icrea - results from the lhc run ii. mario martinez

75
Results from the LHC Run II Mario Mar5nez 68th ICREA Colloquium, Barcelona, November 2015

Upload: icrea

Post on 21-Jan-2017

399 views

Category:

Science


0 download

TRANSCRIPT

Page 1: ICREA - Results from the LHC Run II. Mario Martinez

Results  from  the  LHC  Run  II      

Mario  Mar5nez  

68th  ICREA  Colloquium,    Barcelona,    November  2015  

Page 2: ICREA - Results from the LHC Run II. Mario Martinez

Outline  •  The  SM  in  30´´  

•  Few  basic  ideas  on  modern  HEP  

•  CERN,    LHC,  ATLAS  

•  The  success  of    Run  I  Physics    

•  First  Run  II  Results  from  ATLAS  

•  Notes  on  Prospects  

Disclaimer:  

Many  many  results  exist  that  I  will  not  show…  

LHC  (running…)            

Page 3: ICREA - Results from the LHC Run II. Mario Martinez
Page 4: ICREA - Results from the LHC Run II. Mario Martinez

The Standard Model (SM)

H  

Page 5: ICREA - Results from the LHC Run II. Mario Martinez

InteracCons  mediated  by  bosons  

10/11/15   5  

1  

10-­‐40   10-­‐5  

10-­‐2  

Page 6: ICREA - Results from the LHC Run II. Mario Martinez

10/11/15   6  

                                                   UnificaCon  of  forces  Higgs  mechanism  makes  the  small  range  and      weak  interacCon    (massive  Ws  and  Z  )  

Same  Cme  allows  for  fermion  masses  

σ ∝1Q4

σ ∝1

(Q2 + MW2 )2

We  are  here  

H  

Page 7: ICREA - Results from the LHC Run II. Mario Martinez

A    world  without  mass  ?  

a0 = 1αem me

(natural units)

GF ∝ 1MW

2

Without  giving  masses  to  fermions  it  would  be  impossible  to  form  stables  atoms  

Light  W  ?      Faster  reacCons  and  a  Cold  Universe  

Page 8: ICREA - Results from the LHC Run II. Mario Martinez

The  Sun  using  Neutrinos  

106    cm-­‐2  s-­‐1  

10/11/15   8  

Page 9: ICREA - Results from the LHC Run II. Mario Martinez

The Standard Model (SM)

H   The Higgs mechanism allows to explain the origin of the mass of the particles in the SM and at the same time explains weakness of the weak interaction…

mγ = 0 mg = 0mW = 80GeVmZ = 91GeVmH =125 GeV

Page 10: ICREA - Results from the LHC Run II. Mario Martinez

Higgs  Mechanism  

Page 11: ICREA - Results from the LHC Run II. Mario Martinez

Fermion  Masses  Most  of  the  free  parameters  in  the  SM  model  come  from  here  

Page 12: ICREA - Results from the LHC Run II. Mario Martinez

Why  such  a  mass  hierarchy  ?  

10/11/15   12  

Page 13: ICREA - Results from the LHC Run II. Mario Martinez

Mass  F  =  M  a  

E  =  M  c2  Mass  as  a    form  of  energy  

Protón  

(uud)  

Only  2%  of  the  proton  mass  is  due  to  quarks…most  of  it  is    QCD  confinement  energy  

I.  Newton  

A.  Einstein  

Page 14: ICREA - Results from the LHC Run II. Mario Martinez

Accelerators      ..as  huge  microscopes

10−19mThe  proton-­‐proton  collisions    probe  distances  down  to    

?

ParPcles  behave  as  waves…  E  =  hν                                  h    Planck  const.                                            λ=  h  /|p|    

