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From the Standard Model to String Theory Hans Peter Nilles Physikalisches Institut Universit ¨ at Bonn From the Standard Model to String Theory, Morelia, November 2010 – p. 1/62

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Page 1: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

From the Standard Model toString Theory

Hans Peter Nilles

Physikalisches Institut

Universitat Bonn

From the Standard Model to String Theory, Morelia, November 2010 – p. 1/62

Page 2: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Questions

What can we learn from strings for particle physics?

Can we incorporate particle physics models within theframework of string theory?

From the Standard Model to String Theory, Morelia, November 2010 – p. 2/62

Page 3: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Questions

What can we learn from strings for particle physics?

Can we incorporate particle physics models within theframework of string theory?

Recent progress:

explicit model building towards the MSSM

Heterotic brane worldlocal grand unification

moduli stabilization and Susy breakdown

gaugino condensation and upliftingmirage mediation

From the Standard Model to String Theory, Morelia, November 2010 – p. 2/62

Page 4: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

The road to the Standard Model

What do we want?

gauge group SU(3) × SU(2) × U(1)

3 families of quarks and leptons

scalar Higgs doublet

From the Standard Model to String Theory, Morelia, November 2010 – p. 3/62

Page 5: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

The road to the Standard Model

What do we want?

gauge group SU(3) × SU(2) × U(1)

3 families of quarks and leptons

scalar Higgs doublet

But there might be more:

supersymmetry (SM extended to MSSM)

neutrino masses and mixings

as a hint for a large mass scale around 1016 GeV

From the Standard Model to String Theory, Morelia, November 2010 – p. 3/62

Page 6: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Indirect evidence

Experimental findings suggest the existence of two newscales of physics beyond the standard model

MGUT ∼ 1016GeV and MSUSY ∼ 103GeV:

From the Standard Model to String Theory, Morelia, November 2010 – p. 4/62

Page 7: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Indirect evidence

Experimental findings suggest the existence of two newscales of physics beyond the standard model

MGUT ∼ 1016GeV and MSUSY ∼ 103GeV:

Neutrino-oscillations and “See-Saw Mechanism”

mν ∼ M2W /MGUT

mν ∼ 10−3eV for MW ∼ 100GeV,

From the Standard Model to String Theory, Morelia, November 2010 – p. 4/62

Page 8: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Indirect evidence

Experimental findings suggest the existence of two newscales of physics beyond the standard model

MGUT ∼ 1016GeV and MSUSY ∼ 103GeV:

Neutrino-oscillations and “See-Saw Mechanism”

mν ∼ M2W /MGUT

mν ∼ 10−3eV for MW ∼ 100GeV,

Evolution of coupling constants of the standard modeltowards higher energies.

From the Standard Model to String Theory, Morelia, November 2010 – p. 4/62

Page 9: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

MSSM (supersymmetric)

From the Standard Model to String Theory, Morelia, November 2010 – p. 5/62

Page 10: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Standard Model

From the Standard Model to String Theory, Morelia, November 2010 – p. 6/62

Page 11: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Grand Unification

This leads to SUSY-GUTs with nice things like

unified multiplets (e.g. spinors of SO(10))

gauge coupling unification

Yukawa unification

neutrino see-saw mechanism

From the Standard Model to String Theory, Morelia, November 2010 – p. 7/62

Page 12: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Grand Unification

This leads to SUSY-GUTs with nice things like

unified multiplets (e.g. spinors of SO(10))

gauge coupling unification

Yukawa unification

neutrino see-saw mechanism

But there remain a few difficulties:

breakdown of GUT group (large representations)

doublet-triplet splitting problem (incomplete multiplets)

proton stability (need for R-parity)

From the Standard Model to String Theory, Morelia, November 2010 – p. 7/62

Page 13: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

String Theory

What do we get from string theory?

supersymmetry

extra spatial dimensions

large unified gauge groups

consistent theory of gravity

From the Standard Model to String Theory, Morelia, November 2010 – p. 8/62

Page 14: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

String Theory

What do we get from string theory?

supersymmetry

extra spatial dimensions

large unified gauge groups

consistent theory of gravity

These are the building blocks for a unified theory of all thefundamental interactions.But do they fit together, and if yes how?

