M.C. Veraar
Please Note
13 records found
1
Will It Blow Up?
Existence of Global Solutions of Weighted Nonlocal Reaction-Diffusion Problems
m
. In this equation we consider the evolution as a result of diffusion, nonlinear local growth and a weighted nonlocal inhibition term that considers the current state of the entire domain. These equations are particularly useful for models in biology, chemistry and evolution theory.
The main objective is to extend an existing global existence result for an unweighted nonlocal reaction-diffusion equation to a weighted one for a positive bounded weight. Unlike the original result, showing only the boundedness of solutions, we show the entire process of proving the global existence of classical solutions.
After introducing the necessary analytical tools and notations we go about proving the main result in five steps. Firstly we prove the existence of a unique mild solution using the well-known Banach fixed-point method. Standard regularity results are then used to obtain a local classical solution. With a classical solution in hand we can study various properties of the solution. First, it is shown that non-negative initial data results in non-negative solutions by means of bounding the size of the negative part of the solution by 0. Next, uniform a priori estimates are derived in L
k
(R
m
) for β≤k≤∞, where β comes from the nonlinearity inside the nonlocal inhibition term. These estimates hold under some restrictions concerning the exponents of the equation and the dimension of the x-domain. The most important aspect of these estimates is that they are independent of the local existence time. The proof for these estimates follows that of the unweighted nonlocal reaction-diffusion equation.
Finally, a continuation argument is employed, using the a priori estimate and the fact that it is independent of the local existence time, to show that every unique local classical solution of an equation satisfying the restrictions needed for the a priori estimate can be extended to a unique global classical solution. This concludes the extension of the global existence of solutions to the weighted problem.
As a last note, we also discuss the possibility of further study into the existence of global solutions for less restricted weights. ...
m
. In this equation we consider the evolution as a result of diffusion, nonlinear local growth and a weighted nonlocal inhibition term that considers the current state of the entire domain. These equations are particularly useful for models in biology, chemistry and evolution theory.
The main objective is to extend an existing global existence result for an unweighted nonlocal reaction-diffusion equation to a weighted one for a positive bounded weight. Unlike the original result, showing only the boundedness of solutions, we show the entire process of proving the global existence of classical solutions.
After introducing the necessary analytical tools and notations we go about proving the main result in five steps. Firstly we prove the existence of a unique mild solution using the well-known Banach fixed-point method. Standard regularity results are then used to obtain a local classical solution. With a classical solution in hand we can study various properties of the solution. First, it is shown that non-negative initial data results in non-negative solutions by means of bounding the size of the negative part of the solution by 0. Next, uniform a priori estimates are derived in L
k
(R
m
) for β≤k≤∞, where β comes from the nonlinearity inside the nonlocal inhibition term. These estimates hold under some restrictions concerning the exponents of the equation and the dimension of the x-domain. The most important aspect of these estimates is that they are independent of the local existence time. The proof for these estimates follows that of the unweighted nonlocal reaction-diffusion equation.
Finally, a continuation argument is employed, using the a priori estimate and the fact that it is independent of the local existence time, to show that every unique local classical solution of an equation satisfying the restrictions needed for the a priori estimate can be extended to a unique global classical solution. This concludes the extension of the global existence of solutions to the weighted problem.
As a last note, we also discuss the possibility of further study into the existence of global solutions for less restricted weights.
Y(t) = ∫R(t-x)+H(x)-1/α - (-x)+H(x)-1/α dL(x).
Here (x)+ = max(x, 0), α ∈ (0, 2), L is a standard symmetric α-stable Lévy process and finally, the multifractional parameter H is a jointly measurable stochastic process, adapted to the natural filtration generated by L, taking values in [H-,H-] ⊆ (0, 1). Under the assumption that H admits a deterministic modulus of continuity w and that H is strictly bounded from below by 1/α, it is proven that the uniform Hölder exponent ρYunif([a,b]) over a compact interval satisfies
ρYunif([a,b]) ≥ mint∈[a,b]H(t)-1/α.
Under the further assumption that w(h) log h → 0 as h ↓ 0, it is shown that Y is locally self-similar and that the pointwise Hölder exponent ρY(t) satisfies
ρY(t) ≤ H(t). ...
Y(t) = ∫R(t-x)+H(x)-1/α - (-x)+H(x)-1/α dL(x).
