The Compact Muon Solenoid (CMS) experiment. at the Large Hadron Collider (LHC)

Similar documents
4. LHC experiments Marcello Barisonzi LHC experiments August

Particle + Physics at ATLAS and the Large Hadron Coillder

Dr. Andrea Bocci. Using GPUs to Accelerate Online Event Reconstruction. at the Large Hadron Collider. Applied Physicist

Recent CMS results on heavy quarks and hadrons. Alice Bean Univ. of Kansas for the CMS Collaboration

Introduction to CERN and CMS

LHC & ATLAS. The largest particle physics experiment in the world. Vincent Hedberg - Lund University 1

The Why, What, and How? of the Higgs Boson

Saeid Paktinat School of Particles and accelerators IPM, Tehran

ATLAS EXPERIMENT : HOW THE DATA FLOWS. (Trigger, Computing, and Data Analysis)

Particle detection 1

Unravelling the Mysteries of Matter with the CERN Large Hadron Collider An Introduction/Overview of Particle Physics

The Compact Muon Solenoid Experiment. Conference Report. Mailing address: CMS CERN, CH-1211 GENEVA 23, Switzerland. Commissioning of the CMS Detector

Introduction of CMS Detector. Ijaz Ahmed National Centre for Physics, Islamabad

An Introduction to Particle Physics

2 ATLAS operations and data taking

Particle Detectors for

The Large Hadron Collider, a marvel of technology Lyn Evans. Royal Institution of South Wales St David s day lecture, 16 th March 2017

Identifying Particle Trajectories in CMS using the Long Barrel Geometry

Particle accelerators

Top Physics at CMS. Intae Yu. Sungkyunkwan University (SKKU), Korea Yonsei University, Sep 12 th, 2013

Last Friday: pp(bar) Physics Intro, the TeVatron

PoS(EPS-HEP 2013)508. CMS Detector: Performance Results. Speaker. I. Redondo * CIEMAT

The Big-Bang Machine. Stefan Spanier Physics and Astronomy University of Tennessee, Knoxville. 25 February 2017 Stefan Spanier, The Big Bang Machine

The Particle World. This talk: What is our Universe made of? Where does it come from? Why does it behave the way it does?

Analyzing CMS events

SUSY Search at CMS. Jet+MET+0 lepton analysis Jet+MET+leptons analysis MET independent analysis Conclusions

The Discovery of the Higgs Boson: one step closer to understanding the beginning of the Universe

The Search for the Higgs Boson, and the CMS Project

I. Antoniadis CERN. IAS CERN Novice Workshop, NTU, 7 Feb 2014

(a) (b) Fig. 1 - The LEP/LHC tunnel map and (b) the CERN accelerator system.

The ATLAS Detector - Inside Out Julia I. Hofmann

PoS(DIS 2010)190. Diboson production at CMS

Future prospects for the measurement of direct photons at the LHC

Search for a Z at an e + e - Collider Thomas Walker

The God particle at last? Astronomy Ireland, Oct 8 th, 2012

Elementary Particle Physics Glossary. Course organiser: Dr Marcella Bona February 9, 2016

b Physics Prospects For The LHCb Experiment Thomas Ruf for the LHCb Collaboration Introduction Detector Status Physics Program

The God particle at last? Science Week, Nov 15 th, 2012

The rejection of background to the H γγ process using isolation criteria based on information from the electromagnetic calorimeter and tracker.

Particle Physics at the Energy Frontier. Kevin Stenson University of Colorado Boulder October 23, 2006

How and Why to go Beyond the Discovery of the Higgs Boson

7 Physics at Hadron Colliders

CMS Note Mailing address: CMS CERN, CH-1211 GENEVA 23, Switzerland

THE ATLAS TRIGGER SYSTEM UPGRADE AND PERFORMANCE IN RUN 2

CMS Event Simulation

How and Why to go Beyond the Discovery of the Higgs Boson

LHC Detectors and their Physics Potential. Nick Ellis PH Department, CERN, Geneva

READINESS OF THE CMS DETECTOR FOR FIRST DATA

Compact Muon Solenoid Surapat Ek-In École Polytechnique Fédérale de Lausanne

The Hunt for the Higgs (and other interesting stuff at the Tevatron) Robert Roser Fermi National Accelerator Laboratory

