Note on the Evolution of the Gravitational Potential in Rastall Scalar Field Theories
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🌌 astro-ph.CO
gr-qc
keywords
componentevolutionfieldgammagravitationalpotentialrastallscalar
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We investigate the evolution of the gravitational potential in Rastall scalar field theories. In a single component model a consistent perturbation theory, formulated in the newtonian gauge, is possible only for $\gamma = 1$, which is the General Relativity limit. On the other hand, the addition of another canonical fluid component allows also to consider the case $\gamma \neq 1$.
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