relic density at the lhc b. dutta in collaboration with: r. arnowitt, a. gurrola, t. kamon, a....
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![Page 1: Relic Density at the LHC B. Dutta In Collaboration With: R. Arnowitt, A. Gurrola, T. Kamon, A. Krislock, D.Toback Phys.Lett.B639:46,2006, hep-ph/0608193](https://reader037.vdocuments.mx/reader037/viewer/2022110322/56649d235503460f949fa161/html5/thumbnails/1.jpg)
Relic Density at the LHC
B. Dutta
In Collaboration With:
R. Arnowitt, A. Gurrola, T. Kamon, A. Krislock, D.Toback
Phys.Lett.B639:46,2006, hep-ph/0608193 (Phys. Lett.B), To appear
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The signal to look for: 4 jet + missing ET
SUSY in Early Stage at the LHC
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Kinematical Cuts and Event Selection ET
j1 > 100 GeV, ETj2,3,4 > 50 GeV
Meff > 400 GeV (Meff ETj1+ET
j2+ETj3+ET
j4+ ETmiss)
ETmiss > Max [100, 0.2 Meff]
Phys. Rev. D 55 (1997) 5520
Example Analysis
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SUSY scale is measured with an accuracy of 10-20%
This measurement does not tell us whether the model can generate the right amount of dark matter.
The dark matter content is measured to be 23% with an accuracy of less than 5% at WMAP
Question:
To what accuracy can we calculate the relic density based on the measurements at the LHC?
Relic Density and Meff
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We establish the dark matter allowed regions from the detailed features of the signals.
We accurately measure the masses.
We calculate the relic density and compare with WMAP.
Strategy
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Dark Matter Allowed Regions
Neutralino-stau coannihilation region
A-annihilation funnel region – This appears for large values of m1/2
Focus point region – the lightest neutralino has a larger higgsino component
We choose mSUGRA model. However, the results can be generalized.
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2
1CDM
+…
In the stau neutralino coannihilation region
01~
1~
20Δ
2
/Me
011
~~ MMM Δ
Griest, Seckel ’91
Relic Density Calculation
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2GeV) 37(21/2
15020
2cE
m.m~m
In mSUGRA model the lightest stau seems to be naturally close to the lightest neutralino mass especially for large tan
For example, the lightest selectron mass is related to the lightest neutralino mass in terms of GUT scale parameters:
For larger m1/2 the degeneracy is maintained by increasing m0 and we get a corridor in the m0 - m1/2
plane.
The coannihilation channel occurs in most SUGRA models with non-universal soft breaking,
21/2
160201
m.~
m
Thus for m0 = 0, becomes degenerate with at m1/2 = 370 GeV, i.e. the coannihilation region begins at
0
1
~2
cE~
m1/2 = (370-400) GeV
Coannihilation, GUT Scale
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tan= 40, > 0, A0 = 0
011 ~~
GeV 155
011
~
MMM ~~
Can we measure M at colliders?
Coannihilation Region
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SUSY at LHC
In Coannihilation Region of SUSY Parameter Space:
Soft
Soft
p p p
g~
q~
01
~
02
~
~
q
q~q
q
~ 01
~
02
~
p
g~
q~
01
~
02
~
~
1
~
q
q~q
q
~ 01
~
Soft
Hard Hard
Hard
15 - 5 ~ )~~( 0
11 MFinal state: 3/4 s+jets +missing energy
Signals
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2. Use Counting Method (NOS-LS) & Ditau Invariant Mass (M) to measure mass difference
Use Hadronically Decaying and construct 3 observables
1.Sort τ’s by ET (ET1 > ET
2 > …) and use
OS-LS method to extract pairs from the decays
3. Measure the PT of the low energy
Observables
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Since we are using 3 variables, we can measure M, Mgluino and the universality relation of the gaugino masses i.e. 1/2χ~1/2χ~1/2g~
0.4m~M,0.8m~M ,2.8m~M 01
02
Mgluino measured from the Meff method may not be accurate for this parameter space since the tau jets may pass as jets in the Meff observable.
