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Dense enough compact objects were recently shown to lead to an exponentially fast increase of the vacuum energy density for some free scalar fields properly coupled to the spacetime curvature as a consequence of a tachyonic-like instability.
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We note that Eq. (3) in Ref. [ 2 ] contains an incorrect f ( χ ) f(\chi) factor and should read as shown in Eq. ( 38
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The vacuum inside the small box is harder to awaken because its size introduces an “effective mass” of order 1 / ( a L ) 1/(aL) , which would spoil the effect for realistic stars and ξ ∼ 1 \xi\sim 1 . However, since this is a toy model, we can consider | ξ | ≫ 1 |\xi|\gg 1 for the sake of our illustration
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