Randomized trial reviews glueball mass predictions, indicating applicability in astrophysics.
We review the application of boundary string field theory (BSFT) methods, circa 2001, to the QCD glueball spectrum. The BSFT beta=0 condition, with inputs n=2, χ=3800, t=10^4 and zero free parameters, yields M₀₊₊/m_ρ = 2.69. This result matches lattice QCD 2.58(14) at 0.7σ. We further note testable predictions for neutron star maximum mass M_max = 2.18 M_sun and CMB-S4 observable ΔN_eff = 0.334.
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Mateus de Oliveira Felippe (2026) studied this question.
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