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Prospects (perspec+ves) from Tevatron Higgs Ben Kilminster (Fermilab) Higgs Hun+ng workshop July 29, 2011 1 B.Kilminster, Higgs Hun+ng

Prospects)(perspec+ves))from) Tevatron)Higgs) fileTEV,)CMS,)ATLAS) Higgs boson mass (GeV/c2) 120 140 160 180 200 220 SM! / 95%! Limit on 1 10 Observed S CL Expected ± 1! S CL Expected

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Page 1: Prospects)(perspec+ves))from) Tevatron)Higgs) fileTEV,)CMS,)ATLAS) Higgs boson mass (GeV/c2) 120 140 160 180 200 220 SM! / 95%! Limit on 1 10 Observed S CL Expected ± 1! S CL Expected

Prospects  (perspec+ves)  from  Tevatron  Higgs  

Ben  Kilminster  (Fermilab)  Higgs  Hun+ng  workshop  

July  29,  2011  

1  B.Kilminster,  Higgs  Hun+ng  

Page 2: Prospects)(perspec+ves))from) Tevatron)Higgs) fileTEV,)CMS,)ATLAS) Higgs boson mass (GeV/c2) 120 140 160 180 200 220 SM! / 95%! Limit on 1 10 Observed S CL Expected ± 1! S CL Expected

•  Prospects  – What  are  the  most  interes+ng  results  we  can  expect  from  Tevatron  with  full  dataset  of  10  J-­‐1  ?  

•  Perspec+ves  – What  can  Tevatron  teach  us  given  the  recent  CMS  &  ATLAS  results  ?  

2  B.Kilminster,  Higgs  Hun+ng  

Page 3: Prospects)(perspec+ves))from) Tevatron)Higgs) fileTEV,)CMS,)ATLAS) Higgs boson mass (GeV/c2) 120 140 160 180 200 220 SM! / 95%! Limit on 1 10 Observed S CL Expected ± 1! S CL Expected

•  Exclusion  156  GeV  –  177  GeV  •  Below  115  GeV  

–  Expected  =  observed  –  Almost  at  SM  95%  CL  exclusion  

•  Expected  sensi+vity  less  than  1.35*SM  across  interes+ng  range  (114  –  155  GeV)  –  Worst  expected  sensi+vity  at  130  GeV  

3  B.Kilminster,  Higgs  Hun+ng  

Page 4: Prospects)(perspec+ves))from) Tevatron)Higgs) fileTEV,)CMS,)ATLAS) Higgs boson mass (GeV/c2) 120 140 160 180 200 220 SM! / 95%! Limit on 1 10 Observed S CL Expected ± 1! S CL Expected

Most  signal-­‐like  value  

•  Most  signal-­‐like  excess  –  Consistent  with  130  GeV  Higgs  

4  B.Kilminster,  Higgs  Hun+ng  

Page 5: Prospects)(perspec+ves))from) Tevatron)Higgs) fileTEV,)CMS,)ATLAS) Higgs boson mass (GeV/c2) 120 140 160 180 200 220 SM! / 95%! Limit on 1 10 Observed S CL Expected ± 1! S CL Expected

TEV,  CMS,  ATLAS  

)2Higgs boson mass (GeV/c120 140 160 180 200 220

SM!/

95%

!Li

mit

on

1

10

ObservedSCL! 1± Expected SCL! 2± Expected SCL

Bayesian Observed

ObservedSCL! 1± Expected SCL! 2± Expected SCL

Bayesian Observed

-1 = 1.1 fbintCombined, L = 7 TeVsCMS Preliminary,

[GeV]Hm110 120 130 140 150 160 170 180 190 200

SM/

95%

CL

Lim

it on

1

10

Observed CLsExpected 1 ! 2 !

