Low-energy-density wormholes can be macroscopic in f(Q) gravity only because the free parameter α is chosen small, a result already present in the author's Ref [21].
(1996) Bound states of strings and p-branes
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Wormholes with low energy density
Low-energy-density wormholes can be macroscopic in f(Q) gravity only because the free parameter α is chosen small, a result already present in the author's Ref [21].