Abstract
In this note, we study a geometric property of asymptotically Minkowski spacetimes and an analytic property of the wave operator. More precisely, our first main results show that asymptotically Minkowski spacetimes are geodesically complete under a null non-trap** condition. Secondly, we prove that Sobolev index of a real principal type estimate used in a previous work is optimal.
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A short proof of smoothing effects on the Minkowski spacetimes
A short proof of smoothing effects on the Minkowski spacetimes
In this appendix, we give a short proof of (1.1) and (1.2) using the explicit formula (3.2).
Lemma A.1
Set
Then, for \(\varepsilon >0\) we have
Proof
The second inequality immediately follows from Hölder’s inequality. Thus, we shall show the first inequality. We write \({\hat{f}}(t,\eta )={\mathcal {F}}_{y\rightarrow \eta }f(t,\eta )\) and \(a_2:=-{\mathrm{Im}\;}a=-{\mathrm{Im}\;}\sqrt{|\eta |^2-i}\), where \({\mathcal {F}}_{y\rightarrow \eta }\) denotes the Fourier transform from the variable y to the variable \(\eta \). Fourier transforming in \(y\rightarrow \eta \) and using Young’s inequality, we have
This calculation gives \(\Vert \langle t \rangle ^{-\frac{1}{2}-\varepsilon }{\hat{I}}(t,\eta )\Vert _{L^2_t}\le \Vert \langle t \rangle ^{-\frac{1}{2}-\varepsilon }\Vert _{L^2_t}\Vert {\hat{I}}(t,\eta )\Vert _{L^{\infty }_t}\le C\Vert a_2^{-\frac{1}{2}}{\hat{f}}(t,\eta )\Vert _{L^2_t}\). Plancherel’s theorem and (3.1) imply
\(\square \)
Now we shall prove (1.1) or a stronger bound: \(\Vert \langle t \rangle ^{-\frac{1}{2}-\varepsilon }\langle D_x \rangle ^{\frac{1}{2}}(P-i)^{-1}f\Vert _{L^2({\mathbb {R}}^{n+1})}\le C\Vert f\Vert _{L^2({\mathbb {R}}^{n+1})}\). To do this, it suffices to prove
where we recall \(x=(t,y)\in {\mathbb {R}}\times {\mathbb {R}}^n\). In fact, we take \(\varphi (D_x)=\psi (P/(-\Delta _x+1))\), where \(\psi \!\in \! C_c^{\infty }({\mathbb {R}};[0,1])\) satisfies \(\psi (s)\!=\!1\) on \(|s|\!\le \! \frac{1}{4}\) and \({\mathrm{supp}\;}\psi \!\subset \! \{|s|\!\le \! \frac{1}{2}\}\). Moreover, we set \(\chi (D_x)=\varphi (D_x)\langle D_x \rangle ^{\frac{1}{2}}\langle D_y \rangle ^{-\frac{1}{2}}\). Since P is elliptic on the essential support of \(1-\varphi (D_{x})\), we have \(\Vert (1-\varphi (D_x))\langle D_x \rangle ^{\frac{1}{2}}(P-i)^{-1}f\Vert _{L^2({\mathbb {R}}^{n+1})}\le C\Vert f\Vert _{L^2({\mathbb {R}}^{n+1})}\). Moreover, since \(c^{-1}|\xi |\le |\eta |\le c|\xi |\) on the essential support of \(\varphi (D_x)\) with a constant \(c\ge 1\), it turns out that \(\chi (D_x)\) is bounded in \(L^2({\mathbb {R}}^{n+1})\). Hence,
due to (4.1). Combining these inequalities with (4.2), we obtain (1.1). Now we turn to the proof of (4.1). Lemma A.1 with the formula (3.2) immediately implies
which shows (4.1).
Finally, we prove (1.2) or a stronger bound: \(\Vert \langle t \rangle ^{-\frac{1}{2}-\varepsilon }\langle D_x \rangle (P\!-i)^{-1}\langle t \rangle ^{-\frac{1}{2}-\varepsilon } f \Vert _{L^2({\mathbb {R}}^{n+1})}\le C\Vert f\Vert _{L^2({\mathbb {R}}^{n+1})}\). Lemma A.1 with the formula (3.2) implies
where we recall \(x=(t,y)\in {\mathbb {R}}\times {\mathbb {R}}^n\). Let \(\varphi \) be as in the proof of (4.1) and set \(\chi _1(D_x)=\varphi (D_x)\langle D_x \rangle \langle D_y \rangle ^{-1}\). We repeat an argument similar to the proof of (4.1): Since P is elliptic on the essential support of \(1-\varphi (D_{x})\), we have \(\Vert (1-\varphi (D_x))\langle D_x \rangle (P-i)^{-1}f\Vert _{L^2({\mathbb {R}}^{n+1})}\le C\Vert f\Vert _{L^2({\mathbb {R}}^{n+1})}\). Moreover, since \(c^{-1}|\xi | \le |\eta |\le c|\xi |\) on the essential support of \(\varphi (D_x)\) with a constant \(c\ge 1\), it turns out that \(\chi _1(D_x)\) is bounded in \(L^2({\mathbb {R}}^{n+1})\). Since \(\chi _1(D_x)\) is a pseudodifferential operator of order 0, then \([\langle t \rangle ^{-\frac{1}{2}-\varepsilon },\chi _1(D_x)]\) is a pseudodifferential operator of order \(-1\). Hence, \([\langle t \rangle ^{-\frac{1}{2}-\varepsilon },\chi _1(D_x)]\langle D_y \rangle \) is bounded on \(L^2({\mathbb {R}}^{n+1})\). Thus, we have
This completes the proof of (1.2). See also the proof of [4, Theorem C.1].
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Taira, K. Remarks on the geodesically completeness and the smoothing effect on asymptotically Minkowski spacetimes. Lett Math Phys 112, 22 (2022). https://doi.org/10.1007/s11005-022-01517-2
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DOI: https://doi.org/10.1007/s11005-022-01517-2