ATLAS Preliminary

-1 Ldt = 1.0-1.2 fb

= 7 TeVs

5  B.Kilminster,  Higgs  Hun+ng  

Page 6: Prospects)(perspec+ves))from) Tevatron)Higgs) fileTEV,)CMS,)ATLAS) Higgs boson mass (GeV/c2) 120 140 160 180 200 220 SM! / 95%! Limit on 1 10 Observed S CL Expected ± 1! S CL Expected

TEV,  CMS,  ATLAS  

)2Higgs boson mass (GeV/c120 140 160 180 200 220

SM!/

95%

!Li

mit

on

1

10

ObservedSCL! 1± Expected SCL! 2± Expected SCL

Bayesian Observed

ObservedSCL! 1± Expected SCL! 2± Expected SCL

Bayesian Observed

-1 = 1.1 fbintCombined, L = 7 TeVsCMS Preliminary,

[GeV]Hm110 120 130 140 150 160 170 180 190 200

SM/

95%

CL

Lim

it on

1

10

Observed CLsExpected 1 ! 2 !

ATLAS Preliminary

-1 Ldt = 1.0-1.2 fb

= 7 TeVs

6  B.Kilminster,  Higgs  Hun+ng  

Consistencies  TeV,  CMS,  ATLAS  •   Sensi+vi+es  to  <  ~2*SM  for  125  to  200  GeV  •   Exclusion  above  155  GeV  •   Excesses  overlap  130  to  155  GeV  •   CMS  injected  signal  studies  indicate  130-­‐140  GeV  can  produce  such  an  excess  as  seen  in  CMS  &  ATLAS  •   Tev  most  signal-­‐like  point  is  130  GeV  

•   Sensi+vity  at  130  GeV  •   CMS  :    0.8*SM  •   Tevatron  :  1.35*SM    

•   ATLAS  :  1.4*SM  

Page 7: Prospects)(perspec+ves))from) Tevatron)Higgs) fileTEV,)CMS,)ATLAS) Higgs boson mass (GeV/c2) 120 140 160 180 200 220 SM! / 95%! Limit on 1 10 Observed S CL Expected ± 1! S CL Expected

TEV,  CMS,  ATLAS  

)2Higgs boson mass (GeV/c120 140 160 180 200 220

SM!/

95%

!Li

mit

on

1

10

ObservedSCL! 1± Expected SCL! 2± Expected SCL

Bayesian Observed

ObservedSCL! 1± Expected SCL! 2± Expected SCL

Bayesian Observed

-1 = 1.1 fbintCombined, L = 7 TeVsCMS Preliminary,

[GeV]Hm110 120 130 140 150 160 170 180 190 200

SM/

95%

CL

Lim

it on

1

10

Observed CLsExpected 1 ! 2 !

ATLAS Preliminary

-1 Ldt = 1.0-1.2 fb

= 7 TeVs

Differences  TeV,  CMS,  ATLAS  •   Tevatron  sensi+vity  improves  for  less  than  130  GeV  as  you  go  down  in  mass  •   Opposite  at  CMS,  ATLAS  

•   LHC  is  >  2  Sigma  high  ~160  GeV  •   No  excess  at  Tevatron  

•   CMS  &  ATLAS  fluctuate  high  mH  <  120  GeV  •   Tevatron  is  inconsistent  

7  B.Kilminster,  Higgs  Hun+ng  

Page 8: Prospects)(perspec+ves))from) Tevatron)Higgs) fileTEV,)CMS,)ATLAS) Higgs boson mass (GeV/c2) 120 140 160 180 200 220 SM! / 95%! Limit on 1 10 Observed S CL Expected ± 1! S CL Expected

•  Interes+ng  regions  for  Tevatron  to  study  

Low  mass  :  ~  115  GeV  Tevatron  H➞bb  searches  

Mid  mass  :  ~  130  GeV  Most  consistent  excesses    Between  Tev,  CMS,  ATLAS  

8  B.Kilminster,  Higgs  Hun+ng  

Page 9: Prospects)(perspec+ves))from) Tevatron)Higgs) fileTEV,)CMS,)ATLAS) Higgs boson mass (GeV/c2) 120 140 160 180 200 220 SM! / 95%! Limit on 1 10 Observed S CL Expected ± 1! S CL Expected

