22
D-term Dynamical Supersymmetry Breaking K. Fujiwara and, H.I. and M. Sakaguchi arXiv: hep-th/0409060, P. T. P. 113 arXiv: hep-th/0503113, N. P. B 723 H. I., K. Maruyoshi and S. Minato arXiv:0909.5486, Nucl. Phys. B 830 cf. 1 with N. Maru (Keio U.) arXiv:1109.2276 one in preparation I) Introduction breaking of SUSY less frequent compared with that of internal symmetry ble to break SUSY dynamically (DSB) has been popular since mid 80’s, in particular, ontext of instanton generated superpotential k, we will accomplish D term DSB, DDSB, for short e nonrenormalizable D-gaugino-matter fermion and most natural in the context of SUSY gaug ous broken to ala APT-FIS

D-term Dynamical Supersymmetry Breaking

  • Upload
    damita

  • View
    62

  • Download
    0

Embed Size (px)

DESCRIPTION

D-term Dynamical Supersymmetry Breaking. with N. Maru (Keio U.) arXiv:1109.2276 one in preparation. K. Fujiwara and, H.I. and M. Sakaguchi arXiv : hep-th /0409060, P. T. P. 113 arXiv : hep-th /0503113, N. P. B 723 H. I., K. Maruyoshi and S. Minato - PowerPoint PPT Presentation

Citation preview

Page 1: D-term Dynamical Supersymmetry Breaking

D-term Dynamical Supersymmetry BreakingK. Fujiwara and, H.I. and M. SakaguchiarXiv: hep-th/0409060, P. T. P. 113arXiv: hep-th/0503113, N. P. B 723H. I., K. Maruyoshi and S. MinatoarXiv:0909.5486, Nucl. Phys. B 830

cf.

1

with N. Maru (Keio U.)• arXiv:1109.2276 • one in preparation

I) Introduction• spontaneous breaking of SUSY is much less frequent compared with that of internal symmetry • most desirable to break SUSY dynamically (DSB) • F term DSB has been popular since mid 80’s, in particular, in the context of instanton generated superpotential • In this talk, we will accomplish D term DSB, DDSB, for short• based on the nonrenormalizable D-gaugino-matter fermion coupling and most natural in the context of SUSY gauge theory spontaneous broken to ala APT-FIS

Page 2: D-term Dynamical Supersymmetry Breaking

II) Basic idea• Start from a general lagrangian

: a Kähler potential : a gauge kinetic superfield of the chiral superfield in the adjoint representation: a superpotential.

• bilinears:

where .no bosonic counterpart assume is the 2nd derivative of a trace fn.

the gauginos receive masses of mixed Majorana-Dirac type and are split.

: holomorphic and nonvanishing part of the mass

2

Page 3: D-term Dynamical Supersymmetry Breaking

3

• Determination of

stationary condition to

where is the one-loop contribution

and is a counterterm.

In fact, the stationary condition is nothing but the well-known gap equation ofthe theory on-shell which contains four-fermi interactions.

condensation of the Dirac bilinear is responsible for

Page 4: D-term Dynamical Supersymmetry Breaking

The rest of my talk

ContentsI) IntroductionII) Basic ideaIII) Illustration by the Theory with vacuum at tree levelIV) Mass spectrum at tree level and supercurrentV) Self-consistent Hartree Fock approximationVI) Vacuum shift and metastability (qualitative)VII) Our work in the context of MSSMVIII) More on the fermion masses in the H. F. (qualitative)

4

Page 5: D-term Dynamical Supersymmetry Breaking

III) Theory with   vacuum at tree level

• U(N) gauge group assumed for definiteness (product gauge group O.K.)

• : prepotential, input function

• superpotential W supplied by the electric and magnetic FI terms, made possible by a particular fixing of rigid SU(2)R symmetry

• should contrast with

• Later, will work with

Action to work with

5

Page 6: D-term Dynamical Supersymmetry Breaking

Off-shell component lagrangianThe off-shell component lagrangian is

where is the Kähler metric and its derivatives are defined asand .

The gauge part is, in components,

Finally, the superpotential can be written as

6

Page 7: D-term Dynamical Supersymmetry Breaking

Eq of motion for auxiliary fields

While, from the transformation laws,

7

Page 8: D-term Dynamical Supersymmetry Breaking

8

susy of and tree vacua• construction of 2nd susy : Let be

• the form of     and are derived by imposing

• ; vacuum condition

• generic breaking pattern of gauge symmetry:

so that follows from

where

2nd susy broken

Page 9: D-term Dynamical Supersymmetry Breaking

IV) Mass spectrum at tree level and supercurrent

99

a

Page 10: D-term Dynamical Supersymmetry Breaking

10

vacuum condition

Page 11: D-term Dynamical Supersymmetry Breaking

V) Self-consistent Hartree-Fock approximation

11

For simplicity, consider the case U(N) unbroken

Recall we hunt for the possibility (up to one-loop):

no such coupling to bosons present

Mixed Maj.-Dirac mass to gaugino,

DSB

Page 13: D-term Dynamical Supersymmetry Breaking

13

• :

In order to trade A with in Vc.t. ,

impose, for instance,

we obtain

(some number),

Page 18: D-term Dynamical Supersymmetry Breaking

• transmission of DDSB in to the rest of the theory by higher order loop-corrections

the sfermion masses

the gaugino masses of the quadratic Casimir of representation some function of , which is essentially

Fox, Nelson, Weiner, JHEP(2002)

18

Page 19: D-term Dynamical Supersymmetry Breaking

19

• Demanding

We obtain

Page 20: D-term Dynamical Supersymmetry Breaking

20

VIII) More on the fermion masses in the H. F. (qualitative)

• Back to the general theory with 3 input functions

• H. F. can be made into a systematic expansion by an index loop argument.

• Take to be .

• In the unbroken phase,

The gap eq. is

Page 21: D-term Dynamical Supersymmetry Breaking

21

• Two sources beyond tree but leading in H. F.

i) Due to the vacuum shift, as well

ii) For U(1) sector, an index loop circulates

These contribute to the masses in the leading order in the H. F.

+

Page 22: D-term Dynamical Supersymmetry Breaking

22

D-term Dynamical Supersymmetry BreakingK. Fujiwara and, H.I. and M. SakaguchiarXiv: hep-th/0409060, P. T. P. 113arXiv: hep-th/0503113, N. P. B 723H. I., K. Maruyoshi and S. MinatoarXiv:0909.5486, Nucl. Phys. B 830

cf.with N. Maru (Keio U.)• arXiv:1109.2276 • one in preparation

gluino

gluon

𝜓 ′λ ′massive fermion

scalar gluon

-1 -1/2 0 1/2 1

mass

h-1/2 0 1/2

mass

𝑆𝑧

Obserbale (SU(N)) sector