We need to understand the mechanism of compactificationof the extra spatial dimensions

From the Standard Model to String Theory, Morelia, November 2010 – p. 8/62

Page 15: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Calabi Yau Manifold

From the Standard Model to String Theory, Morelia, November 2010 – p. 9/62

Page 16: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Orbifold

From the Standard Model to String Theory, Morelia, November 2010 – p. 10/62

Page 17: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Where do we live?

From the Standard Model to String Theory, Morelia, November 2010 – p. 11/62

Page 18: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Localization

Quarks, Leptons and Higgs fields can be localized:

in the Bulk (d = 10 untwisted sector)

on 3-Branes (d = 4 twisted sector fixed points)

on 5-Branes (d = 6 twisted sector fixed tori)

From the Standard Model to String Theory, Morelia, November 2010 – p. 12/62

Page 19: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Localization

Quarks, Leptons and Higgs fields can be localized:

in the Bulk (d = 10 untwisted sector)

on 3-Branes (d = 4 twisted sector fixed points)

on 5-Branes (d = 6 twisted sector fixed tori)

but there is also a “localization” of gauge fields

E8 × E8 in the bulk

smaller gauge groups on various branes

Observed 4-dimensional gauge group is common subroupof the various localized gauge groups!

From the Standard Model to String Theory, Morelia, November 2010 – p. 12/62

Page 20: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Localized gauge symmetries

SU(6)×SU(2)

SU(6)×SU(2)

SO(10)

SU(4)2

(Förste, HPN, Vaudrevange, Wingerter, 2004)From the Standard Model to String Theory, Morelia, November 2010 – p. 13/62

Page 21: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Standard Model Gauge Group

SU(6)×SU(2)

SU(6)×SU(2)SU

(3) 2

SU(5)

SU(4)×SU(2)2

SO(10)

SU(4)2

SU

(4)×

SU

(2)2

SU(5)S

U(3) 2

(Förste, HPN, Vaudrevange, Wingerter, 2004)From the Standard Model to String Theory, Morelia, November 2010 – p. 14/62

Page 22: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Local Grand Unification

In fact string theory gives us a variant of GUTs

complete multiplets for fermion families

split multiplets for gauge- and Higgs-bosons

partial Yukawa unification

From the Standard Model to String Theory, Morelia, November 2010 – p. 15/62

Page 23: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Local Grand Unification

In fact string theory gives us a variant of GUTs

complete multiplets for fermion families

split multiplets for gauge- and Higgs-bosons

partial Yukawa unification

Key properties of the theory depend on the geography ofthe fields in extra dimensions.

This geometrical set-up called local GUTs, can berealized in the framework of the “heterotic braneworld”.(Förste, HPN, Vaudrevange, Wingerter, 2004; Buchmüller, Hamaguchi, Lebedev, Ratz, 2004)

From the Standard Model to String Theory, Morelia, November 2010 – p. 15/62

Page 24: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

The “fertile patch”: Z6 II orbifold

(Kobayashi, Raby, Zhang, 2004; Buchmüller, Hamaguchi, Lebedev, Ratz, 2004)

provides fixed points and fixed tori

allows SO(10) gauge group

allows for localized 16-plets for 2 families

SO(10) broken via Wilson lines

nontrivial hidden sector gauge group

From the Standard Model to String Theory, Morelia, November 2010 – p. 16/62

Page 25: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Selection Strategy

criterion V SO(10),1 V SO(10),2

➁ models with 2 Wilson lines 22, 000 7, 800

➂ SM gauge group ⊂ SO(10) 3563 1163

➃ 3 net families 1170 492

➄ gauge coupling unification 528 234

➅ no chiral exotics 128 90

(Lebedev, HPN, Raby, Ramos-Sanchez, Ratz, Vaudrevange, Wingerter, 2006)

From the Standard Model to String Theory, Morelia, November 2010 – p. 17/62

Page 26: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

The road to the MSSM

This scenario leads to

200 models with the exact spectrum of the MSSM(absence of chiral exotics)

local grand unification (by construction)

gauge- and (partial) Yukawa unification(Raby, Wingerter, 2007)

examples of neutrino see-saw mechanism(Buchmüller, Hamguchi, Lebedev, Ramos-Sanchez, Ratz, 2007)

models with matter-parity + solution to the µ-problem(Lebedev, HPN, Raby, Ramos-Sanchez, Ratz, Vaudrevange, Wingerter, 2007)

gaugino condensation and mirage mediation(Löwen, HPN, 2008)

