- The paper constructs the first inhomogeneous Einstein metrics on complex projective spaces for n=3,4,5,6,7 by reducing the problem to a four-dimensional cohomogeneity-one matching system and rigorously certifying a solution with interval arithmetic and Krawczyk’s theorem.
- The resulting SO(n+1)-invariant metrics are genuinely inhomogeneous, non-Hermitian, not nearly Kähler, and do not have non-negative sectional curvature, while their Yamabe energy is numerically 6.4–22.2% lower than that of the Fubini–Study metric.
- The paper answers Berger’s 1965 question about a second Einstein metric on CP^n, establishes complex dimension 3 as the minimal case, and leaves existence for n≥8 and classification of Hermitian–Einstein metrics as open problems.
The construction of new Einstein metrics on compact manifolds with high symmetry is a long-standing problem in Riemannian geometry. This paper by Cao-Labora and Rodríguez-Vázquez constructs the first inhomogeneous Einstein metrics on complex projective spaces CPn, for n∈{3,4,5,6,7}, answering affirmatively a question posed by Berger in 1965 concerning the existence of a second Einstein metric on CPn. Prior to this work, the only known Einstein metrics on CPn were the homogeneous ones: the Fubini–Study metric and, in odd complex dimension, Ziller's metric obtained via a canonical variation along the twistor fibration over HPn (2608.16880). The new metrics are SOn+1-invariant, of cohomogeneity one, non-Hermitian, and not nearly Kähler; their existence is established by a computer-assisted argument based on interval arithmetic and Krawczyk's fixed-point theorem.
Geometric setup and the cohomogeneity-one action
The construction exploits the standard SOn+1-action on CPn=S2n+1/S1, which descends to a cohomogeneity-one action whose orbit space is an interval. The two singular orbits are a totally geodesic Lagrangian RPn (the fixed-point set of complex conjugation) and the complex quadric Qn−1≅SOn+1/(SO2×SOn−1); principal orbits are diffeomorphic to the unit tangent bundle n∈{3,4,5,6,7}0. The group diagram is n∈{3,4,5,6,7}1.
Any n∈{3,4,5,6,7}2-invariant metric on the regular part takes the diagonal form
n∈{3,4,5,6,7}3
where n∈{3,4,5,6,7}4 is the isotropy decomposition with n∈{3,4,5,6,7}5 and n∈{3,4,5,6,7}6 the standard n∈{3,4,5,6,7}7-module. A key point, established via Dammermann's diagonalization theorem, is that for n∈{3,4,5,6,7}8 every n∈{3,4,5,6,7}9-invariant Einstein metric on CPn0 admits this diagonal form, so the ansatz is exhaustive in that range. Smoothness conditions at the two singular orbits, derived from the general theory of Verdiani–Ziller, impose that the local solution space at each endpoint is two-dimensional — a structural feature that distinguishes this problem from the classical two-function CPn1 ansatz on spheres, where the matching problem is only two-dimensional.
The Einstein equations CPn2 reduce to a system of four ODEs (equations (E1)–(E4)) for CPn3, which are dependent via the Eschenburg–Wang first integral relating CPn4, CPn5, and CPn6 to CPn7. The Fubini–Study metric, with CPn8, CPn9, CPn0 and CPn1, is a solution.
The CPn2-reparametrization and the four-dimensional matching problem
The authors reparametrize the autonomous six-dimensional ODE system using the mean curvature CPn3 of the principal orbits. By the Riccati equation and Cauchy–Schwarz, CPn4, so CPn5 is a strictly monotone function of CPn6 mapping CPn7 onto CPn8, with asymptotics CPn9 near the HPn0 orbit and HPn1 near the quadric. In the scale-invariant variables HPn2, HPn3 and logarithmic derivatives HPn4, the system becomes a four-dimensional non-autonomous ODE in HPn5. A converse proposition reconstructs HPn6 from any solution of this system satisfying sign conditions on HPn7 and on HPn8, so solving the HPn9-system is fully equivalent to solving the Einstein equations.
Each singular orbit admits a two-parameter family of smooth local solutions, encoded in convergent series in SOn+10: near SOn+11 the free parameters are SOn+12; near SOn+13 they are SOn+14 in the symmetric variables adapted to the quadric. Gluing these two families into a global solution requires matching four quantities at the minimal orbit (SOn+15), yielding a four-dimensional matching function SOn+16. The existence of a smooth Einstein metric is thus equivalent to SOn+17 having a zero in a suitable region.
Series expansions and computer-assisted proof
Local solutions at both endpoints are constructed by explicit power series in SOn+18, with recurrences determined by the free parameters. Convergence is proved by propagating Catalan-number bounds on the Taylor coefficients, yielding uniform convergence on half-lines SOn+19 and SOn+10 together with explicit remainder estimates and analytic dependence on the parameters — the latter needed for rigorous derivative bounds via Cauchy estimates.