Page 15: ICREA - Results from the LHC Run II. Mario Martinez

Quantum  Field  Theory  •  AnCma^er  

–  ParPcle-­‐  (anP)  parPcle  annihilaPon  produces  pure  energy  

–  Energy  can  then  transform  into  new  kind  of  maYer  

•  Virtual  ParCcles  

–  InteracPons  are  understood  and  the  “exchange”  of  virtual  parPcles      

•  Probability  –  For  each  reacPon  different  final  

states  are  possible  according  to    a  given  probability  to  be  produced  

E  =  m  c2  

e+  e-­‐  

E 2 − p2 ≠ m2

ΔEΔt ≥ h

Page 16: ICREA - Results from the LHC Run II. Mario Martinez

                       27  Km  1232  high-­‐tech  superconducCng  dipole  magnets  

   (at  1.8  K…the  coldest  (and  coolest)  place  in  the  universe)  

proton  –  proton    7-­‐8  TeV  in  Run  I    (2010  –  2012)  (13  TeV  in  Run  II)        (2015    -­‐-­‐    )    

Approved  in  1994    

(at  99.999999%  of  the  speed  of  light)     bunches  of  1011  protons  collide  every  25  ns     109  interacCons  per  second/experiment  

                 also  Pb-­‐Pb  collisions  (1  month/year)  

Page 17: ICREA - Results from the LHC Run II. Mario Martinez

LHC  construcCon  

Page 18: ICREA - Results from the LHC Run II. Mario Martinez

LHC  ConstrucCon  

Page 19: ICREA - Results from the LHC Run II. Mario Martinez

ATLAS  LHC  will  run  for  15  years..  A  total  of    6    1015  collisions  

Page 20: ICREA - Results from the LHC Run II. Mario Martinez
Page 21: ICREA - Results from the LHC Run II. Mario Martinez

ATLAS  

Page 22: ICREA - Results from the LHC Run II. Mario Martinez

Hadron Calorimeter (1993 )

 Big  contribuCon  to  TileCal  in  ATLAS  

 R&D  for  design  of  prototype   ConstrucCon  of  1/3  TielCal  (Barrel-­‐C)  

 Understanding  of  test-­‐beam  data   Design/construcPon/maintenance  of        calibraPon  electronics  (Cs137  &  MB)     Study  of  TileCal  Performance   TileCal  DQ  Monitoring   ContribuPon  to  Run  CoordinaPon  

ADCs  and  RB  models  designed  and  built  at  IFAE      

Page 23: ICREA - Results from the LHC Run II. Mario Martinez

IBL  ConstrucCon  Final  stave  assembly  done  at  CERN:  

IBL  Stave  assembly  

CNM  3D  sensors  

Barcelona  made  a  key    contribuCon  to  the    Pixel:    the  most  complex  detector    of  ATLAS  (and  using  3D)  

Final  IBL  stave  being  mounted    26  March  2014  

Page 24: ICREA - Results from the LHC Run II. Mario Martinez

The  ATLAS    Experiment  selects  ONLINE  the  most  interesCng  events  out  of  the  109  interacCons/second  

ATLAS  output  rate  of  400  Hz    (1.5  Mb/event)  

Page 25: ICREA - Results from the LHC Run II. Mario Martinez
Page 26: ICREA - Results from the LHC Run II. Mario Martinez

Physics  Menu  

The  collision  results  are  typically  driven  by  uninteresCng  events     InteresCng  events  have  small  probabiliCes  to  occur       Need  for  accumulaCng  a  huge  number  of  collisions  

N  events  =    σ  x    Luminosity  

1b =10−28m

Page 27: ICREA - Results from the LHC Run II. Mario Martinez

LHC  Performance  (2010-­‐2012)  Spectacular  LHC  performance  (rapid  increase  of  data  samples)  

..als…    rapid  increase  of  pile-­‐up  condiCons  

LHC  ended  pp  run  at  7+8  TeV  aler  delivering  more  than      28  m-­‐1  

…back    in  2015    with  13  TeV  collisions    

Page 28: ICREA - Results from the LHC Run II. Mario Martinez

MulCple  InteracCons  

Mean Number of Interactions per Crossing0 5 10 15 20 25 30 35 40 45

/0.1

]-1

Rec

orde

d Lu

min

osity

[pb

020406080

100120140160180

Online LuminosityATLAS> = 20.7!, <-1Ldt = 20.8 fb = 8 TeV, s

> = 9.1!, <-1Ldt = 5.2 fb = 7 TeV, s

Up  to  40  interacCons  /  crossing  

(requires  enormous  efforts  to    understand    the  reconstrucCon  of  the  physics  objects…)  

Z    µµ  events  with    20  interacCons  on  top  

Page 29: ICREA - Results from the LHC Run II. Mario Martinez

Summary  QCD/EWK/Top  Physics    

29  

Page 30: ICREA - Results from the LHC Run II. Mario Martinez

Resonances..  