From the Standard Model to String Theory, Morelia, November 2010 – p. 18/62

Page 27: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

A Benchmark Model

At the orbifold point the gauge group is

SU(3) × SU(2) × U(1)9 × SU(4) × SU(2)

one U(1) is anomalous

there are singlets and vectorlike exotics

decoupling of exotics and breakdown of gauge grouphas been verified

remaining gauge group

SU(3) × SU(2) × U(1)Y × SU(4)hidden

for discussion of neutrinos and R-parity we keep alsothe U(1)B−L charges

From the Standard Model to String Theory, Morelia, November 2010 – p. 19/62

Page 28: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Spectrum

# irrep label # irrep label

3 (3,2;1,1)(1/6,1/3) qi 3`

3,1;1,1´

(−2/3,−1/3)ui

3 (1,1;1,1)(1,1) ei 8 (1,2;1,1)(0,∗) mi

3 + 1`

3,1;1,1´

(1/3,−1/3)di 1 (3,1;1,1)(−1/3,1/3) di

3 + 1 (1,2;1,1)(−1/2,−1) ℓi 1 (1,2;1,1)(1/2,1) ℓi

1 (1,2;1,1)(−1/2,0) hd 1 (1,2;1,1)(1/2,0) hu

6`

3,1;1,1´

(1/3,2/3)δi 6 (3,1;1,1)(−1/3,−2/3) δi

14 (1,1;1,1)(1/2,∗) s+i 14 (1,1;1,1)(−1/2,∗) s−i

16 (1,1;1,1)(0,1) ni 13 (1,1;1,1)(0,−1) ni

5 (1,1;1,2)(0,1) ηi 5 (1,1;1,2)(0,−1) ηi

10 (1,1;1,2)(0,0) hi 2 (1,2;1,2)(0,0) yi

6 (1,1;4,1)(0,∗) fi 6`

1,1;4,1´

(0,∗)fi

2 (1,1;4,1)(−1/2,−1) f−

i 2`

1,1;4,1´

(1/2,1)f+

i

4 (1,1;1,1)(0,±2) χi 32 (1,1;1,1)(0,0) s0i

2`

3,1;1,1´

(−1/6,2/3)vi 2 (3,1;1,1)(1/6,−2/3) vi

From the Standard Model to String Theory, Morelia, November 2010 – p. 20/62

Page 29: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Unification

Higgs doublets are inuntwisted (U3) sector

heavy top quark

µ−term protected by adiscrete symmetry

3 4 5 6 7 8 9 10 11 12 13 14 15 16 17log10 HΜGeVL

0.02

0.03

0.04

0.05

0.06

0.07

0.08

0.09

Αi

Α3

Α2

Α1

Αt

threshold corrections (“on third torus”) allow unificationat correct scale around 1016 GeV

natural incorporation of gauge-Yukawa unification(Faraggi, 1991; Hosteins, Kappl, Ratz, Schmidt-Hoberg, 2009)

From the Standard Model to String Theory, Morelia, November 2010 – p. 21/62

Page 30: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

See-saw neutrino masses

The see-saw mechanism requires

right handed neutrinos (Y = 0 and B − L = ±1),

heavy Majorana neutrino masses MMajorana,

Dirac neutrino masses MDirac.

The benchmark model has 49 right handed neutrinos:

the left handed neutrino mass is mν ∼ M2Dirac/Meff

with Meff < MMajorana and depends on the number ofright handed neutrinos.