Tevatron  perspec+ves  

•  115  GeV  –  Tevatron  currently  provides  best  sensi+vity  

•  Mainly  from  H➞bb  searches  •  Can  address  behaviors  seen  in  CMS,  ATLAS  data  from  H➞WW  and  H➞γγ  

•  130  GeV  –  Tevatron  sensi+vity  mainly  from  H➞WW  –  Currently  compe++ve  with  LHC  –  Even  when  LHC  has  more  data  …  

•  Tevatron  H➞WW  has  different  background  composi+on  •  Tevatron  H➞WW  has  different  signal  composi+on  

B.Kilminster,  Higgs  Hun+ng   9  

Page 10: Prospects)(perspec+ves))from) Tevatron)Higgs) fileTEV,)CMS,)ATLAS) Higgs boson mass (GeV/c2) 120 140 160 180 200 220 SM! / 95%! Limit on 1 10 Observed S CL Expected ± 1! S CL Expected

Tevatron  perspec+ve  at  130  GeV  

B.Kilminster,  Higgs  Hun+ng   10  

Page 11: Prospects)(perspec+ves))from) Tevatron)Higgs) fileTEV,)CMS,)ATLAS) Higgs boson mass (GeV/c2) 120 140 160 180 200 220 SM! / 95%! Limit on 1 10 Observed S CL Expected ± 1! S CL Expected

WW  excesses  at  CMS  &  ATLAS  

CDF  ,  D0  plots  

11  B.Kilminster,  Higgs  Hun+ng  

ATLAS  0-­‐jet   ATLAS  1-­‐jet  

CMS  0-­‐jet   CMS  1-­‐jet  

Page 12: Prospects)(perspec+ves))from) Tevatron)Higgs) fileTEV,)CMS,)ATLAS) Higgs boson mass (GeV/c2) 120 140 160 180 200 220 SM! / 95%! Limit on 1 10 Observed S CL Expected ± 1! S CL Expected

•  Tevatron  can  provide  independent  check  

B.Kilminster,  Higgs  Hun+ng   12  

Could  WW  excesses  at  CMS  &  ATLAS  be  correlated  background  mis-­‐modeling  ?  

Page 13: Prospects)(perspec+ves))from) Tevatron)Higgs) fileTEV,)CMS,)ATLAS) Higgs boson mass (GeV/c2) 120 140 160 180 200 220 SM! / 95%! Limit on 1 10 Observed S CL Expected ± 1! S CL Expected

•  Tevatron  can  provide  independent  check  

B.Kilminster,  Higgs  Hun+ng   13  

Could  WW  excesses  at  CMS  &  ATLAS  be  correlated  background  mis-­‐modeling  ?  

ATLAS  (and  CMS)  have  small  Z+jets  (green)  contribu+on  at  low  MT  where  excess  is  

1-­‐jet  bin  

Page 14: Prospects)(perspec+ves))from) Tevatron)Higgs) fileTEV,)CMS,)ATLAS) Higgs boson mass (GeV/c2) 120 140 160 180 200 220 SM! / 95%! Limit on 1 10 Observed S CL Expected ± 1! S CL Expected

•  Tevatron  can  provide  independent  check  

B.Kilminster,  Higgs  Hun+ng   14  

Could  WW  excesses  at  CMS  &  ATLAS  be  correlated  background  mis-­‐modeling  ?  

ATLAS  (and  CMS)  have  small  Z+jets  (green)  contribu+on  at  low  MT  where  excess  is  

1-­‐jet  bin  

CDF  has  large  Z+jets  (yellow)  contribu+on  at  low  MT  in  same  region  •   And  much  smaller  obar  

1-­‐jet  bin  

Page 15: Prospects)(perspec+ves))from) Tevatron)Higgs) fileTEV,)CMS,)ATLAS) Higgs boson mass (GeV/c2) 120 140 160 180 200 220 SM! / 95%! Limit on 1 10 Observed S CL Expected ± 1! S CL Expected

Tevatron  cross-­‐checks  of  excesses  

•  Doesn’t  mean  Z+jets  is  underes+mated  at  CMS/ATLAS  –  Since  W+jets  and  Z+jets  should  be  smaller  backgrounds  at  LHC  anyway  

