```
Kadota, Kenji, Kawasaki, Masahiro, Kavli Institute for the Physics and Mathematics of the Universe, and Saikawa, Ken’ichi.
```*Gravitational waves from domain walls in the next-to-minimal supersymmetric standard model*. United States: N. p., 2015.
Web. doi:10.1088/1475-7516/2015/10/041.

```
Kadota, Kenji, Kawasaki, Masahiro, Kavli Institute for the Physics and Mathematics of the Universe, & Saikawa, Ken’ichi.
```*Gravitational waves from domain walls in the next-to-minimal supersymmetric standard model*. United States. doi:10.1088/1475-7516/2015/10/041.

```
Kadota, Kenji, Kawasaki, Masahiro, Kavli Institute for the Physics and Mathematics of the Universe, and Saikawa, Ken’ichi. 2015.
"Gravitational waves from domain walls in the next-to-minimal supersymmetric standard model". United States.
doi:10.1088/1475-7516/2015/10/041.
```

```
@article{osti_22458394,
```

title = {Gravitational waves from domain walls in the next-to-minimal supersymmetric standard model},

author = {Kadota, Kenji and Kawasaki, Masahiro and Kavli Institute for the Physics and Mathematics of the Universe and Saikawa, Ken’ichi},

abstractNote = {The next-to-minimal supersymmetric standard model predicts the formation of domain walls due to the spontaneous breaking of the discrete Z{sub 3}-symmetry at the electroweak phase transition, and they collapse before the epoch of big bang nucleosynthesis if there exists a small bias term in the potential which explicitly breaks the discrete symmetry. Signatures of gravitational waves produced from these unstable domain walls are estimated and their parameter dependence is investigated. It is shown that the amplitude of gravitational waves becomes generically large in the decoupling limit, and that their frequency is low enough to be probed in future pulsar timing observations.},

doi = {10.1088/1475-7516/2015/10/041},

journal = {Journal of Cosmology and Astroparticle Physics},

number = 10,

volume = 2015,

place = {United States},

year = 2015,

month =

}