(Buchmüller, Hamguchi, Lebedev, Ramos-Sanchez, Ratz, 2007;

Lebedev, HPN, Raby, Ramos-Sanchez, Ratz, Vaudrevange, Wingerter, 2007)

From the Standard Model to String Theory, Morelia, November 2010 – p. 22/62

Page 31: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Spectrum

# irrep label # irrep label

3 (3,2;1,1)(1/6,1/3) qi 3`

3,1;1,1´

(−2/3,−1/3)ui

3 (1,1;1,1)(1,1) ei 8 (1,2;1,1)(0,∗) mi

3 + 1`

3,1;1,1´

(1/3,−1/3)di 1 (3,1;1,1)(−1/3,1/3) di

3 + 1 (1,2;1,1)(−1/2,−1) ℓi 1 (1,2;1,1)(1/2,1) ℓi

1 (1,2;1,1)(−1/2,0) hd 1 (1,2;1,1)(1/2,0) hu

6`

3,1;1,1´

(1/3,2/3)δi 6 (3,1;1,1)(−1/3,−2/3) δi

14 (1,1;1,1)(1/2,∗) s+i 14 (1,1;1,1)(−1/2,∗) s−i

16 (1,1;1,1)(0,1) ni 13 (1,1;1,1)(0,−1) ni

5 (1,1;1,2)(0,1) ηi 5 (1,1;1,2)(0,−1) ηi

10 (1,1;1,2)(0,0) hi 2 (1,2;1,2)(0,0) yi

6 (1,1;4,1)(0,∗) fi 6`

1,1;4,1´

(0,∗)fi

2 (1,1;4,1)(−1/2,−1) f−

i 2`

1,1;4,1´

(1/2,1)f+

i

4 (1,1;1,1)(0,±2) χi 32 (1,1;1,1)(0,0) s0i

2`

3,1;1,1´

(−1/6,2/3)vi 2 (3,1;1,1)(1/6,−2/3) vi

From the Standard Model to String Theory, Morelia, November 2010 – p. 23/62

Page 32: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Matter-Parity

matter-parity allows the distinction between Higgsbosons and sleptons

SO(10) contains matter-parity as a discrete subgroup ofU(1)B−L.

in conventional “field theory GUTs” one needs largerepresentations to break U(1)B−L (≥ 126 dimensional)

in heterotic string models one has more candidates formatter-parity (and generalizations thereof)

one just needs singlets with an even B − L charge thatbreak U(1)B−L down to matter-parity

(Lebedev, HPN, Raby, Ramos-Sanchez, Ratz, Vaudrevange, Wingerter, 2007)

From the Standard Model to String Theory, Morelia, November 2010 – p. 24/62

Page 33: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Discrete Symmetries

There are numerous discrete symmetries:

from geometry

and stringy selection rules,

both of abelian and nonabelian nature(Kobayashi, HPN, Plöger, Raby, Ratz, 2006)

The importance of these discrete symmetries cannot beunderestimated. After all, besides the gauge symmetriesthis is what we get in string theory.

At low energies the discrete symmetries might appear asaccidental continuous global U(1) symmetries.

From the Standard Model to String Theory, Morelia, November 2010 – p. 25/62

Page 34: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Accidental Symmetries

Applications of discrete and accidental global symmetries:

(nonabelian) family symmetries (and FCNC)(Ko, Kobayashi, Park, Raby, 2007)

Yukawa textures (via Frogatt-Nielsen mechanism)

a solution to the µ-problem(Lebedev, HPN, Raby, Ramos-Sanchez, Ratz, Vaudrevange, Wingerter, 2007)

creation of hierarchies(Kappl, HPN, Ramos-Sanchez, Ratz, Schmidt-Hoberg, Vaudrevange, 2008)

proton stability via “Proton Hexality”(Dreiner, Luhn, Thormeier, 2005; Förste, HPN, Ramos-Sanchez, Vaudrevange, 2010)

approximate global U(1) for a QCD accion(Choi, Kim, Kim, 2006; Choi, HPN, Ramos-Sanchez, Vaudrevange, 2008)

From the Standard Model to String Theory, Morelia, November 2010 – p. 26/62

Page 35: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Gaugino Condensation

2 4 6 8 10 12 14 16log10 HLGeVL

0

5

10

15

20

25

#of

mod

els

Gravitino mass m3/2 = Λ3/M2Planck and Λ ∼ exp(−S)

We need to fix the dilaton!