The Alice Experiment Felix Freiherr von Lüdinghausen

Digital Calorimetry for Future Linear Colliders. Tony Price University of Birmingham University of Birmingham PPE Seminar 13 th November 2013

Frontier Particle Accelerators

Discovery of the W and Z 0 Bosons

Year- 1 (Heavy- Ion) Physics with CMS at the LHC

The Compact Muon Solenoid Experiment. Conference Report. Mailing address: CMS CERN, CH-1211 GENEVA 23, Switzerland. First Physics at CMS

Collider Physics Analysis Procedures

CMS Status and the US-CMS DAQ projects

Analysis of a Potential Tracking Algorithm for the SLHC Upgrade

PERFORMANCE OF THE ATLAS MUON TRIGGER IN RUN 2

The achievements of the CERN proton antiproton collider

CMS Conference Report

Top Physics in Hadron Collisions

QCD cross section measurements with the OPAL and ATLAS detectors

The Start of the LHC Era. Peter Wittich Laboratory of Elementary Particle Physics Cornell University

The Discovery of the Higgs boson Matthew Herndon, University of Wisconsin Madison Physics 301: Physics Today. M. Herndon, Phys

Modern Accelerators for High Energy Physics

The ATLAS Experiment and the CERN Large Hadron Collider

The Collider Detector at Fermilab. Amitabh Lath Rutgers University July 25, 2002

Search for Displaced Supersymmetry using the Compact Muon Solenoid Detector

Conference Report Mailing address: CMS CERN, CH-1211 GENEVA 23, Switzerland

PoS(CORFU2016)060. First Results on Higgs to WW at s=13 TeV with CMS detector

Optimizing Selection and Sensitivity Results for VV->lvqq, 6.5 pb -1, 13 TeV Data

Walter Hopkins. February

Observation of a New Particle with a Mass of 125 GeV

Physics with Jets at the LHC

A Search for Doubly Charged Higgs Production at 8 TeV Using the CMS Detector at the LHC

ATLAS Z-Path Masterclass 2013

A glance at LHC Detector Systems. Burkhard Schmidt, CERN PH-DT

Introduction to the Standard Model

The ALICE Experiment Introduction to relativistic heavy ion collisions

Design of the new ATLAS Inner Tracker for the High Luminosity LHC era

Visiting LHCb and LHC

arxiv: v1 [hep-ex] 2 Nov 2010

Recent Results from 7 GeV proton proton running at CMS

UNVEILING THE ULTIMATE LAWS OF NATURE: DARK MATTER, SUPERSYMMETRY, AND THE LHC. Gordon Kane, Michigan Center for Theoretical Physics Warsaw, June 2009

The Large Hadron Collider, and New Avenues in Elementary Particle Physics. Gerard t Hooft, Public Lecture, IPMU Tokyo, April 16, 2015

Particle Physics at the Energy Frontier. Kevin Stenson University of Colorado Boulder November 7, 2007

Brief Report from the Tevatron. 1 Introduction. Manfred Paulini Lawrence Berkeley National Laboratory Berkeley, California 94720

Mojtaba Mohammadi Najafabadi School of Particles and Accelerators, IPM Aban 22- IPM Workshop on Electroweak and Higgs at the LHC

HEAVY ION PHYSICS WITH CMS

Measurement of the Inclusive Isolated Prompt Photon Cross Section at CDF

The Importance of High-Precision Hadronic Calorimetry to Physics

Electron reconstruction and identification in CMS at LHC

Quarks and the Cosmos

The LHCb Flavour Physics Experiment

The ATLAS Detector at the LHC

ATLAS Experiment at Large Hadron Collider. Richard Stroynowski SMU

Muon commissioning and Exclusive B production at CMS with the first LHC data

Results from the Tevatron: Standard Model Measurements and Searches for the Higgs. Ashutosh Kotwal Duke University

Transcription:

The Compact Muon Solenoid (CMS) experiment at the Large Hadron Collider (LHC) Thursday, 12 February 2015

$ whoami S Lukasz (Luke) Kreczko Particle Physicist S Computing Research Assistant at the University of Bristol S My work involves: S Programming & project management (aka physics analysis) S SysAdmin, DevOps & user support S Outreach: among others, this talk

This talk includes S A (very) short introduction to particle physics S An overview of the LHC and the CMS experiment S Our data problem and our evolving solution

What is Particle Physics? In a nutshell Particle physics is the study of the smallest matter and anti-matter particles and the interactions between them.

