Results in Mathematics, cilt.78, sa.6, 2023 (SCI-Expanded)
Given a smooth map φ: M→ N between two Riemannian manifolds (M, g) and (N,〈,〉N) , the φ -scalar curvature of the manifold M, denoted by Sφ , is defined as the trace, with respect to the metric g, of the φ -Ricci tensor, denoted by Ricφ , introduced in [3–5]. In this paper, we focus on the simplest quadratic functional of the φ -scalar curvature Sφ of M and we observe that its Euler-Lagrange equations give rise to a particular Einstein-type structure on M as defined in [3]. With the aid of the latter together with the completeness of g and two more mild assumptions, we are able to conclude that M is φ -scalar flat when it is of at least dimension 5 and infMSφ>-∞ . We point out that this result is new also in the special case that φ is constant, that is, in the usual setting of Riemannian geometry.