(Lebedev, HPN, Raby, Ramos-Sanchez, Ratz, Vaudrevange, Wingerter, 2006)

From the Standard Model to String Theory, Morelia, November 2010 – p. 27/62

Page 36: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Run-away potential

2.1 2.2 2.3 2.4

0

0.5

1

1.5

2

Re S

V

10-

32

N = 4 A = 4.9 d = 0 p = 0 b = 0

From the Standard Model to String Theory, Morelia, November 2010 – p. 28/62

Page 37: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Basic Questions

origin of the small scale?

stabilization of moduli?

From the Standard Model to String Theory, Morelia, November 2010 – p. 29/62

Page 38: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Basic Questions

origin of the small scale?

stabilization of moduli?

Recent progress in

moduli stabilization via fluxes in warpedcompactifications of Type IIB string theory

(Dasgupta, Rajesh, Sethi, 1999; Giddings, Kachru, Polchinski, 2001)

generalized flux compactifications ofheterotic string theory

(Gurrieri, Lukas, Micu, 2004; Parameswaran, Ramos-Sanchez, Zavala, 2010)

combined with gaugino condensates and “uplifting”(Kachru, Kallosh, Linde, Trivedi, 2003; Löwen, HPN, 2008)

From the Standard Model to String Theory, Morelia, November 2010 – p. 29/62

Page 39: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Run-away potential

2.1 2.2 2.3 2.4

0

0.5

1

1.5

2

Re S

V

10-

32

N = 4 A = 4.9 d = 0 p = 0 b = 0

From the Standard Model to String Theory, Morelia, November 2010 – p. 30/62

Page 40: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Corrections to Kähler potential

2.1 2.2 2.3 2.4

0

0.5

1

1.5

2

Re S

V

10-

28

N = 4 A = 4.9 d = 5.7391 p = 1.1 b = 1

(Barreiro, de Carlos, Copeland, 1998)

From the Standard Model to String Theory, Morelia, November 2010 – p. 31/62

Page 41: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Sequestered sector “uplifting”

1.5 2 2.5 3 3.5 4 4.5

0

1

2

3

4

5

6

Re S

V

10-

30

N = 4 A = 4.9 C0 = 0.73

(Lebedev, HPN, Ratz, 2006; Löwen, HPN, 2008)

From the Standard Model to String Theory, Morelia, November 2010 – p. 32/62

Page 42: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Downlift

(Löwen, HPN, 2008)

From the Standard Model to String Theory, Morelia, November 2010 – p. 33/62

Page 43: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Fluxes and gaugino condensation

Is there a general pattern of the soft mass terms?

We always have (from flux and gaugino condensate)

W = something − exp(−X)

where “something” is small and X is moderately large.

From the Standard Model to String Theory, Morelia, November 2010 – p. 34/62

Page 44: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Fluxes and gaugino condensation

Is there a general pattern of the soft mass terms?

We always have (from flux and gaugino condensate)

W = something − exp(−X)

where “something” is small and X is moderately large.

In fact in this simple scheme

X ∼ log(MPlanck/m3/2)

providing a “little” hierarchy.(Choi, Falkowski, HPN, Olechowski, Pokorski, 2004)

From the Standard Model to String Theory, Morelia, November 2010 – p. 34/62

Page 45: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Mixed Mediation Schemes

The contribution from “Modulus Mediation” is thereforesuppressed by the factor

X ∼ log(MPlanck/m3/2) ∼ 4π2.

From the Standard Model to String Theory, Morelia, November 2010 – p. 35/62

Page 46: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Mixed Mediation Schemes

The contribution from “Modulus Mediation” is thereforesuppressed by the factor

X ∼ log(MPlanck/m3/2) ∼ 4π2.

Thus the contribution due to radiative corrections becomescompetitive, leading to mixed mediation schemes.

The simplest case for radiative corrections leads toanomaly mediation competing now with the suppressedcontribution of modulus mediation.

For reasons that will be explained later we call this scheme

MIRAGE MEDIATION(Loaiza, Martin, HPN, Ratz, 2005)

From the Standard Model to String Theory, Morelia, November 2010 – p. 35/62

Page 47: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

The little hierarchy

mX ∼ 〈X〉m3/2 ∼ 〈X〉2msoft

is a generic signal of such a scheme

moduli and gravitino are heavy

gaugino mass spectrum is compressed(Choi, Falkowski, HPN, Olechowski, 2005; Endo, Yamaguchi, Yoshioka, 2005;

Choi, Jeong, Okumura, 2005)

such a situation occurs if SUSY breaking is e.g.“sequestered” on a warped throat

(Kachru, McAllister, Sundrum, 2007)

From the Standard Model to String Theory, Morelia, November 2010 – p. 36/62

Page 48: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Mirage Unification

Mirage Mediation provides a

characteristic pattern of soft breaking terms.

