Abstract
This work is concerned with the construction of Gaussian Beam (GB) solutions for the numerical approximation of wave equations, semi-discretized in space by finite difference schemes. GB are high-frequency solutions whose propagation can be described, both at the continuous and at the semi-discrete levels, by microlocal tools along the bi-characteristics of the corresponding Hamiltonian. Their dynamics differ in the continuous and the semi-discrete setting, because of the high-frequency gap between the Hamiltonians. In particular, numerical high-frequency solutions can exhibit spurious pathological behaviors, such as lack of propagation in space, contrary to the classical space-time propagation properties of continuous waves. This gap between the behavior of continuous and numerical waves introduces also significant analytical difficulties, since classical GB constructions cannot be immediately extrapolated to the finite difference setting, and need to be properly tailored to accurately detect the propagation properties in discrete media. Our main objective in this paper is to present a general and rigorous construction of the GB ansatz for finite difference wave equations, and corroborate this construction through accurate numerical simulations.
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Notes
We recall that, given two vectors \(\varvec{v} = (v_1,v_2,\ldots ,v_d)\in \mathbb {R}^d\) and \(\varvec{w} = (w_1,w_2,\ldots ,w_d)\in \mathbb {R}^d\), their Hadamard product is the vector \(\varvec{v}\odot \varvec{w} = \varvec{z} = (z_1,z_2,\ldots ,z_d)\in \mathbb {R}^d\) with \(z_i=v_iw_i\) for all \(i\in \{1,\ldots ,d\}\).
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Acknowledgements
The authors wish to acknowledge Dr. Konstantin Zerulla (Friedrich-Alexander-Universität Erlangen-Nürnberg, Germany) for his careful revision and precious comments on early versions of this work.
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E. Zuazua has been funded by the Alexander von Humboldt-Professorship program, the ModConFlex Marie Curie Action, HORIZON-MSCA-2021-DN-01, the COST Action MAT-DYN-NET, the Transregio 154 Project “Mathematical Modelling, Simulation and Optimization Using the Example of Gas Networks” of the DFG, Grants PID2020-112617GB-C22 and TED2021-131390B-I00 of MINECO (Spain), and by the Madrid Government—UAM Agreement for the Excellence of the University Research Staff in the context of the V PRICIT (Regional Programme of Research and Technological Innovation)
Appendices
Appendix A. Proof of Theorem 4.1
We give here the proof of Theorem 4.1, concerning the construction of a GB ansatz for the wave equation (1.1). To this end, we shall first need the following technical result.
Proposition A.1
Let \({\varvec{x}}_0\in \mathbb {R}^d\), \(N\in \mathbb {N}\) and \(f\in L^\infty (\mathbb {R}^d)\) be a function satisfying
Then, for any positive constant \(0<\beta \in \mathbb {R}\), we have
for some \(\mathcal C= \mathcal C(d,N,\beta ) > 0\) that does not depend on k.
Proof
Using (A.1), we have that there exists a function \(g\in L^\infty (\mathbb {R}^d)\) such that
In view of this, we can apply the Hölder inequality to estimate
Now, by means of the change of variable \(\varvec{y} = \sqrt{2k\beta }({\varvec{x}}-{\varvec{x}}_0)\), we obtain that
Finally, by employing polar coordinates, we can compute
where \(\Gamma \) denotes the Euler gamma function. Putting everything together, we finally obtain that
\(\square \)
Proof of Theorem 4.1
We organize the proof in three steps, one for each statement of the theorem.