How small is small? Observable Universe The Top? 10 30 m 10 20 m Galaxy clusters 10 10 m Solar system 1m You are here 10-10 m Atoms 10-20 m Standard Model 10-30 m Unknown? 10-40 m Planck length The Bottom?

Why are we doing this? S Our business is fundamental physics and we are trying to figure out how our universe works

Where does mass come from? S What is the origin of mass? S We are a step closer with the Higgs boson! S/(S+B) Weighted Events / 1.5 GeV 1500 1000 500 0 CMS -1 s = 7 TeV, L = 5.1 fb Data S+B Fit B Fit Component ±1σ ±2 σ Events / 1.5 GeV 1500 1000-1 s = 8 TeV, L = 5.3 fb Unweighted 120 130 (GeV) m γγ 110 120 130 140 150 (GeV) m γγ Discovered in 2012

Where does mass come from? S What is the origin of mass? S We are a step closer with the Higgs boson! S/(S+B) Weighted Events / 1.5 GeV 1500 1000 500 0 CMS -1 s = 7 TeV, L = 5.1 fb Data S+B Fit B Fit Component ±1σ ±2 σ Events / 1.5 GeV 1500 1000-1 s = 8 TeV, L = 5.3 fb Unweighted 120 130 (GeV) m γγ 110 120 130 140 150 (GeV) m γγ Francois Englert & Peter W. Higgs Nobel Prize in Physics 2013

What is Dark Matter? S What is 96 % of the universe made of? We only see 4%! What is Dark Matter and Dark Energy? dark energy, 73% dark matter, 23% stars, etc, 0.4% intergala ctic gas, 3.6%

Where has the anti-matter gone? S At the Big Bang, matter and anti-matter have been produced in equal quantities: why do we exist? S Matter and anti-matter should have annihilated each other shortly after S But there is lots of matter and almost no anti-matter in the universe!

S What is the state of matter just after the Big Bang?

What we know so far: The Standard Model S Describes elementary particles and the interactions between them S So far we know 6 quarks, 6 leptons and 4 force carriers + their anti-particles *Discovered in 2012!

The Standard Model S Normal matter consists of only the first generation proton neutron *Discovered in 2012!

The Standard Model S Muons: 1 per cm 2 per minute from cosmic rays at sea level *Discovered in 2012!

The Standard Model S Neutrinos: 7*10 10 particles per cm 2 per second from the sun S pass almost undisturbed through matter S Can oscillate into each other (discovered in 2001) Borexino experiment in Gran Sasso *Discovered in 2012!

The Standard Model S Photons (light) carriers of the electro-magnetic force: holding electrons within atoms together *Discovered in 2012!

The Standard Model S Photons (light) carriers of the electro-magnetic force: holding electrons within atoms together S Z- and W-bosons carriers of the weak force: radioactive betadecays *Discovered in 2012!

The Standard Model S Photons (light) carriers of the electro-magnetic force: holding electrons within atoms together S Z- and W-bosons carriers of the weak force: radioactive betadecays S Gluons: carriers of the strong force: holding the atomic nucleus together *Discovered in 2012!

The Standard Model S Newest observed member of the quarks (1995) S Highest mass (by a huge margin) comparable to a gold atom S Very short lifetime ~10-25 s: decays before it can interact with other matter! S My subject of study *Discovered in 2012!

The Standard Model S All of this is not stable and has to be produced in particle collisions! *Discovered in 2012!