To see this, let us consider the gaugino masses

M1/2 = Mmodulus + Manomaly

as a sum of two contributions of comparable size.

Manomaly is proportional to the β function,i.e. negative for the gluino, positive for the bino

thus Manomaly is non-universal below the GUT scale

From the Standard Model to String Theory, Morelia, November 2010 – p. 37/62

Page 49: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Evolution of couplings

3 4 5 6 7 8 9 10 11 12 13 14 15 16 17log10 HΜGeVL

0.02

0.03

0.04

0.05

0.06

0.07

0.08

0.09Α

i

From the Standard Model to String Theory, Morelia, November 2010 – p. 38/62

Page 50: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

The Mirage Scale

3 4 5 6 7 8 9 10 11 12 13 14 15 16 17log10 HΜGeVL

600

800

1000

1200

1400

1600

Mi

GeV

M3

M2

M1

(Lebedev, HPN, Ratz, 2005)

From the Standard Model to String Theory, Morelia, November 2010 – p. 39/62

Page 51: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

The Mirage Scale (II)

The gaugino masses coincide

above the GUT scale

at the mirage scale µmirage = MGUT exp(−8π2/ρ)

where ρ denotes the “ratio” of the contribution of modulusvs. anomaly mediation. We write the gaugino masses as

Ma = Ms(ρ + bag2a) =

m3/2

16π2(ρ + bag

2a)

and ρ → 0 corresponds to pure anomaly mediation.

From the Standard Model to String Theory, Morelia, November 2010 – p. 40/62

Page 52: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

The Mirage Scale (III)

The gaugino masses coincide

above the GUT scale

at the mirage scale µmirage = MGUT exp(−8π2/ρ)

There is a different notation used in the literature using aparameter α where

the mirage scale is µmirage = MGUT

(

m3/2

MPlanck

)α/2

α → 0 corresponds to pure gravity mediation

and α log(

m3/2

MPlanck

)

∼ 1/ρ

From the Standard Model to String Theory, Morelia, November 2010 – p. 41/62

Page 53: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Some important messages

Please keep in mind:

the uplifting mechanism plays an important role for thepattern of the soft susy breaking terms

predictions for gaugino masses are more robust thanthose for sfermion masses

dilaton/modulus mediation suppressed in many cases

mirage pattern for gaugino masses rather generic

From the Standard Model to String Theory, Morelia, November 2010 – p. 42/62

Page 54: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

The string signatures

We might consider the following schemes:

Type II string theory

Heterotic string theory

M-theory on manifolds with G2 holonomy

F-theory

From the Standard Model to String Theory, Morelia, November 2010 – p. 43/62

Page 55: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

The string signatures

We might consider the following schemes:

Type II string theory

Heterotic string theory

M-theory on manifolds with G2 holonomy

F-theory

Questions:

are there distinct signatures for the various schemes?

can they be identified with LHC data?(Choi, HPN, 2007)

From the Standard Model to String Theory, Morelia, November 2010 – p. 43/62

Page 56: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

What to expect from the LHC

At the LHC we scatter

protons on protons, i.e.

quarks on quarks and/or

gluons on gluons

Thus LHC will be a machine to produce strongly interactingparticles. If TeV-scale susy is the physics beyond thestandard model we might expect LHC to become a

GLUINO FACTORY

with cascade decays down to the LSP neutralino.