Step 1: proof of (4.7). Starting from (4.14), we have that
where we recall
Since \(a,\phi \in C^\infty (\mathbb {R}^d\times \mathbb {R})\), we clearly have that also \(r_0,r_1,r_2 \in C^\infty (\mathbb {R}^d\times \mathbb {R})\). Moreover, by construction, \(r_1\) and \(r_2\) vanish on \({\varvec{x}}={\varvec{x}}(t)\) up to the order 0 and 2. In view of that, we have that \(r_0,r_1,r_2\) satisfy (A.1) with \(N = 0\), \(N = 1\) and \(N = 3\), respectively. Then, applying Proposition A.1 with \({\varvec{x}}_0 = {\varvec{x}}(t)\) and the previous values of \(N\in \mathbb {N}\), we get
Putting everything together, since \(k\ge 1\), we finally obtain that
that is,
Step 2: proof of (4.8). Starting from (4.1), we have that
where we have denoted
Notice that since \(a,\phi \in C^\infty (\mathbb {R}^d\times \mathbb {R})\) and \(\Im (M_0)>0\), we have that for all \(t\in (0,T)\)
Hence,
As for the term \(\Xi _0^k(t)\), replacing in it the explicit expression (4.5) of the amplitude function a, we get that
where \(I_d\) denotes the identity matrix in dimension \(d\times d\). Moreover, using (3.7) and the explicit expression (4.6) of the phase function a, we can compute
and we obtain from (A.4) that
Now, since \(2 I_d + k\Im (M_0)>0\), we can apply the change of variables
and we get
Finally, the two integrals in the expression above can be computed by employing polar coordinates. In this way, we obtain that
Hence,
From (A.3) and (A.5), we immediately get (4.8).
Step 3: proof of (4.9). Since \(a,\phi \in C^\infty (\mathbb {R}^d\times \mathbb {R})\) and \(k\ge 1\), we have that
with \(\mathcal C= \mathcal C(a,\phi )>0\) a positive constant not depending on k. Moreover, by employing the change of variable \(\varvec{y} = k^{-\frac{1}{2}}\varvec{z}\), we have that
From this last estimate, (4.9) follows immediately. \(\square \)
Appendix B. Proof of Theorem 5.1
1.1 B.1. Concentration of Solutions
We give here the proof of Theorem 5.1, concerning the construction of a GB ansatz for the semi-discrete wave equation (5.2).
Proof of Theorem 5.1
We are going to split the proof into three steps, one for each point in the statement of the theorem. Moreover, in what follows, we will denote by \(\mathcal C>0\) a generic positive constant independent of h. This constant may change even from line to line.
Step 1: proof of(5.10). Starting from (5.46), we have that
Moreover, using (5.35), we see that
and, therefore,
In view of this, we get
Now, by means of (5.31) and (5.45), we have that
and
Hence,
The first two terms on the right-hand side of the above inequality can be estimated by observing that
This can be easily seen by considering the Riemann sum approximating on the mesh \(\mathcal G_h\) the integral
Hence, using (B.2), we obtain that
and, therefore,
Finally, since by construction \(\widetilde{\mathcal R}_1 A_j\) and \(\mathcal R_{fd}\) vanish on the discrete characteristics \(x_{fd}(t)\) up to the order 0 and 2, respectively, we have that
This is the discrete version of Proposition A.1, which can be proven once again by applying Riemann sum to approximate the corresponding integrals. In view of this, we obtain
and we can finally conclude that
Step 2: proof of(5.11). First of all, starting from (5.3), (5.4) and (5.23), we can write
Moreover, we can easily compute
Using these identities and (B.1), we then obtain
where we have denoted
Moreover, by construction of A and \(\Phi \), we have that \(|\mathcal S_i|\le \mathcal C(A,\phi )\) for \(i\in \{1,2,3\}\). Using this and (B.2), we finally obtain
Step 3: proof of(5.12). Repeating the computations of Step 2, we have that
with \(\mathcal S_1\), \(\mathcal S_2\) and \(\mathcal S_3\) defined in (B.3a), (B.3b) and (B.3c), respectively. Hence, recalling that \(|\mathcal S_i|\le \mathcal C(A,\Phi )\) for \(i\in \{1,2,3\}\), we obtain
Now, employing the transformation
and denoting
we have that
Substituting this in (B.4), we finally conclude that
\(\square \)
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Biccari, U., Zuazua, E. Gaussian Beam Ansatz for Finite Difference Wave Equations. Found Comput Math (2023). https://doi.org/10.1007/s10208-023-09632-9
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DOI: https://doi.org/10.1007/s10208-023-09632-9