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Collider Phenomenology of SUSY Cosmic Connections &

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Presentation on theme: "Collider Phenomenology of SUSY Cosmic Connections &"— Presentation transcript:

1 Collider Phenomenology of SUSY Cosmic Connections &
Jin Min Yang Institute of Theoretical Physics, CAS IHEP

2 目 录 1、Introduction to SUSY 2、Fine-tuning & SUSY 3、GUT & SUSY
4、Dark Matter & SUSY 5、 SUSY at Colliders 6、Conclusion

3 1、Introduction 1.1 What is SUSY ? Why SUSY ? SUSY |B |F

4

5 History: At end of 60‘s: SUSY proposed from math logic
At beginning of 70’s: physics model Has been hot for 30 years; papers Why ? SUSY SUSY SUSY

6 Fine Tuning Dark Matter GUT SUSY Inflation Electroweak Baryogenesis Affleck-Dine Baryogenesis

7

8 SUSY is physics? How heavy ? Accessible at LHC? ??? SUSY

9 1.2 SUSY Models R-parity R-parity

10 MSSM NMSSM Singlet S

11 MSSM mSUGRA

12 mSUGRA

13 SUSY breaking mechanisms

14 Fine-tuning GUT Dark Matter TeV-Scale SUSY Split-SUSY
all sparticles < TeV TeV-Scale SUSY 1 < 130 GeV 5 Higgs bosons 4 < TeV Fine-tuning GUT Dark Matter Gauginos/Higgsinos < TeV sparticles Others:superheavy Split-SUSY 1 < 150 GeV Higgs Bosons 4 :superheavy

15 2. Fine-tuning & SUSY 1019 GeV 1015 GeV GUT Fine-tuning 1 TeV
SM break 100 GeV Weak Scale

16 Bare 100 GeV 2

17

18

19 In SUSY: 2 cancel remain How heavy ? Depends on

20 More about Higgs mass: EW baryogenesis:

21 3. GUT & SUSY not sensitive to sfermions light gauginos/higgsino (??)
SM

22

23 GUT sfermions gauginos/higgsino Maybe unaccessible at LHC Light !
Not necessarily so light for LHC

24 4. Dark Matter & SUSY

25 Dark Matter Mass: weak-scale Interaction: weak-scale WIMP

26 Which one is LSP dark matter ?

27 LSP (Dark Matter)

28 mSUGRA

29 Split-SUSY

30 Dark Matter sfermions gauginos/higgsino Maybe heavy
Maybe unaccessible at LHC Dark Matter sfermions gauginos/higgsino Light ! Most likely accessible at LHC

31 5、SUSY Search at Colliders
LEP (I, II) Tevatron I closed Tevatron II on-going LHC up-coming ILC imagining

32 LEP (I, II) SUSY Tevatron (I,II)

33 tan > 2 LEP mh , mA ,mH > 95 GeV 103.5 GeV < chargino
47 GeV < neutralino Selectron > 100 GeV Smuon > 97 GeV 100 GeV < squark Stau > 93 GeV 100 GeV < stop 100 GeV < sbottom

34 Tevatron stop -> b l snu stop -> c chi stop -> c chi

35

36 Future Colliders International Linear Collider (ILC)

37 LHC ILC

38 Find a needle in a haystack!
LHC ILC Find a needle in a haystack! 1/10 billions

39 LHC: discover ILC: precison test

40 LHC: SUSY Typical Signature

41 b-jet b ET b b-jet ET

42 LHC

43 squarks sfermions sleptons Sparticles gauginos gluino Higgsinos
What SUSY partilces can be found at LHC? h, H (CP-even) Higgs Bosons A (CP-odd) H squarks sfermions sleptons Sparticles gauginos Higgsinos gluino charginos neutralinos

44 LHC only see LEP II excluded Depends on good detection capabilities
for b’s and tau’s only see Gold -plated signal LEP II excluded

45 LHC TeV-scale SUSY mSUGRA

46 LHC Dark Matter Constraint

47 ? MSSM sfermion sparticle gaugino higgsino Split SUSY h, H Higgs A, H
many all at least h sfermion several sparticle h, H Higgs gaugino higgsino A, H ? maybe no only h Split SUSY

48 Split-SUSY + pp - 1 1 e+e- + - 1 1

49 LHC Higgs bosons sparticles SM  weak-scale SUSY   ??     ??
h H, A, H   sfermions gaugino/Higgsino SM weak-scale SUSY  ??  ?? Split-SUSY

50 weak-scale SUSY LHC ILC discover Predict dark matter Precision
test Predict dark matter ILC

51 6、Conclusion E. Witten 2002, Beijing

52 Thanks!


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