Abstract
The incompressible fractional Navier–Stokes equations in the rotational framework is considered. We establish the global existence result and temporal decay estimate for a unique smooth solution when the speed of rotation is sufficiently rapid. It is found that the strong rotational effect enhances the temporal decay rate of a certain norm of the velocity.
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Acknowledgements
The authors express sincere gratitude to the anonymous referees for their helpful remarks and their careful reading of our manuscript. J. Lee’s work is supported by NRF Grant No. 2016R1A2B3011647.
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Appendix
Appendix
In this appendix, we prove Lemmas 8–9 and provide a regularity criteria for (2). We use the notations (27) and (35) for convenience. We note, from the embedding relation \((\dot{H}^s \cap \dot{H}^s_q)(\mathbb {R}^3)\hookrightarrow L^{2}(\mathbb {R}^{3})\) and the skew–symmetry of \(\varOmega e_{3}\times u\), that a solution u in Lemma 8 or Lemma 9 satisfies
Proof of Theorem 3
By Lemma 1 and the boundedness properties of Leray projection, we have
where \(r>1\) is a number
Note that \(1-\frac{1}{p}<\frac{1}{r}\). Indeed, by the upper inequality of (3)\(_{1}\) and \(\frac{1}{2}<\alpha \le \frac{5}{4}\), we have \( s<\ \frac{3(5-2\alpha )}{2(2\alpha +3)}< \frac{3(2-\alpha )}{2(2\alpha -1)} \) and thus, it follows from the lower inequality of (3)\(_{2}\) that \( \frac{\alpha }{\alpha +1}\left( \frac{s}{3}+\frac{1}{2} \right) <\frac{1}{3}+\frac{s}{9}\le \frac{1}{p}\), and so \(1-\frac{1}{p}<\frac{1}{r}\). Using the interpolation inequality
(A.1), and a direct computation, we have
where \( J:= \int _0^{\frac{t}{2}} R(\tau )^{-\alpha }d\tau \). Using change of variable \(\tilde{\tau } = |\varOmega |\tau \), we note that
Using \( \frac{1}{p} \ge \frac{1}{3}>\frac{1}{q} - \frac{2}{3} \), we also note that
Now, we consider two cases
separately.
In the case of
the boundedness of the integral term in (A.4) gives
Thus, it follows from (A.2)–(A.3) that
Using \(\frac{1}{p}\ge \frac{1}{3}+\frac{s}{9}\) and \(q>1\), we note that
and thus,
By this fact with \(t\ge 1\), it follows that
Therefore, (47) is obtained.
We next deal with the case
By a direct calculation, if \(1-\frac{3}{2} \left( \frac{1}{q} - \frac{1}{p} \right) - \alpha \left( 1 - \frac{2}{p} \right) >0\), then we have
and if \(1-\frac{3}{2} ( \frac{1}{q} - \frac{1}{p} )- \alpha ( 1 - \frac{2}{p} )=0\), then we have
Thus, we can compute J in (A.4) as
Then, it follows from (A.3) that
In the case of \(\frac{1}{2}<\alpha < 1\), we have
In the case of \(1\le \alpha \le \frac{5}{4}\), using \(\frac{5}{2} - 2\alpha < s\), we have
Hence, with \(t > 1\) we observe that
Therefore, (47) is obtained. This completes the proof.
Proof of ....
By (A.1) and interpolation inequality, we have
where \(r >1\) is a number
Note that \(1-\frac{1}{p}<\frac{1}{r}\). Indeed, by the upper inequality of (3)\(_{1}\) and \(\frac{5}{4}<\alpha <\frac{5}{2}\), we have \( s<\ \frac{3(5-2\alpha )}{2(2\alpha +3)}< \frac{3(\alpha +1)}{(8\alpha -1)} \) and thus, it follows from the lower inequality of (3)\(_{2}\) that \( \frac{\alpha (2s+3)}{10\alpha +1}<\frac{1}{3}+\frac{s}{9}\le \frac{1}{p}\), and so \(1-\frac{1}{p}<\frac{1}{r}\). Then, it follows from (A.2) that
where \(\tilde{J}:= \int _0^{\frac{t}{2}} R(\tau )^{-\frac{6\alpha }{4\alpha + 1}}d\tau \) and this can be rewritten as
Now, we claim that
Indeed, by \(q>1\), \(\frac{1}{3}+\frac{s}{9}\le \frac{1}{p}\), \(s>0\), and \(\frac{5}{4}<\alpha \), the lower inequality of (A.8) holds true. The upper inequality of (A.8) holds true because \(\frac{1}{q} \ge \frac{1}{3} + \frac{2}{p} - \frac{s}{3}\) gives
the upper inequality of (3)\(_2\) gives
and the upper inequality of (3)\(_1\) gives
By (A.8), the integral term in (A.7) is bounded and thus,
Then, it follows from (A.6) that
Moreover, we see that
because \(\frac{1}{q} < 1\) and (3)\(_2\) implies
Therefore, with \(t > 1\) we have
Hence, (48) is obtained. This completes the proof. \(\square \)
We close the appendix by giving a regularity criterion for (2). Using the estimates in the proof below we can deduce that the solution to (2) given by Theorem 1 is smooth for \(t>0\) .
Lemma 10
Let \(\alpha >\frac{1}{2}\), \(u_{0}\in H^{5\alpha }(\mathbb {R}^{3})\), and \(\mathrm {div}\, u_0 = 0\). Suppose that \((u,\pi )\) is a weak solution to (2) subject to the initial data \(u_{0}\), and satisfies
Then, \((u,\pi )\) is smooth for \(0<t\le T\).
Proof
We note that the classical solvability of (2) with \(\varOmega =0\) for \(\alpha \ge \frac{5}{4}\) was obtained by Lions [16] and its extension to the case of nonzero \(\varOmega \) is rather straightforward. We also note, for \(1\le \alpha \le \frac{3}{2}\), that the regularity criterion (A.9) can be found in [22]. Thus, it is sufficient to deal with the case \(\frac{1}{2}<\alpha <1\).
Let \(\frac{1}{2}<\alpha <1\). We only provide the estimate for \( u\in L^{\infty }(0,T; \dot{H}^{\alpha } )\cap L^{2}(0,T; \dot{H}^{2\alpha } ) \) because the higher order estimates \(u\in L^{\infty }(0,T; \dot{H}^{k\alpha })\cap L^{2}(0,T; \dot{H}^{(k+1)\alpha })\), \(k=2,3,4,5\) can be obtained in a similar way. We denote \(\varLambda \) as the \(\frac{1}{2}\) power of the negative Laplacian, i.e., \(\varLambda =(-\varDelta )^{\frac{1}{2}}\). Multiplying both sides of (2) by \(\varLambda ^{2\alpha } u\), integrating over \(\mathbb {R}^{3}\), and using Hölder’s inequality, we can compute
Using Young’s inequality and the interpolation inequality
we have
Applying Grönwall’s inequality to (A.10), and using (A.9) with \(\frac{2\alpha }{2/(1-\lambda )}=2\alpha -1-\frac{3}{r}\), we see that \( u\in L^{\infty }(0,T; \dot{H}^{\alpha })\cap L^{2}(0,T; \dot{H}^{2\alpha })\). This completes the proof.\(\square \)
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Ahn, J., Kim, J. & Lee, J. Coriolis effect on temporal decay rates of global solutions to the fractional Navier–Stokes equations. Math. Ann. 383, 259–289 (2022). https://doi.org/10.1007/s00208-020-02122-1
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DOI: https://doi.org/10.1007/s00208-020-02122-1