From the Standard Model to String Theory, Morelia, November 2010 – p. 44/62

Page 57: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

The Gaugino Code

First step to test these ideas at the LHC:

look for pattern of gaugino masses

Let us assume the

low energy particle content of the MSSM

measured values of gauge coupling constants

g21 : g2

2 : g23 ≃ 1 : 2 : 6

The evolution of gauge couplings would then lead tounification at a GUT-scale around 1016 GeV

From the Standard Model to String Theory, Morelia, November 2010 – p. 45/62

Page 58: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Formulae for gaugino masses

(

Ma

g2a

)

TeV

= M(0)a + M

(1)a |loop + M

(1)a |gauge + M

(1)a |string

M(0)a =

1

2F I∂If

(0)a

M(1)a |loop =

1

16π2ba

FC

C−

1

8π2

m

Cma F I∂I ln(e−K0/3Zm)

M(1)a |string =

1

8π2F I∂IΩa

From the Standard Model to String Theory, Morelia, November 2010 – p. 46/62

Page 59: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

The Gaugino Code

Observe that

evolution of gaugino masses is tied to evolution ofgauge couplings

for MSSM Ma/g2a does not run (at one loop)

This implies

robust prediction for gaugino masses

gaugino mass relations are the key to reveal theunderlying scheme

3 CHARACTERISTIC MASS PATTERNS(Choi, HPN, 2007)

From the Standard Model to String Theory, Morelia, November 2010 – p. 47/62

Page 60: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

SUGRA Pattern

Universal gaugino mass at the GUT scale

SUGRA pattern:M1 : M2 : M3 ≃ 1 : 2 : 6 ≃ g2

1 : g22 : g2

3

as realized in popular schemes such asgravity-, modulus- and gaugino-mediation

This leads to

LSP χ01 predominantly Bino

G = Mgluino/mχ01≃ 6

as a characteristic signature of these schemes.

From the Standard Model to String Theory, Morelia, November 2010 – p. 48/62

Page 61: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Anomaly Pattern

Gaugino masses below the GUT scale determinedby the β functions

anomaly pattern:M1 : M2 : M3 ≃ 3.3 : 1 : 9

at the TeV scale as the signal of anomaly mediation.

For the gauginos, this implies

LSP χ01 predominantly Wino

G = Mgluino/mχ01≃ 9

Pure anomaly mediation inconsistent, as sfermion massesare problematic in this scheme (tachyonic sleptons).

From the Standard Model to String Theory, Morelia, November 2010 – p. 49/62

Page 62: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Mirage Pattern

Mixed boundary conditions at the GUT scalecharacterized by the parameter ρ(the ratio of anomaly to modulus mediation).

M1 : M2 : M3 ≃ 1 : 1.3 : 2.5 for ρ ≃ 5

M1 : M2 : M3 ≃ 1 : 1 : 1 for ρ ≃ 2

The mirage scheme leads to

LSP χ01 predominantly Bino

G = Mgluino/mχ01

< 6

a “compact” gaugino mass pattern.

From the Standard Model to String Theory, Morelia, November 2010 – p. 50/62

Page 63: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

The Mirage Scale (III)

The gaugino masses coincide

above the GUT scale

at the mirage scale µmirage = MGUT exp(−8π2/ρ)

There is a different notation used in the literature using aparameter α where

the mirage scale is µmirage = MGUT

(

m3/2

MPlanck

)α/2

α → 0 corresponds to pure gravity mediation

and α log(

m3/2

MPlanck

)

∼ 1/ρ

From the Standard Model to String Theory, Morelia, November 2010 – p. 51/62

Page 64: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

The Gaugino Code

Mixed boundary conditions at the GUT scalecharacterized by the parameter α:the ratio of modulus to anomaly mediation.

M1 : M2 : M3 ≃ 1 : 2 : 6 for α ≃ 0

M1 : M2 : M3 ≃ 1 : 1.3 : 2.5 for α ≃ 1

M1 : M2 : M3 ≃ 1 : 1 : 1 for α ≃ 2

M1 : M2 : M3 ≃ 3.3 : 1 : 9 for α ≃ ∞

The mirage scheme leads to

LSP χ01 predominantly Bino

a “compact” gaugino mass pattern.(Choi, HPN, 2007; Löwen, HPN, 2009)

