Fig. 3.

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Variation of total radius, base of convective zone and effective radius under the fifth-force for uncalibrated solar models. Each observable is normalised with respect to its value at 𝒴 = 0 (no fifth force) at a fixed initial helium abundance (Y0), initial metallicity (Z0) and mixing-length parameter (αMLT). Whereas the fifth force has a significant effect on the radius and position of the convective zone, its effect is milder on the effective temperature.
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