E  =  M  c2  

e+  e-­‐  

10/11/15   30  

You  just  learnt  we  can  transform  energy  in  new  parCcles…  but  what  about  if  they  decay  immediately  ?  

If  the  energy  in  the  collision  comes  close  to  the    mass  of  the  (unknown)  mediated  parCcle    a  resonance  (a  peak  of  events)  is  observed…    

And  this  is  the  way    to  discover  new  parCcles  

Page 31: ICREA - Results from the LHC Run II. Mario Martinez

Want    a  Nobel?...find  a  resonance  

10/11/15   31  

Page 32: ICREA - Results from the LHC Run II. Mario Martinez

Building  up  the  peaks..  

Page 33: ICREA - Results from the LHC Run II. Mario Martinez

Higgs  !!   As    in    Moriond  2013  E

vent

s / 2

GeV

2000

4000

6000

8000

10000

H

-1Ldt = 4.8 fb = 7 TeV s-1Ldt = 20.7 fb = 8 TeV s

ATLAS

Data 2011+2012=126.8 GeV (fit)

HSM Higgs boson mBkg (4th order polynomial)

[GeV]m100 110 120 130 140 150 160E

vent

s - F

itted

bkg

-200-100

0100200300400500

!"#$%&!!'(() (*) (+) (,) (-)./

".01&!2

$3456$7!89$:6;!/!(<-!#$%

)

()))

*)))

+)))

,)))

-))) =>6>.01!?361@4!?36!AB'CB:$:6

"(±"*±

!"D%E&F(!G!H!I$%J!K!G!(L<M!NO;!"D%E&F(!G!P!I$%J!K!G!-<(!NO;

AD.!QR$S3'3:>RT

A  mass  peak  in  the  vicinity  of  125  GeV    

Page 34: ICREA - Results from the LHC Run II. Mario Martinez

Higgs  !!    

[GeV]4lm100 150 200 250

Even

ts/5

GeV

0

5

10

15

20

25

30

35

40

-1Ldt = 4.6 fb = 7 TeV s-1Ldt = 20.7 fb = 8 TeV s

4lZZ*HData 2011+ 2012SM Higgs Boson

=124.3 GeV (fit)H mBackground Z, ZZ*

tBackground Z+jets, tSyst.Unc.

ATLAS

[GeV]4lm80 100 120 140 160 180

Even

ts /

3 G

eV

0

5

10

15

20

25

30

35Data

Z+X

,ZZ*Z

=126 GeVHm

CMS Preliminary -1 = 8 TeV, L = 19.6 fbs ; -1 = 7 TeV, L = 5.1 fbs

A  mass  peak  in  the  vicinity  of  125  GeV    

Page 35: ICREA - Results from the LHC Run II. Mario Martinez

H    ZZ*    4l

Page 36: ICREA - Results from the LHC Run II. Mario Martinez

8th  Oct.  2013  

Page 37: ICREA - Results from the LHC Run II. Mario Martinez

Higgs  at  the  PDG  

Page 38: ICREA - Results from the LHC Run II. Mario Martinez

Latest    Higgs  Results  If  it  looks  like  a  duck,  swims  like  a  duck,  and  quacks  like  a  duck…  

arXiv:1507.04548  (July  2015)  

38  

Page 39: ICREA - Results from the LHC Run II. Mario Martinez

The Standard Model (i.e., the need for new physics)

H  

•  Who ordered 3 generations? •  Origin of different masses ? •  Matter/Anti-Matter ?