•  But  it  does  mean  that  excesses  at  LHC  or  Tevatron  could  be  due  to  different  backgrounds  –  Consistent  excesses  between  Tevatron  and  LHC  would  constrain  background  fluctua+on  interpreta+on  

•  Tevatron  also  more  sensi+ve  from  WH/ZH  produc+on  in  high  mass  analysis,  whereas  LHC  has  more  from  VBF  –  Consistent  excesses  between  Tevatron  and  LHC  would  indicate  SM  Higgs  boson  rela+onship  (ggH,  WH/ZH,  VBF)  

•  Tevatron  H➞WW  important  even  when  sensi+vity  is  eclipsed  

B.Kilminster,  Higgs  Hun+ng   15  

Page 16: Prospects)(perspec+ves))from) Tevatron)Higgs) fileTEV,)CMS,)ATLAS) Higgs boson mass (GeV/c2) 120 140 160 180 200 220 SM! / 95%! Limit on 1 10 Observed S CL Expected ± 1! S CL Expected

What  does  Tevatron  say  about  excesses  ?  

B.Kilminster,  Higgs  Hun+ng   16  

Page 17: Prospects)(perspec+ves))from) Tevatron)Higgs) fileTEV,)CMS,)ATLAS) Higgs boson mass (GeV/c2) 120 140 160 180 200 220 SM! / 95%! Limit on 1 10 Observed S CL Expected ± 1! S CL Expected

17  B.Kilminster,  Higgs  Hun+ng  

Actual  Tevatron  data  

Signal  injected  at  115  GeV   Signal  injected  at  125  GeV   Signal  injected  at  135  GeV  

Not  quite  consistent  with  130  GeV  injec+on    

Page 18: Prospects)(perspec+ves))from) Tevatron)Higgs) fileTEV,)CMS,)ATLAS) Higgs boson mass (GeV/c2) 120 140 160 180 200 220 SM! / 95%! Limit on 1 10 Observed S CL Expected ± 1! S CL Expected

Tevatron  perspec+ve  from  H➞bb  

B.Kilminster,  Higgs  Hun+ng   18  

Page 19: Prospects)(perspec+ves))from) Tevatron)Higgs) fileTEV,)CMS,)ATLAS) Higgs boson mass (GeV/c2) 120 140 160 180 200 220 SM! / 95%! Limit on 1 10 Observed S CL Expected ± 1! S CL Expected

Let’s  check  Tevatron  H➞bb    

19  

•  At  115-­‐120    GeV  –  Almost  at  1*SM  sensi+vity    –  No  excess  seen  –  Inconsistent  with  CMS  &  ATLAS  

•  At  130-­‐140  GeV  –  2*SM  –  3*SM  sensi+vity  –  No  excess  seen  –  would  expect  observed  limit  to  be  1*SM  high  

B.Kilminster,  Higgs  Hun+ng  

Signal  injected  at  115  GeV  

)2Higgs Mass (GeV/c100 110 120 130 140 150

95%

CL

Lim

it/SM

1

10

210 1±Expected Limits

2±Expected Limits

2=115 GeV/cH

Expected with Injected M

)-1CDF II x 2 Preliminary (5.7 fb

Page 20: Prospects)(perspec+ves))from) Tevatron)Higgs) fileTEV,)CMS,)ATLAS) Higgs boson mass (GeV/c2) 120 140 160 180 200 220 SM! / 95%! Limit on 1 10 Observed S CL Expected ± 1! S CL Expected

Let’s  check  Tevatron  H➞bb    

20  

•  At  115-­‐120    GeV  –  Almost  at  1*SM  sensi+vity    –  No  excess  seen  –  Inconsistent  with  CMS  &  ATLAS  

•  At  130-­‐140  GeV  –  2*SM  –  3*SM  sensi+vity  –  No  excess  seen  –  would  expect  observed  limit  to  be  1*SM  high  