Here (x)+ = max(x, 0), α ∈ (0, 2), L is a standard symmetric α-stable Lévy process and finally, the multifractional parameter H is a jointly measurable stochastic process, adapted to the natural filtration generated by L, taking values in [H-,H-] ⊆ (0, 1). Under the assumption that H admits a deterministic modulus of continuity w and that H is strictly bounded from below by 1/α, it is proven that the uniform Hölder exponent ρYunif([a,b]) over a compact interval satisfies
ρYunif([a,b]) ≥ mint∈[a,b]H(t)-1/α.
Under the further assumption that w(h) log h → 0 as h ↓ 0, it is shown that Y is locally self-similar and that the pointwise Hölder exponent ρY(t) satisfies
ρY(t) ≤ H(t).
To show stability, we construct a multiscale expansion of the solution around an arbitrarily shifted version of the pattern, and show that this expansion is accurate to second order. From this expansion an obvious candidate for the correct phase shift arises. For technical reasons we then construct a sequence of approximations to this phase shift, which is necessary to show the multiscale expansion around the correctly shifted pattern. We then combine this expansion with a deterministic stability result to get stochastic stability.
Finally, we take first steps towards formulating and proving the same results in a more general setting, where the pattern shift is represented by the action of a Lie group. We obtain some estimates necessary for the multiscale expansion, find the correct phase, and formulate necessary assumptions for the stability to hold. ...
To show stability, we construct a multiscale expansion of the solution around an arbitrarily shifted version of the pattern, and show that this expansion is accurate to second order. From this expansion an obvious candidate for the correct phase shift arises. For technical reasons we then construct a sequence of approximations to this phase shift, which is necessary to show the multiscale expansion around the correctly shifted pattern. We then combine this expansion with a deterministic stability result to get stochastic stability.
Finally, we take first steps towards formulating and proving the same results in a more general setting, where the pattern shift is represented by the action of a Lie group. We obtain some estimates necessary for the multiscale expansion, find the correct phase, and formulate necessary assumptions for the stability to hold.
through different materials.
Because the wave equation is such an important tool to model these phenomena, there are many people working on solving the wave equation in different contexts, i.e. finding a solution. However, it is difficult (often impossible) to find an exact solution. Therefore, people usually calculate a ’solution’ that is approximately correct.
An important question to ask is: ’Does the wave equation always have a solution?And is there only one solution?’. Physically, the answer is clear. If a string is vibrating, it clearly cannot vibrate in two ways at the same time and it will always vibrate in some particular way. Even though the answer is clear physically, answering this question mathematically is more difficult. It is good to remember that the wave equation is just a mathematical model of propagating waves, and it could very well be that the wave equation has more than one solution or no solution at all in some particular context.
The answer of this question is important for the people calculating approximate solutions to the wave equation. If there does not exist a unique solution, the process of calculating the approximate solution may break down.
Answering that question is the subject of this thesis. We will first introduce the necessary mathematical tools, after which we will use existing research to find out under which conditions the wave equation has one, and only one solution. Finally, we will extend our results to more general equations than just the wave equation. ...
through different materials.
Because the wave equation is such an important tool to model these phenomena, there are many people working on solving the wave equation in different contexts, i.e. finding a solution. However, it is difficult (often impossible) to find an exact solution. Therefore, people usually calculate a ’solution’ that is approximately correct.
An important question to ask is: ’Does the wave equation always have a solution?And is there only one solution?’. Physically, the answer is clear. If a string is vibrating, it clearly cannot vibrate in two ways at the same time and it will always vibrate in some particular way. Even though the answer is clear physically, answering this question mathematically is more difficult. It is good to remember that the wave equation is just a mathematical model of propagating waves, and it could very well be that the wave equation has more than one solution or no solution at all in some particular context.
The answer of this question is important for the people calculating approximate solutions to the wave equation. If there does not exist a unique solution, the process of calculating the approximate solution may break down.
Answering that question is the subject of this thesis. We will first introduce the necessary mathematical tools, after which we will use existing research to find out under which conditions the wave equation has one, and only one solution. Finally, we will extend our results to more general equations than just the wave equation.
We propose a model based on Gaussian random fields, defined as the solutions to a class of space-time fractional stochastic partial differential equations (SPDEs) driven by Gaussian noise. The tunable parameters characterizing this class are expected to admit intuitive interpretations, in which case an efficient numerical approximation scheme for solutions to these SPDEs yields a powerful spatiotemporal model which is usable in practice.
