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H.Sung Cheon (천화성, 千和聖) - DESY Theory workshop 2008

H.Sung Cheon (천화성, 千和聖) - DESY Theory workshop 2008

H.Sung Cheon (천화성, 千和聖) - DESY Theory workshop 2008

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In order to guarantee the stability of the dark matter candidates,<br />

1. Z 2 symmetry is conserved<br />

2. Spontaneously symmetry break the EW gauge group<br />

<br />

After the spontaneously EW symmetry breaking, the singlet scalar<br />

dependent part of the scalar potential is given by<br />

V = 1 2 (m2 0 + λv2 EW)φ 2 + λ s<br />

4 φ4 + λv EW φ 2 h + h 2 φ2 h 2

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