutrino Experiment (DUNE) Measures neutrino oscillations at long baseline (1300 km) Flagship US Accelerator program, takes data after 2020 o MicroBooNE Searching for oscillations at short baseline (800 m) Currently commissioning detector with cosmic rays First beam data expected Fall 2015 (perfect timescale for new students) o ICARUS Pioneered LArTPC technique Will be moved to Fermilab to augment MicroBooNE First beam data expected in 2018 21

MicroBooNE Status Installation finished 2014 Commissioning underway Very exciting time on MicroBooNE! First beam events expected 2015 22

Opportunities for Students Short-term opportunities o o o MicroBooNE commissioning, initial data-taking and physics analysis ICARUS transition to Fermilab learn to operate with high rates and high backgrounds Learn LArTPC technology from the world s experts Longer-term opportunities o DUNE experiment will be flagship on-shore US experiment in 2020 s o Opportunity to contribute to its design and become an expert in LArTPCs and neutrino physics Current SLAC roles (on all three experiments) o o o o High-speed Data Acquisition systems Automated event reconstruction Studies of SuperNova burst neutrino detection 23

Neutrino Contact info Dr. Mark Convery convery@slac.stanford.edu 24

Summary Current SLAC particle physics experiments address some of the most important questions in physics today: o What is the origin of mass? o What constitutes the Dark Matter? o Are there new particles or Hidden Sectors? o What is the nature of the neutrino? It s a propitious time for particle physics. Powerful new experimental tools can fundamentally change our understanding of the universe. SLAC plays a major role in designing future experiments SLAC is developing state-of-the-art detector and readout technologies and advanced analysis and computing techniques. 25