The accuracy of measuring these parameters are important for calculating relic density.
SUSY Parameters
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Version 7.69 (m1/2 = 347.88, m0 = 201.06) Mgluino = 831
Chose di- pairs from neutralino decays with (a) || < 2.5(b) = hadronically-decaying tau
Nu
mb
er o
f C
oun
ts /
1 G
eV
(GeV) visM
ETvis(true) > 20, 20 GeV
ETvis(true) > 40, 20 GeV
ETvis(true) > 40, 40 GeV
GeV) 5.7(
011
02
M
~~~
0162
141143
441137
116264
1
01
02
.endpont
.~.~.~
ET > 20 GeV is essential!
Mvis in ISAJET
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EVENTS WITH CORRECT FINAL STATE : 1 + 3j + ETmiss
APPLY CUTS TO REDUCE SM BACKGROUND (W+jets, …)
ETmiss > 100 GeV, ET
j1 > 100 GeV, ETmiss + ET
j1 > 400 GeV
ORDER TAUS BY PT & APPLY CUTS ON TAUS: WE EXPECT A SOFT AND A HARD
PT > 40, 40, 20 GeV,
LOOK AT PAIRS AND CATEGORIZE THEM AS OPPOSITE SIGN (OS) OR LIKE SIGN (LS)
OS: FILL LOW OS PT HISTOGRAM WITH PT OF SOFTER
FILL HIGH OS PT HISTOGRAM WITH PT OF HARDER
LS: FILL LOW LS PT HISTOGRAM WITH PT OF SOFTER
FILL HIGH LS PT HISTOGRAM WITH PT OF HARDER
LOW OS
HIGH OS
LOW LS
HIGH LS
LOW OS-LS
HIGH OS-LS
Extracting Pairs from Decays02
~EETTmissmiss + 1j+ 1j ++ 33 Analysis PathAnalysis Path
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ETmiss + 1j + 3 Analysis
Much smaller SM background, but a lower acceptance
[1] ISAJET + PGS sample of ETmiss, 1 jet and at least 3 taus with pT
vis > 40,
40, 20 GeV and = 50%, fake (fj ) = 1%. Final cuts :
ETjet1 > 100 GeV, ET
miss > 100 GeV, ETjet1 + ET
miss > 400 GeV
[2] Select OS low di-tau mass pairs, subtract off LS pairs
Note: fj = 0% 1.6 counts/fb1
Small dependence on the uncertainty of fj
3 +1 Jet
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Next: combine NOS-LS and M values to measure M and Mgluino simultaneously
Counts drop with Mgluino
Mass rises with Mgluino
M/M ~15% and Mgluino/Mgluino ~6%
3 +1 Jet (contd)
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EVENTS WITH CORRECT FINAL STATE : 2 + 2j + ETmiss
APPLY CUTS TO REDUCE SM BACKGROUND (W+jets, …)
ETmiss > 180 GeV, ET
j1 > 100 GeV, ETj2 > 100 GeV, ET
miss + ETj1 + ET
j2 > 600 GeV
ORDER TAUS BY PT & APPLY CUTS ON TAUS: WE EXPECT A SOFT AND A HARD
PTall > 20 GeV, PT
1 > 40 GeV
LOOK AT PAIRS AND CATEGORIZE THEM AS OPPOSITE SIGN (OS) OR LIKE SIGN (LS)
OS: FILL LOW OS PT HISTOGRAM WITH PT OF SOFTER
FILL HIGH OS PT HISTOGRAM WITH PT OF HARDER
LS: FILL LOW LS PT HISTOGRAM WITH PT OF SOFTER
FILL HIGH LS PT HISTOGRAM WITH PT OF HARDER
LOW OS
HIGH OS
LOW LS
HIGH LS
LOW OS-LS
HIGH OS-LS
02
~EETTmissmiss + 2j + + 2j + 22 Analysis PathAnalysis Path
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ETmiss + 2j + 2 Analysis
[1] ISAJET + ATLFAST sample of ETmiss, 2 jets, and at least 2 taus with
pTvis > 40, 20 GeV and = 50%, fake (fj ) = 1%. Optimized cuts :
ETjet1 > 100 GeV; ET
jet2 > 100 GeV; ETmiss > 180 GeV; ET
jet1 + ETjet2 + ET
miss > 600 GeV
[2] Number of SUSY and SM events (10 fb1):Top : 115 eventsW+jets : 44 eventsSUSY : 590 events
top SUSYMgluino = 830 GeVM = 10.6 GeV)
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A small M can be detected in first few years of LHC.