•  What about Gravity? •  very very weak and only relevant at planetary/cosmological levels

QED/GRAVITY strength ~ 1036

•  Hierarchy Problem … •  Unification at Large Scale? •  Dark Matter in the Cosmos? • ………

New Physics (!) O(TeV) scale phenomenology

Page 40: ICREA - Results from the LHC Run II. Mario Martinez

The  rotaCon  of  the  stars  around  the    center  of  the  galaxies  is  not  consistent    with  the  amount  of  mass  observed    (L/M  raCo)SUN  

Collisions  of  clusters  of  galaxies  

Large  distorCon    of  the  imagines  of  distant    galaxies  due  to  gravitaCon  lensing        indicaCon  of  DM  in  galaxy  clusters  

GravitaConal  Lensing  

Considered  the  ulCmate  demonstraCon  of  the  presence  of  Dark  Ma^er  since  this  does  not  involve    Newton’s  Law  

Evidence  for  Dark  Ma^er  

Spherical  dark  ma^er  halo  

Page 41: ICREA - Results from the LHC Run II. Mario Martinez

10/11/15   41  

Planck  (20  March  2013)  arXiv:1303.5062v1  

CMB  radiaCon  

380.000  years  

13.82  billion  years  

Page 42: ICREA - Results from the LHC Run II. Mario Martinez

Super-­‐symmetry  (SUSY)  In  the    SM  the  parPcles  are    classified  as  fermions    of  bosons    according  to  the  spin  of  the  parPcle   SUSY    predicts  that  for    

each  parPcle  in  the  SM  there  is    a  super-­‐partner  with  different    spin    configuraPon    

Examples  :    

 electron  (fermion)      s-­‐electron  (boson)    quark            (fermion)      s-­‐quark  (boson)    gluon            (boson)            gluino  (fermion)  

So,  SUSY  DOUBLES  the  spectrum  of  parPcles  

   SUSY  parCcles  are  heavy  and  (if  exist)    could  be    produced  at  colliders    

Page 43: ICREA - Results from the LHC Run II. Mario Martinez

Strong

Weak

Electromagnetic

Unification of Forces & SUSY

Page 44: ICREA - Results from the LHC Run II. Mario Martinez

1.  Squarks and Gluinos are heavy

2.  mixing of third generation leads to light stop and sbottom

3.  good candidate for Dark Matter

4.  One higgs is very light ( < 135 GeV)

SUSY before LHC era (2010)

Page 45: ICREA - Results from the LHC Run II. Mario Martinez

Dark  Ma^er  search  with  Mono-­‐jets  

45  

Pillar  of  LHC  Physics  Program  for  Run  II  

gluon  

EPJC  75  (2015)  299  

Page 46: ICREA - Results from the LHC Run II. Mario Martinez

Inclusive  Searches  MulCple-­‐jets  and  large  ETmiss    

meff = ETmiss +HT

HT = pTjets∑

SIMPLIFIED  SCENARIO  

JHEP09(2014)176  

2  jets  

6  jets  

2  jets  

MSUGRA  

Background  from    1  lepton  b-­‐tag/veto  &    photon  CRs  with  similar  jet  and  kinemaCc  selecCons  as  in  SRs  

46  

Page 47: ICREA - Results from the LHC Run II. Mario Martinez

“Natural  SUSY  2012”  

 Light higgsinos

 Light stop (t1 < 1 TeV)

 Light gluinos (< 1-2 TeV)

One  light  stop  and  sbo^on  ….rest  of  sparCcles  can  be  decoupled….  

(same  weak  isospin  mulPplet)  47  

Page 48: ICREA - Results from the LHC Run II. Mario Martinez

Summary  Searches  for  Stop  (different  mass  hierarchies,  simplified  models)  

Exclusion  for  m(~t1)  <  ~720  GeV  for  massless  LSP  Exclusion  up  to  m(LSP)  ~280  GeV  

 arXiv:1506.08616  

48  

Page 49: ICREA - Results from the LHC Run II. Mario Martinez

10/11/15   49  

Page 50: ICREA - Results from the LHC Run II. Mario Martinez

No  hint  for  SUSY  ?    

50  

Page 51: ICREA - Results from the LHC Run II. Mario Martinez

Non-­‐SUSY  Searches  

Extra  dimensions,    q*,  new  bosons,  vector-­‐like  quarks,  lepto-­‐quarks,..  

Page 52: ICREA - Results from the LHC Run II. Mario Martinez

Large  Extra  Dimensions  

52  

g,q  

g,q Jet,γ

G  Extra  spaCal  dimensions    explain  the  apparent    weakness  of  Gravity  (relevant  scale  ~TeV)  

Page 53: ICREA - Results from the LHC Run II. Mario Martinez

No  hint  for  BSM  ?    