The Large Hadron Collider Mankind s biggest machine (27 km circumference)

The Large Hadron Collider 4.3 km

The Large Hadron Collider the worlds most powerful microscope : allows the measurement of very small distances (~10-20 m)

The Large Hadron Collider the worlds fastest race track : protons go around the LHC ~10000 times per second

The Large Hadron Collider Cardiff Geneva: 150 times per second

The Large Hadron Collider a time machine : Recreates conditions as they were available nanoseconds after the Big Bang

The Large Hadron Collider collisions are 100,000 times hotter than the centre of the sun

The Large Hadron Collider And more dense than neutron stars!

The Large Hadron Collider Colder than deep space: (super) liquid helium at 1.9 K (-271 C) is used to cool LHC s superconducting magnets

A complex of accelerators

The CMS Experiment CMS DETECTOR Total weight Overall diameter Overall length Magnetic field : 14,000 tonnes : 15.0 m : 28.7 m : 3.8 T STEEL RETURN YOKE 12,500 tonnes SILICON TRACKERS Pixel (100x150 μm) ~16m2 ~66M channels Microstrips (80x180 μm) ~200m2 ~9.6M channels SUPERCONDUCTING SOLENOID Niobium titanium coil carrying ~18,000A Built like an onion around the collision point MUON CHAMBERS Barrel: 250 Drift Tube, 480 Resistive Plate Chambers Endcaps: 468 Cathode Strip, 432 Resistive Plate Chambers PRESHOWER Silicon strips ~16m2 ~137,000 channels FORWARD CALORIMETER Steel + Quartz fibres ~2,000 Channels CRYSTAL ELECTROMAGNETIC CALORIMETER (ECAL) ~76,000 scintillating PbWO4 crystals HADRON CALORIMETER (HCAL) Brass + Plastic scintillator ~7,000 channels

The CMS Experiment Charged particles leave a track in the tracker

The CMS Experiment Electrons and photons leave all of their energy in the electro-magnetic calorimeter

The CMS Experiment Protons and neutrons (and other hadrons) leave most of their energy in the hadron calorimeter

The CMS Experiment Muons travel through the whole detector and leave a track

The CMS Experiment Neutrinos can t be detected directly: through conservation of energy and momentum they are identified as missing energy

The CMS Experiment Like a big digital camera Ø > 76 million detector channels Ø 200 m 2 of silicon detector (tracker) Ø 40 million pictures (events) per second Ø ~ 1 MB of data per event Ø 3 microseconds data buffer

Decision to store/dump data comes from hardware trigger (custom FPGAs) The CMS Experiment

Decision to store/dump data comes from hardware trigger (custom FPGAs) The CMS Experiment

The CMS Experiment Decision to store/dump data comes from hardware trigger (custom FPGAs) Ø 100 000 events per second to computer farm (software trigger) Ø 1000 events per second to storage (tape/disk)

The CMS Experiment Decision to store/dump data comes from hardware trigger (custom FPGAs) Ø 100 000 events per second to computer farm (software trigger) Ø 1000 events per second to storage (tape/disk) From detector to disk: 40 MHz -> 100 khz -> 1kHz (while trying to keep interesting event)

CERN computing centre The data S The data is stored in data centres like these on both tape (backup) and disk (usage) S Multiple copies ensure availability and fault tolerance

The data S The data is segmented into data sets depending on trigger decision (electron trigger fired -> electron data set) S To understand the data we need simulation. Simulated data is segmented by physics process

Analysing a year of data S CMS records 10 000 Terabytes of data every year (around 70 years of full HD movies) 5000 x 2 TB

Analysing a year of data S CMS records 10 000 Terabytes of data every year (around 70 years of full HD movies) S + similar amount of simulation (usually more)

Analysing a year of data S CMS records 10 000 Terabytes of data every year (around 70 years of full HD movies) S + similar amount of simulation (usually more) S To analyse this on a single computer would take 64,000 years!

