The information content of the minimum spanning tree (MST), used to capture higher-order statistics and other information from the cosmic web, is compared to that of the power spectrum for a 𝜈ΛCDM model. The measurements are made in redshift space using haloes from the Quijote simulation of mass ≥ 3.2 × 10 13 ℎ −1 M in a box of length 𝐿 box = 1 ℎ −1 Gpc. The power spectrum multipoles (monopole and quadrupole) are computed for Fourier modes in the range 0.006 < 𝑘 < 0.5 ℎMpc −1 . For comparison the MST is measured with a minimum length scale of 𝑙 min 13 ℎ −1 Mpc. Combining the MST and power spectrum allows for many of the individual degeneracies to be broken; on its own the MST provides tighter constraints on the sum of neutrino masses 𝑀 𝜈 , Hubble constant ℎ, spectral tilt 𝑛 s , and baryon energy density Ω b but the power spectrum alone provides tighter constraints on Ω m and 𝜎 8 . The power spectrum on its own gives a standard deviation of 0.25 eV on 𝑀 𝜈 while the combination of power spectrum and MST gives 0.11 eV. There is similar improvement of a factor of two for ℎ, 𝑛 s , and Ω b . These improvements appear to be driven by the MST's sensitivity to small scale clustering, where the effect of neutrino free-streaming becomes relevant. The MST is shown to be a powerful tool for cosmology and neutrino mass studies, and therefore could play a pivotal role in ongoing and future galaxy redshift surveys (such as DES, DESI, Euclid, and Rubin-LSST).