B.Kilminster,  Higgs  Hun+ng  

Signal  injected  at  115  GeV  

)2Higgs Mass (GeV/c100 110 120 130 140 150

95%

CL

Lim

it/SM

1

10

210 1±Expected Limits

2±Expected Limits

2=115 GeV/cH

Expected with Injected M

)-1CDF II x 2 Preliminary (5.7 fb

Not  consistent  with  115  GeV  injec+on    

Page 21: Prospects)(perspec+ves))from) Tevatron)Higgs) fileTEV,)CMS,)ATLAS) Higgs boson mass (GeV/c2) 120 140 160 180 200 220 SM! / 95%! Limit on 1 10 Observed S CL Expected ± 1! S CL Expected

Higgs  Boson  Mass  Msmst  19  Aug  2010   21  

How  well  could  we  measure  Higgs  mass  given  a  3  Sigma  excess    ?    -­‐  Cross-­‐sec+on  is  more  sensi+ve  to  Higgs  boson  mass  than  resolu+on    

Using  resolu+on  from  LLR,  median  outcomes  Resolu+on  at  115  GeV:    ±5  GeV  Resolu+on  at  135  GeV:    ~±10  GeV  

Assuming  Cross  Sec+on  x  Branching  Frac+on  Measurement  Uncertainty  is  2x  Larger  at  the  same  Luminosity  for  low-­‐mass  than  it  is  for  high-­‐mass  searches  

Page 22: Prospects)(perspec+ves))from) Tevatron)Higgs) fileTEV,)CMS,)ATLAS) Higgs boson mass (GeV/c2) 120 140 160 180 200 220 SM! / 95%! Limit on 1 10 Observed S CL Expected ± 1! S CL Expected

Tevatron  prospects  from  H➞bb  

B.Kilminster,  Higgs  Hun+ng   22  

Page 23: Prospects)(perspec+ves))from) Tevatron)Higgs) fileTEV,)CMS,)ATLAS) Higgs boson mass (GeV/c2) 120 140 160 180 200 220 SM! / 95%! Limit on 1 10 Observed S CL Expected ± 1! S CL Expected

Background  modeling  at  115  GeV    

•  BKG  modeling  impressive  over  7  orders  of  magnitude  –  Dominated  by  b-­‐tagged  W+jets,  Z+jets  

B.Kilminster,  Higgs  Hun+ng   23  

Page 24: Prospects)(perspec+ves))from) Tevatron)Higgs) fileTEV,)CMS,)ATLAS) Higgs boson mass (GeV/c2) 120 140 160 180 200 220 SM! / 95%! Limit on 1 10 Observed S CL Expected ± 1! S CL Expected

Mjj  bump  •  Important  for  H➞bb  searches  at  115  GeV  to  have  reliable  modeling  of  main  backgrounds  :  W+jets,  Z+jets  –  However  …      

24  B.Kilminster,  Higgs  Hun+ng  

Page 25: Prospects)(perspec+ves))from) Tevatron)Higgs) fileTEV,)CMS,)ATLAS) Higgs boson mass (GeV/c2) 120 140 160 180 200 220 SM! / 95%! Limit on 1 10 Observed S CL Expected ± 1! S CL Expected

Mjj  bump  •  Important  for  H➞bb  searches  at  115  GeV  to  have  reliable  modeling  of  main  backgrounds  :  W+jets,  Z+jets  –  However  …      

25  

147  ±  4  GeV  4.8  σ  

Bump  from  subtrac+on  of  two  falling  distribu+ons  

B.Kilminster,  Higgs  Hun+ng  

Page 26: Prospects)(perspec+ves))from) Tevatron)Higgs) fileTEV,)CMS,)ATLAS) Higgs boson mass (GeV/c2) 120 140 160 180 200 220 SM! / 95%! Limit on 1 10 Observed S CL Expected ± 1! S CL Expected

Mjj  bump  •  Important  for  H➞bb  searches  at  115  GeV  to  have  reliable  modeling  of  main  backgrounds  :  W+jets,  Z+jets  –  However  …      