Analysing a year of data S CMS records 10 000 Terabytes of data every year (around 70 years of full HD movies) S + similar amount of simulation (usually more) S To analyse this on a single computer would take 64,000 years! S Solution: more computers

The beginning of the grid 1984: LHC project proposed

The beginning of the grid 1994: LHC project approved

The beginning of the grid Deciding LHC s computing model

The beginning of the grid The conclusion: analyse data where it is located Deciding LHC s computing model

The Grid CERN

The Grid Tape/disk + reconstruction CERN

The Grid Tape/disk + reconstruction CERN Tape/disk + reconstruction + simulation

The Grid Tape/disk + reconstruction CERN Tape/disk + reconstruction + simulation disk + simulation + user analysis

The Grid Tape/disk + reconstruction CERN Tape/disk + reconstruction + simulation disk + simulation + user analysys (disk) + user analysys

The Grid CERN All grid sites use Scientific Linux 5 and 6

Global distributed computing The Grid

Global distributed computing The Grid On a normal day, the grid provides 100,000 CPU days executing 1 million jobs

Global distributed computing The Grid At Bristol we have ~630 TB disk space 948 cores Connected via 10 Gbit/s to the grid

Data on the grid 140 PB > 200 PB of transfers

Data preparation

The CMS Software S The CMS Software (CMSSW) is open source: https://github.com/cms-sw/cmssw S Contains around 3.6M source lines of code (SLOC) S The entire software stack includes 125 external packages like ROOT (http://root.cern.ch) or Geant4 (http://geant4.cern.ch) S Runs on x86 and ARM devices under Linux and OS X S Available on all grid sites via CVMFS (http://cernvm.cern.ch/ portal/filesystem)

The data: a structured mess

The data: a structured mess This is low intensity! Later this year we expect 40 times this per collision!

The data: a much nicer picture Jet: p T = 84.1 GeV/c η = 2.24 Missing E T : 22.3 GeV Jet: p T = 89.0 GeV/c η = 2.14 Jet: p T = 85.3 GeV/c η = 2.02 Jet: p T = 90.5 GeV/c η = 1.40 Muon: p T = 71.5 GeV/c η = 0.82 Run: 163583 Event: 26579562 _ m(f)=1.2 TeV/c 2

The data: a much nicer picture Jet: p T = 84.1 GeV/c η = 2.24 Missing E T : 22.3 GeV Jet: p T = 89.0 GeV/c η = 2.14 Jet: p T = 85.3 GeV/c η = 2.02 Jet: a spray of particles going in a common direction Jet: p T = 90.5 GeV/c η = 1.40 Run: 163583 Event: 26579562 Muon: p T = 71.5 GeV/c η = 0.82 _ m(f)=1.2 TeV/c 2

The data: a much nicer picture Muon: the heavy partner of the electron Jet: p T = 84.1 GeV/c η = 2.24 Missing E T : 22.3 GeV Jet: p T = 89.0 GeV/c η = 2.14 Jet: p T = 85.3 GeV/c η = 2.02 Jet: p T = 90.5 GeV/c η = 1.40 Run: 163583 Event: 26579562 Muon: p T = 71.5 GeV/c η = 0.82 _ m(f)=1.2 TeV/c 2

The data: a much nicer picture Jet: p T = 84.1 GeV/c η = 2.24 Missing E T : 22.3 GeV Jet: p T = 89.0 GeV/c η = 2.14 Jet: p T = 85.3 GeV/c η = 2.02 Other low energy particles Run: 163583 Event: 26579562 Muon: p T = 71.5 GeV/c η = 0.82 Jet: p T = 90.5 GeV/c η = 1.40 _ m(f)=1.2 TeV/c 2

The data: a much nicer picture Jet: p T = 84.1 GeV/c η = 2.24 Missing E T : 22.3 GeV Jet: p T = 89.0 GeV/c η = 2.14 Jet: p T = 85.3 GeV/c η = 2.02 Energy and momentum imbalance Jet: p T = 90.5 GeV/c η = 1.40 Run: 163583 Event: 26579562 Muon: p T = 71.5 GeV/c η = 0.82 _ m(f)=1.2 TeV/c 2

The goal: extend our knowledge Jet: p T = 84.1 GeV/c η = 2.24 Jet: p T = 89.0 GeV/c η = 2.14 Run: 163583 Event: 26579562 Missing E T : 22.3 GeV Muon: p T = 71.5 GeV/c η = 0.82 Jet: p T = 85.3 GeV/c η = 2.02 Jet: p T = 90.5 GeV/c η = 1.40 _ m(f)=1.2 TeV/c 2 Billions of events + simulation S/(S+B) Weighted Events / 1.5 GeV 1500 1000 500 0 CMS -1 s = 7 TeV, L = 5.1 fb Data S+B Fit B Fit Component ±1σ ±2 σ Events / 1.5 GeV 1500 1000-1 s = 8 TeV, L = 5.3 fb Unweighted 120 130 (GeV) m γγ 110 120 130 140 150 m γγ (GeV)