The study of this class of SPDEs is the focus of this work. We define weak and mild solution concepts and show their equivalence under lenient conditions on the differential operators involved. Subsequently we establish results linking the well-posedness, spatiotemporal regularity and asymptotic covariance structure of the SPDEs to conditions on the model parameters, confirming their interpretability. Lastly, we specialize the SPDEs to a class of fractional ordinary differential equations in time, and describe a method to compute numerical approximations of their solutions. Future work is needed to analyze this scheme and generalize it to the original class of SPDEs. ...
We propose a model based on Gaussian random fields, defined as the solutions to a class of space-time fractional stochastic partial differential equations (SPDEs) driven by Gaussian noise. The tunable parameters characterizing this class are expected to admit intuitive interpretations, in which case an efficient numerical approximation scheme for solutions to these SPDEs yields a powerful spatiotemporal model which is usable in practice.
The study of this class of SPDEs is the focus of this work. We define weak and mild solution concepts and show their equivalence under lenient conditions on the differential operators involved. Subsequently we establish results linking the well-posedness, spatiotemporal regularity and asymptotic covariance structure of the SPDEs to conditions on the model parameters, confirming their interpretability. Lastly, we specialize the SPDEs to a class of fractional ordinary differential equations in time, and describe a method to compute numerical approximations of their solutions. Future work is needed to analyze this scheme and generalize it to the original class of SPDEs.
...
This thesis considers the thin-film equation in partial wetting. The mobility in this equation is given by h3+λ3-nhn, where h is the film height, λ is the slip length and n is the mobility exponent. The partial wetting regime implies the boundary condition dh/dz>0 at the triple junction. The asymptotics as h↓0 are investigated. This is done by using a dynamical system for the error between the solution and the microscopic contact angle. Using the linearized version of the dynamical system, values for n when resonances occur are found. These resonances lead to a different behaviour for the solution as h↓0, so the asymptotics are found to be different for different values of n. Together with the asymptotics for h→∞ as found in [Giacomelli et al., 2016], the solution to the thin-film equation in partial wetting can be characterized. Also, via this solution, the relation between the microscopic and macroscopic contact angles can be analyzed. From the main result of this thesis, it can be seen that the macroscopic Tanner law for the contact angle depends smoothly on the microscopic contact angle. ...
This thesis considers the thin-film equation in partial wetting. The mobility in this equation is given by h3+λ3-nhn, where h is the film height, λ is the slip length and n is the mobility exponent. The partial wetting regime implies the boundary condition dh/dz>0 at the triple junction. The asymptotics as h↓0 are investigated. This is done by using a dynamical system for the error between the solution and the microscopic contact angle. Using the linearized version of the dynamical system, values for n when resonances occur are found. These resonances lead to a different behaviour for the solution as h↓0, so the asymptotics are found to be different for different values of n. Together with the asymptotics for h→∞ as found in [Giacomelli et al., 2016], the solution to the thin-film equation in partial wetting can be characterized. Also, via this solution, the relation between the microscopic and macroscopic contact angles can be analyzed. From the main result of this thesis, it can be seen that the macroscopic Tanner law for the contact angle depends smoothly on the microscopic contact angle.
We first consider a classical proof of boundedness of the Hardy-Littlewood maximal operator on rearrangement invariant Banach function spaces. After establishing necessary and sufficient conditions for the boundedness of the Hardy-Littlewood maximal operator, we consider a generalization of the Hardy-Littlewood maximal operator introduced by C. Pérez. We investigate and slightly improve the known sufficient conditions under which this more general maximal operator is bounded on a rearrangement invariant Banach function space. After which we search and find necessary conditions for boundedness in a general setting. In the final section we study Boyd indices and fundamental indices, especially how they are related to boundedness of the more general maximal operator. We also introduce weak fundamental indices and investigate some of their properties and uses. Finally we show how under certain assumptions we can state equivalent necessary and sufficient conditions for boundedness on Lorentz spaces and Orlicz spaces. ...
We first consider a classical proof of boundedness of the Hardy-Littlewood maximal operator on rearrangement invariant Banach function spaces. After establishing necessary and sufficient conditions for the boundedness of the Hardy-Littlewood maximal operator, we consider a generalization of the Hardy-Littlewood maximal operator introduced by C. Pérez. We investigate and slightly improve the known sufficient conditions under which this more general maximal operator is bounded on a rearrangement invariant Banach function space. After which we search and find necessary conditions for boundedness in a general setting. In the final section we study Boyd indices and fundamental indices, especially how they are related to boundedness of the more general maximal operator. We also introduce weak fundamental indices and investigate some of their properties and uses. Finally we show how under certain assumptions we can state equivalent necessary and sufficient conditions for boundedness on Lorentz spaces and Orlicz spaces.
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