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Positr on Fraction from Dark MatterAnnihilation in the CMSSM
Wim de Boer, Markus Horn, Christian Sander
IEKP, Univer sity Karlsruhe
Wim.de .Boer@cern.c h http://home .cern.c h/˜deboerw
ICHEP, Amster dam, July, 2002
OutlineCMSSM Constraints
Positr on fraction in the CMSSM Parameter Space
Comparison with HEAT and AMS data
Summar y
Wim de Boer ICHEP, Amster dam, July, 2002 1
Typical Fits to AMS+HEAT Data vs
10-3
10-2
10-1
1
1 10 102
positron energy [GeV]
e+ /(e+ +
e- ) fr
acti
on
b b–
τ+ τ-
W+ W-
bg+22200• signal χ2=24.2
bg (ep-scaling=0.91)
bg only fit χ2=48.0
HEAT 94/95/2000
AMS 01
tanβ= 1.6; m0= 200; m1/2= 300
10-3
10-2
10-1
1
1 10 102
positron energy [GeV]e+ /(
e+ + e- )
frac
tion
t t–
b b–
τ+ τ-
bg+650•signal χ2=26.2
bg (ep-scaling=0.92)
bg only fit χ2=48.0
HEAT 94/95/2000
AMS 01
tanβ= 35; m0= 250; m1/2= 550
Wim de Boer ICHEP, Amster dam, July, 2002 2
CMSSM Fitpr ocedure
Choose the 10 GUT super gravityinspired parameter s: ! "$# %& ' # %&( )+*, - ./ 0 132 . / 0 154 . / 0 176 . / 0
Minimiz e the Higgs potential in or-der to determine
'98
Calculate masses and couplings atlow energies by integrating about30 coupled RGE’s and decouplingspar tic les at thresholds
calculate
:<; .= >? @ 0 , A BC BDE
Determine the best parameter s byminimizing F G .
H I JKML J KNPO QSR L J KN B BN Q Q TU TJ V WPXY L X
Z []\^ _ ` ab c de d^Z []\f _ gh i c de dfZ []\kj _ ` h a a a ` c de dj
V lnmV lpoV lrq
Z KN O R stvu tw Q TU TO V EH
Z Kxy Kz V| QSR u G ~ t _ Q TU TkZ KM R t ~ t _ Q TU TZ K N R NP J Q TU T$ y N NP J
Z T KM z y ¡ ¢ ¢£ ¤ ¥ y ¦ N B BN Q
and t G str ongl y correlated. Repeat fits for all pair s of t G
Wim de Boer ICHEP, Amster dam, July, 2002 3
10log Q
1/α i
1/α1
1/α2
1/α3
MSSM
10log Q1/
α i
Unification of the Coupling Constants in the SM and the minimal MSSM
0
10
20
30
40
50
60
0 5 10 150
10
20
30
40
50
60
0 5 10 15
U. Amaldi, W. de Boer, H. Furstenau, PL B260(1991)" "! "¨§ coupling constants of electr omagnetic –, weak–, and str ong interactions© ª "$« ¬ ¯® ° ± !due to radiative corrections (LO)
Wim de Boer ICHEP, Amster dam, July, 2002 4
CMSSM Spar tic le Spectrum
From RGE equations:
0
100
200
300
400
500
600
700
2 4 6 8 10 12 14 16
m1/2
m0
√(µ02+m0
2)
Wino
Bino
GluinoqL~
tL~
tR~
lL~
lR~
m1
m2
tan β = 1.65Yb = Yτ
log10 Q
mas
s [G
eV]
Characteristic MSSM Features:Squarks and gluinos heavy thr oughstr ong rad. corr .Gaugino from U(1) (=Bino) LightestNeutral SUSY Partic le (LSP)(if t G not too large w.r.t. )Mass G in Higgs potential driven negati-ve by
² ¥ >EWSB (determines ( G )
Higgs mixing parameter ( usuall y largecompared with ³t G
Consequentl y:Pseudoscalar Higgs and hig gsinos heavy>light Higgs SM-hig gs-likeLSP bino-like , since no mixing with heavyhig gsinos
>
very good dark mattercandidate
Wim de Boer ICHEP, Amster dam, July, 2002 5
Allo wed Parameter Regions for
´ µ¶
500
1000 500
1000
012345678
500
1000
500 1000
excl
. LS
P
excl. Higgs
excl. bsγm0 · [GeV]
m1/2 [GeV]
χ2 tota
l
m1/
2 [G
eV]
m0 [GeV]
Constraints: Gauge Unification and EWSB¸ free! Fit pref ers¸ ¹
from
= >? @ and ( ¹
from A E >
str ong constraint from
º¼» ¹ ½
(much less for
¸ ¾
!!)