53  

Page 54: ICREA - Results from the LHC Run II. Mario Martinez

Great  Success  of  the  SM…  But  lots  of  remaining  quesCons..  

naturalness  dark  maKer  maKer/anMmaKer  asymmetry  the  flavor/family  problems    unificaMon  of  coupling  constants    …….    

54  

Page 55: ICREA - Results from the LHC Run II. Mario Martinez

Things  to  keep  an  eye  on  

Eur.  Phys.  J.  C75  (2015)  318  

   arXiv:1504.04605  

high-­‐mass  diboson  resonances    with  boson-­‐tagged  jets  

2  SS  leptons  +  HT  +b-­‐jets  +  MET  

Z  +  jets+  MET  

Few    sigma  effects    calling  for  more  data….  

 arXiv:1506.00962  

55  

Page 56: ICREA - Results from the LHC Run II. Mario Martinez

56  

?  

The  discovery  of  New  Physics  requires    more  energy  and  more  data  ………  

Page 57: ICREA - Results from the LHC Run II. Mario Martinez

Run  II  has  started……  

57  

Page 58: ICREA - Results from the LHC Run II. Mario Martinez

The  physics  gain  8  TeV    13  TeV  

NO  surprising..    this  is  just  PDFs  

But    tells  you  nicely  what  we  already  know  

•     Huge  improvement  at  the  edge  of  phase  space  •     Searches  should  be  priority  1  in  first  6-­‐12  months  

Consider  this  an    opCmisCc  view  as    it  does  not  include  realiCes  as    

Background  composiCon  Pileup  Data  ValidaCon  MC  simulaCon  ……..  

58  

Page 59: ICREA - Results from the LHC Run II. Mario Martinez

The  physics  gain  8  TeV    13  TeV  

NO  surprising..    this  is  just  PDFs  

But    tells  you  nicely  what  we  already  know  

•     Huge  improvement  at  the  edge  of  phase  space  •     Searches  should  be  priority  1  in  first  6-­‐12  months  

Consider  this  an    opCmisCc  view  as    it  does  not  include  realiCes  as    

Background  composiCon  Pileup  Data  ValidaCon  MC  simulaCon  ……..  

Q*  and  QBH        factors  56  –  370  Gluino  producCon    factor  46  Stop/Sbo^om  producCon  factor  8  ^H    factor  3.9  H(ggF)    factor  2.3  

59  

Page 60: ICREA - Results from the LHC Run II. Mario Martinez

Early  13  TeV  Results  ATLAS-­‐CONF-­‐2015-­‐04  

Going  beyond  Run  I  sensiCvity  

80  pb-­‐1  

60  

Page 61: ICREA - Results from the LHC Run II. Mario Martinez

SUSY/ExoCcs  (Some  PR  plots  @  13TeV)  

Inclusive  SUSY  

Monojet  

Di-­‐photons   Z-­‐prime  

W-­‐prime  

61  

Page 62: ICREA - Results from the LHC Run II. Mario Martinez

SUSY  prospects  (2015-­‐6)   ATL-­‐PHYS-­‐PUB-­‐2015-­‐005  

Assuming  20%  uncertainty  on  backg.    As  inspired  by  8  TeV  analyses  

A  hint  for  SUSY  signal  sCll  possible  if    the  SUSY  parCcles  are  around  the  corner      

62  

Page 63: ICREA - Results from the LHC Run II. Mario Martinez

LHC  Plan    Producción    174M  Higgs  

63  

Page 64: ICREA - Results from the LHC Run II. Mario Martinez

Final  Notes  

64  

El  LHC  almost  doubles    the  centre-­‐of-­‐mass  energy  in  2015                8  TeV    13  TeV  

(about  4    m-­‐1  in  2015…we  need  more)  

Cross  secCon  for  stop  (0.9  TeV  mass)  pair    producCon    @  13  TeV  =    12  x    @  8  TeV      

Ready  for  a  new  discovery  ?  

More  energy  and  more  data  !  

Page 65: ICREA - Results from the LHC Run II. Mario Martinez
Page 66: ICREA - Results from the LHC Run II. Mario Martinez

Hierarchy Problem From EWK to Planck scale ?