From the Standard Model to String Theory, Morelia, November 2010 – p. 52/62

Page 65: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Gaugino Masses

0 1 2 3 5 10 ¥

-3

-2

-1

0

1

2

3

Α

MaÈM

0ÈH

1+Α

2L12

M1

M2

M3

Mod

ulus­

Anom

aly­

From the Standard Model to String Theory, Morelia, November 2010 – p. 53/62

Page 66: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Scalar Masses

0 1 2 3 5 10 ¥

-0.5

0

0.5

1

1.5

Α

mi2ÈM

02H1+Α

2L

qL

eR

LM

odul

us­

Anom

aly­

From the Standard Model to String Theory, Morelia, November 2010 – p. 54/62

Page 67: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Scalar Masses

0 1 2 3 5 10 ¥

-0.1

0

0.1

0.2

0.3

0.4

0.5

0.6

0.7

Α

mi2ÈM

02H1+Α

2L

qL

eR

L

Mod

ulusw

Anom

alyw

From the Standard Model to String Theory, Morelia, November 2010 – p. 55/62

Page 68: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Constraints onα

0 0.25 0.5 0.75 1 1.25 1.5 1.75 2

0

10

20

30

40

50

60

Α

m3

2@T

eVD

tan Β = 30 Ξ = 13 Φ = 0

TACHYONS

tLS

PBelow LEP

W > WWMAP

From the Standard Model to String Theory, Morelia, November 2010 – p. 56/62

Page 69: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Constraints onα (modified mirage)

an Β 30 Ηi t 3

0 1 2 3 4 5 6 7 8

0

10

20

30

40

50

60

3

2T

eVm

Α

g

LSP

No EWSB

Χ + LSP

BelowLEP BelowLEP

tLS

PΧ+

LSP

From the Standard Model to String Theory, Morelia, November 2010 – p. 57/62

Page 70: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Various string schemes

Type IIB with matter on D7 branes:mirage mediation (Choi, Falkowski, HPN, Olechowski, 2005)

Type IIB with matter on D3 branes:anomaly mediation? (Choi, Falkowski, HPN, Olechowski, 2005)

Heterotic string with dilaton domination:mirage mediation (Löwen, HPN, 2008)

Heterotic string with modulus domination:string thresholds might spoil anomaly pattern

(Derendinger, Ibanez, HPN, 1986)

M theory on “G2 manifold”:Kähler corrections might spoil mirage pattern

(Acharya, Bobkov, Kane, Kumar, Shao, 2007)

From the Standard Model to String Theory, Morelia, November 2010 – p. 58/62

Page 71: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Keep in mind

In the calculation of the soft masses we get the most robustpredictions for gaugino masses

Modulus Mediation: (fWW with f = f(Moduli))

If this is supressed we might have loop contributions, e.g.

Anomaly Mediation as simplest example

From the Standard Model to String Theory, Morelia, November 2010 – p. 59/62

Page 72: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Keep in mind

In the calculation of the soft masses we get the most robustpredictions for gaugino masses

Modulus Mediation: (fWW with f = f(Moduli))

If this is supressed we might have loop contributions, e.g.

Anomaly Mediation as simplest example

How much can it be suppressed?

log(m3/2/MPlanck)

So we might expect

a mixture of tree level and loop contributions.

From the Standard Model to String Theory, Morelia, November 2010 – p. 59/62

Page 73: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Conclusion

Gaugino masses can serve as a promising tool for an earlytest for supersymmetry at the LHC

Rather robust predictions

3 basic and simple patterns(Sugra, anomaly, mirage)

Mirage pattern rather generic

With some luck we might find such a simple scheme at theLHC and measure the ratio G = Mgluino/mχ0

1!

Let us hope for a bright future of SUSY at the LHC.

From the Standard Model to String Theory, Morelia, November 2010 – p. 60/62

Page 74: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Conclusion

String theory provides us with new ideas for particle physicsmodel building, leading to concepts such as

MSSM via Local Grand Unification

Accidental symmetries (of discrete origin)

Geography of extra dimensions plays a crucial role:

localization of fields on branes,

sequestered sectors and mirage mediation

We seem to live at a special place in the extra dimensions!

The LHC might clarify the case for (local) grand unification.

From the Standard Model to String Theory, Morelia, November 2010 – p. 61/62

Page 75: From the Standard Model to String Theoryscales of physics beyond the standard model M ... What do we get from string theory? supersymmetry extra spatial dimensions large unified gauge

Where do we live?

From the Standard Model to String Theory, Morelia, November 2010 – p. 62/62