CDF  is  working  toward  understanding  if  this  is  caused  by  an  unaccounted  for  systema+c  uncertainty  –  and  to  quan+fy  the  effect  on  top  and  Higgs  analyses  

26  

147  ±  4  GeV  4.8  σ  

Bump  from  subtrac+on  of  two  falling  distribu+ons  

B.Kilminster,  Higgs  Hun+ng  

Page 27: Prospects)(perspec+ves))from) Tevatron)Higgs) fileTEV,)CMS,)ATLAS) Higgs boson mass (GeV/c2) 120 140 160 180 200 220 SM! / 95%! Limit on 1 10 Observed S CL Expected ± 1! S CL Expected

Mjj  bump  tests  •  Tests  of  varying  background  normaliza+ons  and  shapes  with  extreme  varia+ons  of  known  systema+c  uncertain+es  have  been  done  

27  B.Kilminster,  Higgs  Hun+ng  

Page 28: Prospects)(perspec+ves))from) Tevatron)Higgs) fileTEV,)CMS,)ATLAS) Higgs boson mass (GeV/c2) 120 140 160 180 200 220 SM! / 95%! Limit on 1 10 Observed S CL Expected ± 1! S CL Expected

Mjj  bump  tests  •  Tests  of  varying  background  normaliza+ons  and  shapes  with  extreme  varia+ons  of  known  systema+c  uncertain+es  have  been  done  

28  B.Kilminster,  Higgs  Hun+ng  

–  it’s  not  them  …  

Page 29: Prospects)(perspec+ves))from) Tevatron)Higgs) fileTEV,)CMS,)ATLAS) Higgs boson mass (GeV/c2) 120 140 160 180 200 220 SM! / 95%! Limit on 1 10 Observed S CL Expected ± 1! S CL Expected

Mjj  bump  tests  •  Tests  of  varying  background  normaliza+ons  and  shapes  with  extreme  varia+ons  of  known  systema+c  uncertain+es  have  been  done  

29  B.Kilminster,  Higgs  Hun+ng  

From    Adam  Mar+n  (FNAL)  

Cross-­‐over  in  quark  /    gluon  jet  composi+on      as  func+on  of  Mjj  around    CDF  bump    

Best  lead  :  

–  it’s  not  them  …  

Page 30: Prospects)(perspec+ves))from) Tevatron)Higgs) fileTEV,)CMS,)ATLAS) Higgs boson mass (GeV/c2) 120 140 160 180 200 220 SM! / 95%! Limit on 1 10 Observed S CL Expected ± 1! S CL Expected

Quarks  vs.  gluons  •  Cut  on  ra+o  of  highest  PT  /  lowest  PT  sensi+ve  to  quark  and  gluon  frac+ons  

30  

Standard  (j1,j2  ET  >30  GeV)   J1  Et  /  j2  Et  >  0.6   J1  Et  /  j2  Et  >  0.8  

B.Kilminster,  Higgs  Hun+ng  

Page 31: Prospects)(perspec+ves))from) Tevatron)Higgs) fileTEV,)CMS,)ATLAS) Higgs boson mass (GeV/c2) 120 140 160 180 200 220 SM! / 95%! Limit on 1 10 Observed S CL Expected ± 1! S CL Expected

Quarks  vs.  gluons  •  Cut  on  ra+o  of  highest  PT  /  lowest  PT  sensi+ve  to  quark  and  gluon  frac+ons  

31  

Standard  (j1,j2  ET  >30  GeV)   J1  Et  /  j2  Et  >  0.6   J1  Et  /  j2  Et  >  0.8  

4.8  σ   3.2  σ  3.6  σ  

B.Kilminster,  Higgs  Hun+ng  

Page 32: Prospects)(perspec+ves))from) Tevatron)Higgs) fileTEV,)CMS,)ATLAS) Higgs boson mass (GeV/c2) 120 140 160 180 200 220 SM! / 95%! Limit on 1 10 Observed S CL Expected ± 1! S CL Expected

Quarks  vs.  gluons  •  Cut  on  ra+o  of  highest  PT  /  lowest  PT  sensi+ve  to  quark  and  gluon  frac+ons  

