For f(Q)=Q+αQ² and f(Q)=Q^β, neutron-star solutions that admit power-series expansions at the center or at infinity collapse to General Relativity; genuine beyond-GR effects must be non-analytic.
Zhao, The European Physical Journal C 82, 10.1140/epjc/s10052-022-10266-4 (2022)
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Neutron stars in $f(\mathbb{Q})$ gravity
For f(Q)=Q+αQ² and f(Q)=Q^β, neutron-star solutions that admit power-series expansions at the center or at infinity collapse to General Relativity; genuine beyond-GR effects must be non-analytic.