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Complex, contact, Riemannian, pseudo-Riemannian and Finsler geometry, relativity, gauge theory, global analysis.
5
votes
Accepted
Example of shrinking Ricci soliton
Yes: Take the shrinking Gaussian $(\mathbb{R}^n, dx^2)$ with $X=\rho\nabla\rho$, where $\rho$ denotes the distance to the origin. This space is Ricci flat, so your inequality holds.
4
votes
What are some explicit examples of nontrivial gradient almost Ricci solitons with harmonic c...
The Riemannian product $\mathbb{R}^m \times S^n$ is always of this type, where $\mathbb{R}^m$ is given the flat metric and $S^n$ the round metric of constant sectional curvature one. In this case $\l …
3
votes
The linearization problem of fully nonlinear equation on standard sphere
Here is my favorite way to do this computation.
Let
$$ \delta_{i_1 \dotsm i_k}^{j_1 \dotsm j_k} = \begin{cases} \mathrm{sgn}\, \sigma, & \text{if $j_k = i_{\sigma(k)}$}, \\ 0, & \text{otherwise} \end{ …
7
votes
Nirenberg problem in conformal change
Yes, it is true. This is a consequence of the conformal invariance of the conformal Laplacian.
Let $(M^n,g)$ be a Riemannian manifold. The conformal Laplacian is
$$ L_2^g = -\Delta + \frac{n-2}{4(n- …
2
votes
Kelvin transformation in fully nonlinear equation
This follows easily from the fact that the Kelvin transform is a conformal diffeomorphism and the naturality of the Schouten tensor.
Let $\Phi(z) := \frac{z}{\lvert z\rvert^2}$ denote the Kelvin trans …
2
votes
Accepted
Does any warped product metric admit a function with hessian proportional to the metric?
Yes. (With the caveat that if there is a function such that $\nabla^2\varphi = \psi g$, then necessarily it is a warped product over a one-dimensional base, so your question should really require $\d …
6
votes
Accepted
A closed $(1,1)$-form $\eta$ is harmonic if and only if $\Lambda\eta = \text{constant}$
Let $\eta$ be a closed $(1,1)$-form.
Then $\partial\eta=0$ and $\overline{\partial}\eta=0$.
Recall the Kähler identity
\begin{equation*}
[\partial,\Lambda] = -i\overline{\partial}^\ast .
\end{equatio …
5
votes
Trace and divergence of the Bach tensor
The Bach tensor is only divergence-free in dimension four. In general dimension, it holds that $\nabla^j B_{ij} = (n-4)P^{jk} ( \nabla_i P_{jk} - \nabla_j P_{ik} )$. I pulled this formula from the b …
6
votes
Simplification of integral on the sphere
You can also derive the lemma from the Bochner formula, which in general dimensions can be written
$$ \frac{1}{2}\Delta\lvert\nabla u\rvert^2 = \lvert\nabla^2u\rvert^2 - (\Delta u)^2 + \delta\left((\ …
5
votes
Is the conformal compactification of $M \setminus \{ p \}$ unique?
Theorem 1.4 in C. Frances' preprint "Rigidity at the boundary for conformal structures and other Cartan geometries" asserts that the geodesic compactification is unique (up to conformal diffeomorphism …
3
votes
Einstein warped product manifold Ricci flat
If you also assume that $(N,\ddot g)$ is complete, then your assumptions imply that $(N,\ddot g)$ is Ricci flat. I proved this in my article The nonexistence of quasi-Einstein metrics.
1
vote
Accepted
How to calculate the infimum of Yamabe functional on upper hemisphere
The first observation is that $Q_g(\phi)$ is conformally invariant.
Define
\begin{align*}
L_gu & := -\Delta u + \frac{n-2}{4(n-1)}Ru , \\
B_gu & := \partial_\nu u + \frac{n-2}{2}Hu ,
\end{align*}
wh …
10
votes
Accepted
Definition of the conformal metric
Let $(M,[g])$ be a conformal manifold;
i.e. $(M,g)$ is a Riemannian manifold and $[g] = \{ u^2g \mathrel{}:\mathrel{} u \in C^\infty(M), u>0 \}$ is the set of Riemannian metrics conformal to $g$.
It i …
3
votes
Accepted
Yamabe operator, conformal transformations and square of the Dirac operator
The discrepancy comes from the fact that the square of the Dirac operator is in general not conformally covariant. There are ways to modify powers of the Dirac operator to get a conformally covariant …
4
votes
Accepted
Lee-Parker Yamabe problem proposition 4.6
You are forgetting that, as part of the renormalization, the functions $\psi_s$ all satisfy $\psi_s(-P)=1$ (here $-P$ is the south pole). In particular, since $\psi$ is $C^2$ away from the north pole …