02.07.2013 Views

Perturbative and non-perturbative infrared behavior of ...

Perturbative and non-perturbative infrared behavior of ...

Perturbative and non-perturbative infrared behavior of ...

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

9.3. Metastable vacua in the conformal window<br />

such that the gauge group is weakly coupled <strong>and</strong> we can rely on the <strong>perturbative</strong> analysis.<br />

The <strong>non</strong> supersymmetric vacuum<br />

The <strong>non</strong> supersymmetric vacuum is located near the origin <strong>of</strong> the field space where the superpotential<br />

(9.3.56) can be studied <strong>perturbative</strong>ly. Appropriate bounds on the parameters ρ <strong>and</strong> µ<br />

allow to neglect the <strong>non</strong> <strong>perturbative</strong> dynamics. We will see that these bounds can be consistent<br />

with the running <strong>of</strong> the coupling constants.<br />

Tree level supersymmetry breaking is possible if<br />

N (1)<br />

f<br />

> Ñ ⇒ 2Ñ > N(2)<br />

f<br />

(9.3.58)<br />

where the second inequality follows from (9.3.57). The equation <strong>of</strong> motion for the field N breaks<br />

supersymmetry through the rank condition mechanism. We solve the other equations <strong>of</strong> motion<br />

<strong>and</strong> we find the <strong>non</strong> supersymmetric vacuum<br />

<br />

µ + σ1<br />

q = ˜q = ( µ + σ2 φ2 ) N =<br />

φ1<br />

p = φ5 ˜p = φ6 L = ( φ7 ˜ <br />

φ8<br />

Y ) K =<br />

Y<br />

<br />

σ3 φ3<br />

φ4 X<br />

<br />

(9.3.59)<br />

where we have also inserted the fluctuations around the minimum, σi <strong>and</strong> φi. The fields X, Y<br />

<strong>and</strong> ˜ Y are pseudo-moduli. The <strong>infrared</strong> superpotential is<br />

WIR = Xφ1φ2 − µ 2 X + µ(φ1φ4 + φ2φ3) + µ(φ5φ8 + φ6φ7)<br />

+ Y φ2φ5 + ˜ Y φ1φ6 + ρφ5φ6<br />

(9.3.60)<br />

In the limit <strong>of</strong> small ρ, this is the same superpotential studied in [128]. This superpotential<br />

corresponds to the one studied in [129] in the R symmetric limit. The fields X, Y <strong>and</strong> ˜ Y are<br />

stabilized by one loop corrections at the origin with positive squared masses.<br />

The supersymmetric vacuum<br />

We derive here the low energy effective action for the field N, <strong>and</strong> we recover the supersymmetric<br />

vacuum in the large field region. The supersymmetric vacuum is characterized by a large expectation<br />

value for N. This vev gives mass to the quarks q <strong>and</strong> ˜q <strong>and</strong> we can integrate them out at<br />

zero vev. Also the quarks p <strong>and</strong> ˜p are massive <strong>and</strong> are integrated out at low energy. The scale <strong>of</strong><br />

the low energy theory ΛL is related to the holomorphic scale ˜Λ via the scale matching relation<br />

Λ 3Ñ<br />

L = ˜ Λ 3Ñ−N(1)<br />

f −N(2)<br />

f detρdet N (9.3.61)<br />

The resulting low energy theory is N = 1 SYM plus a singlet, with effective superpotential<br />

W = −µ 2 N + Ñ(˜ Λ 3Ñ−N(1)<br />

f −N(2)<br />

f detρdet N) 1/Ñ<br />

(9.3.62)<br />

153

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!