Wim de Boer ICHEP, Amster dam, July, 2002 6
Main Diagrams for Neutralino Annihilation
Gauge Bosons Fermions
¿ À9Á¿ À9Á Â Ã ÄÃÅ
¿ À9Á¿ À9Á ÆÈÇ É Ã ÄÃ Å¿ ÀÊÁ ÃÅ¿ ÄÁ¿ ÀËÁ Ã Ä
¿ ÀÊÁ Ã Å¿ ÄÍÌ¿ ÀËÁ Ã Å
Only heavy final states relevantneutralinos are Majorana par tic les and fermions
>Pauli-Principle at zero momentum>
p-wave
> ¬ fermion mass !)All x-sections str ong function of
Interf erences (Z-,t-channel) NEGATIVEInterf erences (Higgs-,t-c hannel) POSITIVE
Wim de Boer ICHEP, Amster dam, July, 2002 7
p-wave suppression at low momentum for light final states
Î ¬ G at low neutralino momenta
Ï Ð Ï ÐÑ Ò Ó ÒkÔÊÕ Ö Ó ÖÔ
×Ø ÙØ ÚØÛÝÜÞ ß
à Ø Ô áà Ø Ô ×
Øãâ Ø àØâ à
àà Ø
ä åæçè
éêÕ ëÖ
ì í ì í¯î ï ðï
ñò óò ôòõ÷öø ù
ú òû üú òû ñòþý ò úò ý úú
ú òÿ
t G = ( ½ ¸ ¥ ¸z
Wim de Boer ICHEP, Amster dam, July, 2002 8
s,t-c hannel Interf erences
Higgs large, Z small for
= =
final state Higgs small, Z large for
final state
! " #! " %$ !$ !!!
& '() * +-, ++/. 0 1324 45 67 . 0 1324 45 6 8 1:9 ; <
7 . 0 1324 45 6 8= <
> ? > ?@ A BACD E D F DGHI J
K DL MK DL CD%N D KDN KKK D
O PQR S A/T U V3WX XY ZA-[ A]\T U V3WX XY Z ^_ `\T U V3WX XY Z ^ V:a b `
(t-ch, Higgs) Interf . POS , (t-ch, Z) Interf . NEG
>
(
= =
) final states suppressed (enhanced) due to interf erences!
= =
final state dominates at large
t G = ( ½ ¸ ¥ ¸z
Wim de Boer ICHEP, Amster dam, July, 2002 9
Pseudoscalar Higgs exchang e vs
F F > ¸ > = = F F > ¸ >
c dfe c d g h g i j i
kl ml npoq r
s l ts l uv wx
y z |] | ~ ~
p
Fp Fp > ¸ > = =dominates at large
.
Wim de Boer ICHEP, Amster dam, July, 2002 10
Comparison of X-sections in CalcHEP and darkSUSY
¡ ¢
cm
£
s
¤
¦¥ §¨ª© «¬ ¥ ® ¯
GeV© °²± ¥ ³ ³ ®¯ © °µ´ ¥ ³¶ ³¯GeV
«p ¥ ¨ ¯ ¯
GeV© «¸· ¹º ¥ ¨ ¯ ¯
GeV
CalcHEP darkSUSY» ¼ » ®ª½ ³¿¾ ³¯ À ºÁ ®ª½ ¾ ³¯ À º Áà ¼Ã ¯ ½ ®¾ ³¯ À ºÁ ³ ½ ¶ ¾ ³¯ À º ÁÄ Å Ä À §ª½ ®¾ ³¯ À ºÆ ǽ ®¾ ³¯ À º ÆÈ Å È À  ½ ³¿¾ ³¯ À É Â ½ ³¾ ³¯ À É
Feynar ts agrees with CalcHEP concerning
à Ã
!
