Abstract
Physics studies Nature, its matter content and its evolution modeled by the laws of physics.
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Notes
- 1.
In fact, it must be included from an effective field theory point of view.
- 2.
One can basically use the mass term, the coupling to matter or the kinetic term of the scalar field in order to achieve screening.
- 3.
The non-linear extension for the spin-1 field is trivial in the sense that one does not have to deal with the Boulware-Deser ghost.
- 4.
Note that we are neglecting the helicity-1 field in \({\upvarphi }^a\) since at linear order this field decouples completely. If we had included the helicity-1 field in the expansion of \({\upvarphi }^\mathrm {a}=(x^{\upalpha }+\mathrm {A}^{\upalpha }-{\uppi }^{\upalpha })\, {\updelta }^\mathrm {a}_{\upalpha }\) then the expression for the covariant tensor would have contained the contribution of that field as well \(\mathrm {H}_{{\upmu }{\upnu }}=\frac{\mathrm {h}_{{\upmu }{\upnu }}}{\mathrm {M}_\mathrm{Pl}}+\partial _{\upmu }\mathrm {A}_{\upnu }+\partial _{\upnu }\mathrm {A}_{\upmu }+\partial _{\upmu }{\uppi }_{\upnu }+ \partial _{\upnu }{\uppi }_{\upmu }+\cdots \).
- 5.
In general, there is also a tadpole contribution \(\mathcal {L}_1\), that depends on the bulk content.
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Heisenberg, L. (2015). Introduction. In: Theoretical and Observational Consistency of Massive Gravity. Springer Theses. Springer, Cham. https://doi.org/10.1007/978-3-319-18935-2_1
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