Long-range azimuthal correlations in 2.76 & 13 TeV pp with ATLAS
Andy Buckley
University of Glasgow
MPI@LHC 2015, Trieste, 2015-11-26
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Long-range azimuthal correlations in 2.76 & 13 TeV pp with ATLAS - - PowerPoint PPT Presentation
Long-range azimuthal correlations in 2.76 & 13 TeV pp with ATLAS Andy Buckley University of Glasgow MPI@LHC 2015, Trieste, 2015-11-26 1/9 Introduction to the ridge The near-side ridge phenomenon has been one of the most prominent
University of Glasgow
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arXiv:1212.5198
ch .
rec ch
N 50 100 150 Events / 3 1 10
210
310
410
510
610
710 ATLAS =2.76 TeV s rec ch N 50 100 150 200 1 10
2 3 4 5 6 7ATLAS =13 TeV s
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T, ηa) ǫ(pb T, ηb).
φ ∆
2 4
η ∆
2 4
) φ ∆ , η ∆ C(
0.95 1 1.05 1.1 ATLAS =13 TeV s <5.0 GeV
a,b T
0.5<p <30
rec ch
N ≤ 10 φ ∆ 2 4 η ∆
2 4
) φ ∆ , η ∆ C(
0.98 1 1.02 ATLAS =13 TeV s <5.0 GeV
a,b T
0.5<p 120 ≥
rec ch
N
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2
2 4
) φ ∆ Y( 0.5 0.6 0.7 =13 TeV s =2.76 TeV s ATLAS <20
rec ch
N ≤ |<5.0 η ∆ 2.0<| <5.0 GeV
a,b T
0.5<p (a) 2 4 ) φ ∆ Y( 2.3 2.35 2.4 2.45 ) φ ∆ Y( )+G φ ∆ (
periph
FY (0)
periph
+ FY
ridge
Y ) φ ∆ (
templ
Y =13 TeV s <50
rec ch
N ≤ 40 (b) 2 4 ) φ ∆ Y( 2.9 2.95 3 3.05 3.1 =2.76 TeV s <60
rec ch
N ≤ 50 (c) 2 4 ) φ ∆ Y( 3.4 3.45 3.5 3.55 3.6 =13 TeV s <70
rec ch
N ≤ 60 (d)
φ ∆
2 4
) φ ∆ Y(
4 4.1 4.2 =2.76 TeV s <80
rec ch
N ≤ 70 (e)
φ ∆
2 4
) φ ∆ Y(
5.5 5.6 5.7 =13 TeV s 90 ≥
rec ch
N (f)
Increasing modulation with Nch fills in the near-side minimum ⇒ produces the ridge, and narrows + heightens the far-side peak.
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2 4
) φ ∆ Y( 0.5 0.6 0.7 =13 TeV s =2.76 TeV s ATLAS <20
rec ch
N ≤ |<5.0 η ∆ 2.0<| <5.0 GeV
a,b T
0.5<p (a) 2 4 ) φ ∆ Y( 2.3 2.35 2.4 2.45 ) φ ∆ Y( )+G φ ∆ (
periph
FY (0)
periph
+ FY
ridge
Y ) φ ∆ (
templ
Y =13 TeV s <50
rec ch
N ≤ 40 (b) 2 4 ) φ ∆ Y( 2.9 2.95 3 3.05 3.1 =2.76 TeV s <60
rec ch
N ≤ 50 (c) 2 4 ) φ ∆ Y( 3.4 3.45 3.5 3.55 3.6 =13 TeV s <70
rec ch
N ≤ 60 (d)
φ ∆
2 4
) φ ∆ Y(
4 4.1 4.2 =2.76 TeV s <80
rec ch
N ≤ 70 (e)
φ ∆
2 4
) φ ∆ Y(
5.5 5.6 5.7 =13 TeV s 90 ≥
rec ch
N (f)
Yperiph and Yridge as open points and blue line respectively; Ytempl in red fits several data features with 2 params on one sinusoid.
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T, pb T) = v2(pa T)v2(pb T).
T bins vs track
ch . Extract v2 from
T bins in v2,2:
T and
20 40 60 80 100 2,2
v
0.002 0.004 0.006 =2.76 TeV s ATLAS 20 40 60 80 100 120 0.002 0.004 0.006 =13 TeV s
rec ch
N
20 40 60 80 100 2
v
0.05 0.1 =2.76 TeV s
rec ch
N
20 40 60 80 100 120 0.05 0.1 <5.0 GeV
b T
0.5<p <1.0 GeV
b T
0.5<p <3.0 GeV
b T
2.0<p =13 TeV s |<5.0 η ∆ 2.0<| <5.0 GeV
a T
0.5<p [GeV]
a T
p
1 2 3 4 2
v
0.05 0.1 =2.76 TeV s =13 TeV s ATLAS |<5.0 η ∆ 2.0<| <5.0 GeV
b T
0.5<p <60
rec ch
N ≤ 50 [GeV]
a T
p
1 2 3 4 0.05 0.1 <50
rec ch
N ≤ 40 <80
rec ch
N ≤ 70 100 ≥
rec ch
N =13 TeV s
Extraction of v2(pa
T) showing stability
vs pb
T bin and Nrec ch .
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ch :
ch dependence of Yperiph extraction by
ch
ch + linear growth of G + flattening of F
ch
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ch :
ch dependence of Yperiph extraction by
ch
ch + linear growth of G + flattening of F
ch
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◮ The near-side ridge is still a major puzzle in LHC physics. Still
◮ A new fit of the ∆φ modulation in these pp events shows excellent
ch . ◮ Comparison of the v2,2 Fourier coefficient in ∆φ yields between pT
ch and pb T: consistent
◮ It hence appears that the pp and p + Pb ridge phenomena have the
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