In Riemannian geometry, Gromov's optimal stable 2-systolic inequality is the inequality
                                          s            t            s            y            s                                2                                                                    n                          ≤        n        !                                      v            o            l                                2            n                          (                              C            P                                n                          )                ,
valid for an arbitrary Riemannian metric on the complex projective space, where the optimal bound is attained by the symmetric Fubini–Study metric, providing a natural geometrisation of quantum mechanics. Here                               s          t          s          y                      s                          2                                               is the stable 2-systole, which in this case can be defined as the infimum of the areas of rational 2-cycles representing the class of the complex projective line                                           C            P                                1                          ⊂                              C            P                                n                                   in 2-dimensional homology.
The inequality first appeared in Gromov (1981) as Theorem 4.36.
The proof of Gromov's inequality relies on the Wirtinger inequality for exterior 2-forms.
In the special case n=2, Gromov's inequality becomes                                           s            t            s            y            s                                2                                                                    2                          ≤        2                              v            o            l                                4                          (                              C            P                                2                          )                . This inequality can be thought of as an analog of Pu's inequality for the real projective plane                                           R            P                                2                                  . In both cases, the boundary case of equality is attained by the symmetric metric of the projective plane. Meanwhile, in the quaternionic case, the symmetric metric on                                           H            P                                2                                   is not its systolically optimal metric. In other words, the manifold                                           H            P                                2                                   admits Riemannian metrics with higher systolic ratio                                           s            t            s            y            s                                4                                                                    2                                    /                                      v            o            l                                8                                   than for its symmetric metric (Bangert et al. 2009).