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Gravitational wave interactions in Λ
3
models of dark energy
A. Emir Gumrukcuoglu
,
Kazuya Koyama
Institute of Cosmology & Gravitation
Research output
:
Contribution to journal
›
Article
›
peer-review
39
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3
models of dark energy'. Together they form a unique fingerprint.
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INIS
interactions
100%
nonluminous matter
100%
gravitational waves
100%
scalars
60%
tensors
40%
instability
40%
gravitons
40%
amplitudes
20%
perturbations
20%
decay
20%
strong-coupling model
20%
Physics
Gravitational Wave
100%
Model of Dark Energy
100%
Wave Interaction
100%
Graviton
66%