H f

Already a serious problem at 5 TeV scale (cancellation among top, gauge and Higgs loops)

This kind of conspiracy has name in Physics…

New Symmetry ? (taken from C. Quigg, hep-ph/0704.2232)

EWK  scale:    102  GeV  

Gravity  scale:    1019  GeV  

..nothing  in  the  middle  ???  …  

Page 67: ICREA - Results from the LHC Run II. Mario Martinez

SuperSymmetry  vs  Higgs  

• Fermion/Boson  symmetry  

• Exact  cancellaCon  between    fermion  &  boson  loops  for  Higgs      

..SUSY  must  be  broken…..  model-­‐dependent  phenomenology  

Double  Spectra  of  ParCcles  

..will  mix  to  form  mass  eigenstates..  

Higgs  sector  with  2  doublets  

G   G  ~  

67  

Page 68: ICREA - Results from the LHC Run II. Mario Martinez

QBH  (producCon  of  Black  Holes  in  models  with  extra  spaCal  dimensions)  

JHEP08(2014)103  JHEP  07  (2015)  032  

Lepton  +  Jets   MulCJets  

Spectacular  Events..  Large  MulCpliciCes  of    Jets  and  Leptons….  No  surprises  yet  68  

Page 69: ICREA - Results from the LHC Run II. Mario Martinez

Dileptons  g,q  

g,q

f,V  

f,V  

G  

Limits  on  RS  (ED)  Graviton    mass  vs  coupling     95%  CL  exclusion  in  the  mass  range            MG  =  1.2  TeV  –  2.7  TeV  

Phys.  Rev.  D.  90,  052005  (2014)  

Limits  on  SSM  and    E6    GUT  inspired  models   MZ’      (SSM)  <  2.86  TeV  excluded   MZ’    (E6)    <  2.4  TeV    –  2.6  TeV  excluded    

69  

Page 70: ICREA - Results from the LHC Run II. Mario Martinez

Dijets  Phys.  Rev.  D.  91,  052007  (2015)  

p-­‐value    =  0.027  

Mjj  =  5  TeV  

Excited  quarks  with  mass  <  4  TeV    excluded  at  95%  CL  

Bump  hunCng…  

Dijet  mass  spectrum  fi^ed  to  the  funcConal  form  

70  

Page 71: ICREA - Results from the LHC Run II. Mario Martinez

HL-­‐LHC  prospects  ATL-­‐PHYS-­‐PUB-­‐2013-­‐011  ATL-­‐PHYS-­‐PUB-­‐2014-­‐010  

Will  be  in  the  posiCon    to  “kill  natural  SUSY”  

SensiCvity  up  to  3  –  3.5  TeV    

71  

Page 72: ICREA - Results from the LHC Run II. Mario Martinez

HL-­‐LHC  prospects  ATL-­‐PHYS-­‐PUB-­‐2013-­‐011  ATL-­‐PHYS-­‐PUB-­‐2014-­‐010  

Will  be  in  the  posiCon    to  “kill  natural  SUSY”  

SensiCvity  up  to  1  –  1.5  TeV    

72  

Page 73: ICREA - Results from the LHC Run II. Mario Martinez

HL-­‐LHC  prospects  ATL-­‐PHYS-­‐PUB-­‐2015-­‐032  

SUSY  Weakly  interacCng  

SensiCvity  up  to    1.1  TeV    

73  

Page 74: ICREA - Results from the LHC Run II. Mario Martinez

Q*  and  QBHs  ATL-­‐PHYS-­‐PUB-­‐2015-­‐004  

6  TeV  Q*  10  TeV  QBH  

Large  increase  in  sensiCvity  (it  happens  early  on)  

74  

Page 75: ICREA - Results from the LHC Run II. Mario Martinez

HL-­‐LHC  prospects  Higgs  couplings  (assuming  SM  ΓH)  •   2-­‐5%  in  most  cases  •   10%  for  rare  processes  (H  μμ,  ^H    ^γγ)    

•   may  see  Higgs  self  couplings  ?    (1.3  sigma  significance)    

ATL-­‐PHYS-­‐PUB-­‐2014-­‐019  ATL-­‐PHYS-­‐PUB-­‐2014-­‐016  

75