Wim de Boer ICHEP, Amster dam, July, 2002 11
Neutralino Annihilation X-sections
¥ ³ ½ ¶ ¦¥ § ¨
200400
600800
1000
200400
600800
1000
10-30
10-29
10-28
sigma vTOT
m1/2
Ê [GeV]m 0
Ë [GeV]
<σv>
[cm
3 s-1
GeV
-1]
200400
600800
1000
200400
600800
1000
10-28
10-27
10-26
10-25
sigma vTOT
m1/2
Ê [GeV]m 0
Ë [GeV]
<σv>
[cm
3 s-1
GeV
-1]
Wim de Boer ICHEP, Amster dam, July, 2002 12
Boost factor for AMS and HEAT Data
¥ ³ ½ ¶ ¦¥ § ¨
200400
600800
1000
200400
600800
1000
10 2
10 3
boost-factor (best fit)
m1/2
Ì [GeV]m 0
Í [GeV]
boos
t fa
ctor
200400
600800
1000
200400
600800
1000
10 2
10 3
boost-factor (best fit)
m1/2
Ì [GeV]m 0
Í [GeV]
boos
t fa
ctor
Wim de Boer ICHEP, Amster dam, July, 2002 13
Dark Matter
Î Â Ï ÐÑ Ò Ð Ñ Ó
(from DarkSusy)
¥ ³ ½ ¶ ¦¥ § ¨
200
400
600
800
1000
200 400 600 800 1000
Ωh2-region
excl. Ωh 2 > 0.5
excl
. LSP
m0 [GeV]
m1/
2 [G
eV]
200
400
600
800
1000
200 400 600 800 1000
Ωh2-region
excl. Ωh 2 > 0.5excl. Ωh 2
< 0.1
excl
. LSP
m0 [GeV]
m1/
2 [G
eV]
Green regions pref erred by Boomerang and SN Ia
Wim de Boer ICHEP, Amster dam, July, 2002 14
Typical Fits to AMS+HEAT Data vs
ÔÖÕ ×
10-3
10-2
10-1
1
1 10 102
positron energy [GeV]
e+ /(e+ +
e- ) fr
acti
on
b b–
τ+ τ-
W+ W-
bg+22200• signal χ2=24.2
bg (ep-scaling=0.91)
bg only fit χ2=48.0
HEAT 94/95/2000
AMS 01
tanβ= 1.6; m0= 200; m1/2= 300
10-3
10-2
10-1
1
1 10 102
positron energy [GeV]e+ /(
e+ + e- )
frac
tion
t t–
b b–
τ+ τ-
bg+650•signal χ2=26.2
bg (ep-scaling=0.92)
bg only fit χØ2=48.0
HEAT 94/95/2000
AMS 01
tanβ= 35; m0= 250; m1/2= 550
¥ ³ ½ ¶ «Ù ¥ ³ ¯ ÚÜÛ Ý ¦¥ §¨ «Ù ¥  §¯ Ú Û Ý
Wim de Boer ICHEP, Amster dam, July, 2002 15
Þ Â
contr . for AMS+HEAT Data vs
ÔÖÕ ×
ßàá ¦¥ ³ ½ ¶ ßà á ¦¥ §¨
200400
600800
1000
200400
600800
10000
20
40
χ2 - term
m1/2
Ì [GeV]m 0
Í [GeV]
χ2 - t
erm
200400
600800
1000
200400
600800
10000
20
40
χ2 - term
m1/2
Ì [GeV]m 0
Í [GeV]
χ2 - t
erm
Wim de Boer ICHEP, Amster dam, July, 2002 16
Possib le AMS-02 Data in 2006
one year AMS
10-2
10-1
10-1
1 10 102
positron energy [GeV]
e+ /(e+ +
e- ) fr
acti
on exp. data by DarkSUSY
bgMosk-Strong (e+-scale=0.92)
generated dummy data
tanβ= 35; m0= 300; m1/2= 400
one year AMS
10-2
10-1
10-1
1 10 102
positron energy [GeV]
e+ /(e+ +
e- ) fr
acti
on exp. data by DarkSUSY
bgMosk-Strong (e+-scale=0.92)
generated dummy data
tanβ= 35; m0= 300; m1/2= 800
ßàá ⥠§ ¨ « ãÙ ¥ ³¶ ¯ Ú Û Ý « ãÙ ¥ § ¯ Ú Û Ý
Wim de Boer ICHEP, Amster dam, July, 2002 17
Possib le Þ Â
after one year AMS-02
200400
600800
1000
20040060080010000
20
40
60
80
100
χ2 - term
m1/2 [GeV]
m0
ä [GeV]
χ2 - t
erm
200400
600800
1000
20040060080010000
20
40
60
80
100
χ2 - term
m1/2 [GeV]
m0
ä [GeV]
χ2 - t
erm
Wim de Boer ICHEP, Amster dam, July, 2002 18
Summar y
Low values of (
åçæ è éçê ëì í
) excluded by LEP Higgs Limit of 114 GeV
At larger values of
åçæ è éî î
DOMINANT FINAL STATE
î î
FINAL STATE has orders of magnitude larger x-section thanï ð
final states and also larger thanñ ñ
final states for
åçæ è éçò ó
î î
FINAL STATE fits the AMS+HEAT data as well as the
ï ð
final states
Super symmetr y is an excellent candidate to explain the cold Dark Matterin the univer se. Its signal could be the positr ons and antipr otons fromneutralino annihilation into
î îfinal states
Wim de Boer ICHEP, Amster dam, July, 2002 19
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