The zero of SOn+11 is then certified with Krawczyk's fixed-point theorem: if the Krawczyk box SOn+12 is contained in the interior of a small box SOn+13 around an approximate root SOn+14, then SOn+15 has a genuine zero in SOn+16. The interval-arithmetic implementation combines the series enclosures with the CAPD library for rigorous ODE continuation to SOn+17. This is the only computer-assisted step in the paper, and it is structurally different from prior CAP constructions of Einstein metrics on spheres: instead of a Schauder fixed-point argument on an infinite-dimensional Banach space, the computer certifies a zero of a finite-dimensional (four-dimensional) matching map. The authors note this technique should extend to ansätze depending on more functions.
Properties of the new metrics
The resulting metrics have several notable features, each established within the corresponding section of the paper:
- Inhomogeneity: all homogeneous Einstein metrics on SOn+18 (Fubini–Study and, in odd dimension, Ziller's) are geodesic orbit spaces, so their Jacobi operator has constant spectrum along every geodesic. For the new metrics, SOn+19 takes both positive and negative values on CPn=S2n+1/S10, so the Jacobi operator along the normal geodesic has non-constant spectrum, proving inhomogeneity. This argument simultaneously shows the metrics do not have non-negative sectional curvature.
- Non-Hermiticity: an CPn=S2n+1/S11-invariant metric that is Hermitian with respect to the standard complex structure must satisfy CPn=S2n+1/S12 along the geodesic, forcing CPn=S2n+1/S13; the constructed metrics satisfy CPn=S2n+1/S14 since the certified CPn=S2n+1/S15. Hence they are not CPn=S2n+1/S16-Hermitian and, a fortiori, not conformally Kähler.
- Not nearly Kähler: for CPn=S2n+1/S17 this follows from Nagy's classification of strictly nearly Kähler manifolds combined with the known cases of the LeBrun–Salamon conjecture in real dimensions 8, 12, 16; for CPn=S2n+1/S18 it follows by comparing the singular orbit structure with the unique CPn=S2n+1/S19-preserving cohomogeneity-one action.
- Yamabe energy: numerically, the new metrics have smaller Yamabe energy than Fubini–Study, with ratios RPn0 increasing from RPn1 at RPn2 to RPn3 at RPn4, while the corresponding ratios for Ziller's metric decrease with dimension — a monotonicity phenomenon the authors highlight without explanation.
The Main Theorem also settles the minimal dimension: combining the result with Broder's classification of cohomogeneity-one Einstein metrics on closed 4-manifolds, RPn5 (real dimension 6) is the smallest complex dimension admitting an inhomogeneous cohomogeneity-one Einstein metric on RPn6.
Limitations and open questions
The paper is explicit about the scope of its result. The existence proof is confined to RPn7; numerical exploration suggests no RPn8-invariant solutions exist for RPn9, but this is not proved. The cases Qn−1≅SOn+1/(SO2×SOn−1)0 and Qn−1≅SOn+1/(SO2×SOn−1)1 are topologically distinguished — the principal orbits Qn−1≅SOn+1/(SO2×SOn−1)2 are diffeomorphic to Qn−1≅SOn+1/(SO2×SOn−1)3 exactly in these dimensions — and Qn−1≅SOn+1/(SO2×SOn−1)4 is analytically special because the linear system in the recurrence degenerates (Qn−1≅SOn+1/(SO2×SOn−1)5), consistent with Broder's classification. The authors also flag an error in a related preprint (de Araujo–Grajales–Grama) claiming no totally geodesic singular orbits are possible, which is contradicted by both Fubini–Study and the new metrics. Two questions remain open: whether Qn−1≅SOn+1/(SO2×SOn−1)6 admits inhomogeneous Einstein metrics for Qn−1≅SOn+1/(SO2×SOn−1)7 under any symmetry, and whether every Hermitian–Einstein metric on Qn−1≅SOn+1/(SO2×SOn−1)8 with Qn−1≅SOn+1/(SO2×SOn−1)9 is homogeneous.
Conclusion
This paper resolves a sixty-year-old question by producing inhomogeneous Einstein metrics on n∈{3,4,5,6,7}00 for n∈{3,4,5,6,7}01 via a cohomogeneity-one n∈{3,4,5,6,7}02-invariant ansatz. Methodologically, its contribution is a finite-dimensional matching strategy — convergent series with Catalan-type coefficient bounds at the singular orbits, combined with interval-arithmetic ODE continuation and Krawczyk certification — that avoids infinite-dimensional fixed-point arguments and is designed to generalize to ansätze with more than three functions. The metrics themselves are non-Hermitian, not nearly Kähler, lack non-negative sectional curvature, and carry lower Yamabe energy than the homogeneous examples, and their existence in even complex dimension n∈{3,4,5,6,7}03 had no prior analogue.