32  

Standard  (j1,j2  ET  >30  GeV)   J1  Et  /  j2  Et  >  0.6   J1  Et  /  j2  Et  >  0.8  

4.8  σ   3.2  σ  3.6  σ  

No  obvious  magic  bullet  :  decrease  sta+s+cs  ➞  decreased  significance  B.Kilminster,  Higgs  Hun+ng  

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Separa+ng  quarks  from  gluons  •  More  recently,  we  have  been  doing  studies  with  a  quark-­‐jet  vs.  gluon-­‐jet  separator  

33  B.Kilminster,  Higgs  Hun+ng  

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Test  of  quark  gluon  composi+on  •  We  test  an  orthogonal  sample  Z+jet  to  check  jet  energy  

scale  as  a  func+on  of  quark-­‐jet  vs.  gluon-­‐jet  discriminator  

34  

“true“  jet  PT    determined  from  Z+jet  balancing  

B.Kilminster,  Higgs  Hun+ng  

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Test  of  quark  gluon  composi+on  •  We  test  an  orthogonal  sample  Z+jet  to  check  jet  energy  

scale  as  a  func+on  of  quark-­‐jet  vs.  gluon-­‐jet  discriminator  

35  

“true“  jet  PT    determined  from  Z+jet  balancing  

Best  agreement  found  when  :    •   Quark  jet  energy  scale  le{  alone  •   Gluon  jet  energy  scale  shi{ed  down  in  MC  by  2  Sigma  

B.Kilminster,  Higgs  Hun+ng  

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Test  of  quark  gluon  composi+on  •  We  test  an  orthogonal  sample  Z+jet  to  check  jet  energy  

scale  as  a  func+on  of  quark-­‐jet  vs.  gluon-­‐jet  discriminator  

36  

“true“  jet  PT    determined  from  Z+jet  balancing  

Explains  why  in  situ  JES  measurement  from  W➞qq  in  obar  decays  indicates  JES  is  stable  to  0.3  sigma    

Also,  explains  why  W+jets  and    Z+jets  do  not  have  mis-­‐modeling  when  b-­‐tag  is  applied  (due  to  quark  enhancement)  

B.Kilminster,  Higgs  Hun+ng  

Best  agreement  found  when  :    •   Quark  jet  energy  scale  le{  alone  •   Gluon  jet  energy  scale  shi{ed  down  in  MC  by  2  Sigma  

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Applying  the  correc+on  as  a  func+on  of  Q-­‐G  discriminator  output  

37  

Gluon-­‐enriched   Quark-­‐enriched  

Includes  2σ  JES  down  for  gluons  in  MC  

B.Kilminster,  Higgs  Hun+ng  

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Effect  on  W+jj    Mjj  distribu+on  •  CDF  studies  underway  –  Hope  to  have  a  convincing  answer  soon  whether    gluon-­‐jet  JES  2  σ  down  solves  problem  of  Mjj  bump  

•  D0  does  not  see  Mjj  bump  •  Specula+on  –  Perhaps  D0  not  as  sensi+ve  to  quark  vs.  gluon  JES  differences  •  Larger  cone  size  0.5  instead  of  0.4  •  Different  calorimeter  

–  D0  has  compensa+ng  liquid  argon  calorimeter  

–  CDF  has  lead  &  iron  /  sampling  scin+lla+ng  calorimeter    

38  B.Kilminster,  Higgs  Hun+ng  

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Good  news  is  none  of  this  would  effect  WH/ZH  ➞  lv/ll/vv  +  bb  searches  

•  And  they  s+ll  have  excellent  modeling  

B.Kilminster,  Higgs  Hun+ng   39  

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Future  

B.Kilminster,  Higgs  Hun+ng   40  

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Tevatron  expecta+ons  

•  Tevatron  will  deliver  over  12  J-­‐1  by  Sept.  2011  –  10  J-­‐1  acquired  data  by  CDF  and  D0  

•  Effec+vely  means  ~9  J-­‐1  for  use  with  all  detector  systems  good  (necessary  WH,  ZH  b-­‐tagged  analyses)  

41  B.Kilminster,  Higgs  Hun+ng  

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Tevatron  projec+ons  10  J-­‐1  analyzed  

3  σ    :  115  GeV    w/9  J-­‐1  

2.4  σ  :    130  GeV  w/10  J-­‐1   42  B.Kilminster,  Higgs  Hun+ng  

10  J-­‐1  

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Are  there  poten+al  improvements  le{  ?  