10-20 fb110-20 fb1
2 Analysis : Discovery Luminosity
+5%
5%[Assumption] The gluino mass is measured with M/Mgluino = 5% in a separate analysis.
Negligible fjdependence
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PT STUDY
Slope of the soft PT distribution has a M dependence
Phys.Lett. B639 (2006) 46, hep-ph/06031280
1~~
Slope of PT distribution contains ΔM Information.
PTsoft in ISAJET
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OS
OS-LS
LS
GeVM
GeVM
g 831
6.10
~
[1] ETmiss , at least 2 jets, at least 2 ’s with PT
vis > 20, 40 GeV
[2] = 50% , fake rate 1%
[3] Cuts: ETjet1 > 100 GeV, ET
jet2 > 100 GeV, ETmiss > 180 GeV
ETjet1 + ET
jet2 + ETmiss > 600 GeV
ETmiss + 2j + 2Analysis: PT
soft
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Can we still see the dependence of the PT slope on M using OS-LS Method?
GeV 015
GeV 610
GeV 75
GeV 3260
GeV 831
02
.M
.M
.M
.M
M
~
g~
PT Study
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Measuring M from the PT Slope
Luminosity = 40 fb-1
Slope of PT
PT does not depend on the mass or the mass 02
~M
gM ~
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How accurately can M be measured for our reference point?
Considering only the statistical uncertainty:
We can measure M to ~ 6% accuracy at 40 fb-1 & ~ 12% accuracy at 10 fb-1 for mass
of 831 GeV.
g~
Slope of PT M
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Can parameterize the our observables as functions of M, , &
NOS-LS , to first order, does not depend on mass. A large increase or decrease
in mass is needed to obtain a point that lies outside the error bars Cross-Section is dominated by the gluino mass
02
~02
~
gM ~ 02
~M
Model Parameters
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2~
2
~
2
~
2~
~
1
01
02
1
02
11
M
M
M
MMM end
Model Parameters
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CONTOURS OF CONSTANT VALUES ( L = 40 fb-1 )
• Intersection of the central contours
provides the measurement of M,
, &
• Auxilary lines determine the 1
region
• 1st order test on Universality
gM ~ 02
~M
Testing Gaugino Universality
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M and Mgluino m0 and m1/2
(for fixed A0 and tan
We determine m0/m0 ~ 1.2% and m1/2/m1/2 ~2 % (for A0=0, tan=40)
Determination of m0 and m1/2
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M and Mgluino (for fixed A0 and tan)
Determination of
201h~
h2/h2 ~ 7% (for A0=0, tan=40)
201h~
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h2/h2 ~ 7% for A0=0, tan=40
Analysis with visible ET > 20 GeV establishes stau-
neutralino coannihilation region
2 analysis: Discovery with 10 fb1 M/M ~ 5% , mg/mg ~ 2% using Mpeak, NOS-LS and pT
The analyses can be done for the other models that don’t suppress 2
0 production.
Meff will establish the existence of SUSY
Different observables are needed to establish
the dark matter allowed regions in SUSY model at the LHC
Universality of gaugino masses can be checked
Conclusion