The goal: extend our knowledge Jet: p T = 84.1 GeV/c η = 2.24 Jet: p T = 89.0 GeV/c η = 2.14 Run: 163583 Event: 26579562 Missing E T : 22.3 GeV Muon: p T = 71.5 GeV/c η = 0.82 Jet: p T = 85.3 GeV/c η = 2.02 Jet: p T = 90.5 GeV/c η = 1.40 _ m(f)=1.2 TeV/c 2 S/(S+B) Weighted Events / 1.5 GeV 1500 1000 500 0 CMS -1 s = 7 TeV, L = 5.1 fb Data S+B Fit B Fit Component ±1σ ±2 σ That s the famous Higgs boson Events / 1.5 GeV 1500 1000-1 s = 8 TeV, L = 5.3 fb Unweighted 120 130 (GeV) m γγ 110 120 130 140 150 m γγ (GeV)

The long shutdown S Since the end of 2012 the LHC has been in shutdown S Extensive maintenance was needed to get ready for 13 TeV operation (compared to 8 TeV in 2012)

The long shutdown S Since the end of 2012 the LHC has been in shutdown S Extensive maintenance was needed to get ready for 13 TeV operation (compared to 8 TeV in 2012) S Reprocessing of existing data: better detector knowledge etc. S 364 papers published on these data (as of Jan 2015)

The long shutdown S Since the end of 2012 the LHC has been in shutdown S Extensive maintenance was needed to get ready for 13 TeV operation (compared to 8 TeV in 2012) S Reprocessing of existing data: better detector knowledge etc. S 364 papers published on these data (as of Jan 2015) S Lots of time to think about what we can do better

Using the WAN Deciding LHC s computing model

Using the WAN quotation needed S WANs today are fast and reliable S Most sites connected with > 10 Gbit/s S A few sites have lots of cores but little storage

Using the WAN quotation needed S WANs today are fast and reliable S Most sites connected with > 10 Gbit/s S A few sites have lots of cores but little storage S The conclusion: bring data to where cpu cycles are available S Done via Xrootd (http://xrootd.org/)

The logical next step S Dynamic Data Placement: S Monitor the data sample popularity S Delete unused samples (leave 1 copy on tape) S Copy popular samples to more sites

The logical next step S Dynamic Data Placement: S Monitor the data sample popularity S Delete unused samples (leave 1 copy on tape) S Copy popular samples to more sites S Self-regulated system deployed last year S Frees data manager resources S Fast reaction to bottlenecks or space filling up

Other preparations S Software - big effort on multicore to improve data reconstruction S Together with algorithm improvements back on track

Other preparations S Software - big effort on multicore to improve data reconstruction S Middleware - more use of temporary resources e.g. clouds S Using openstack to build up a site on demand S Looking at docker (https://github.com/cmssw/cms-sw.github.io/blob/master/docker.md)

Other preparations S Software - big effort on multicore to improve data reconstruction S Middleware - more use of temporary resources e.g. clouds S The grid is busy: S First sets of simulation for this year are finished. S The final set (to be used with data) is starting soon

Summary S The LHC and the CMS experiment are large man-made machines to measure the smallest known (anti-)matter

Summary S The LHC and the CMS experiment are large man-made machines to measure the smallest known (anti-)matter S The data storage and analysis challenge has been met with the LHC worldwide grid S Made past discoveries possible but is still evolving S Data is shipped on demand to available computing resources S Data popularity is used to distribute data across sites

Summary S The LHC and the CMS experiment are large man-made machines to measure the smallest known (anti-)matter S The data storage and analysis challenge has been met with the LHC worldwide grid S Made past discoveries possible but is still evolving S Data is shipped on demand to available computing resources S Data popularity is used to distribute data across sites S The LHC is about to start collisions again in May/June S We are ready for the new energy frontier!

Any Questions?