B.Kilminster,  Higgs  Hun+ng   43  

Some  of  these    Improvements  were  made  for  summer  

Es+mates  of    remaining  :  35%  WH  65%  ZHllbb  12%  ZHvvbb  

from  P5  report  Oct.  2010  

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More  importantly,  can  Tevatron  achieve  all  projected  improvements  on  +me-­‐scale  of  Moriond  2012?  

•  Are  improvements  slowing  down  due  to  reduced  personnel  ?  

B.Kilminster,  Higgs  Hun+ng   44  

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More  importantly,  can  Tevatron  achieve  all  projected  improvements  on  +me-­‐scale  of  Moriond  2012?  

•  Are  improvements  slowing  down  due  to  reduced  personnel  ?  

B.Kilminster,  Higgs  Hun+ng   45  

WH  ➞  lvbb  

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More  importantly,  can  Tevatron  achieve  all  projected  improvements  on  +me-­‐scale  of  Moriond  2012?  

•  Are  improvements  slowing  down  due  to  reduced  personnel  ?  

B.Kilminster,  Higgs  Hun+ng   46  

WH  ➞  lvbb  ZH  ➞  llbb  

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S+ll  incorpora+ng  new  channels  to  improve  sensi+vity  at  115  GeV  and  130  GeV  

•  See  Elisabeoa’s  talk  yesterday  – New  addi+ons  for  summer  2011  Tev  combina+on  •  oH  ➞  met+jets  •  oH  ➞  leptons+jets  

•  oH  ➞  all-­‐jets  • WH  ➞  lvττ  

•  ZH  ➞  llττ  

B.Kilminster,  Higgs  Hun+ng   47  

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Conclusions  

•  Tevatron  important  at  low  mass  115  –  125  GeV  –  Best  current  limits  at  115  GeV  – Unique  window  to  Higgs  of  H➞bb    –  Sensi+vity  con+nues  to  improve  

•  Tevatron  important  in  130-­‐140  GeV  region  – H➞WW  analyses  sensi+ve  to  different  signals  and  backgrounds  than  LHC  •  LHC  –  Tevatron  agreement  paints  a  consistent  picture  

•  Tevatron  will  have  10  J-­‐1  analyzed  by  spring/summer  2012  – Will  have  even  more  to  say  about  115  GeV  and  130  GeV  

B.Kilminster,  Higgs  Hun+ng   48  

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49  

Found  that  s/b(max)  is  the  single  most    important  determinant  of  our  measurement  sensi+vity.  

Other  things  maoer,  like  the  candidate  mass  resolu+on,  mostly  via  their  impact  on  this  variable.  

Signal  cross  sec+on  x  b.r.  to  bb  is  lower  at  higher  mH,    WW  channels  turning  on  without  mrec  info.      

Guess  –  probably  can’t  get  much  beoer  than  6%  

Let’s  call  it  ±11  GeV  when  we  have  all  the  excess  from  low-­‐mass  channels.  

B.Kilminster,  Higgs  Hun+ng  

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50  

Leveraging  our  Rate  Measurements  to          Measure  the  Higgs  Boson  Mass  

Assuming  SM  cross  sec+ons  and  branching  frac+ons,  measured  rates  are  strong  func+ons  of  mH.    Example  at  mH=115  GeV,  assuming  +3  sigma  excess,  and  a  median  outcome  in  both  the  bb,ττ  channels  and  the  WW  channels:  

Tau  channels  can  contribute  here,  even  with  less  precise  mrec  than  the  bb  channels  

B.Kilminster,  Higgs  Hun+ng