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Discrete.Differential.Geometry-An.Applied.Introduction(sig2008)笔记

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Chapter 1: Introduction to Discrete Differential Geometry: The Geometry of Plane Curves

A better approximation than the tangent is the circle of curvature.

If the curve is sufficiently smooth (“curvature-continuous at P 】”) then the circle thus approaches a definite position known as the circle of curvatureor osculating circle; the center and radius of the osculating circle are the center of curvatureand radius of curvatureassociated to point P on the curve. The inverse of the radius is K, the curvatureof the curve at P .

Informally we say that P , the tangent at P , and the osculating circle at P have one, two, and three coincident points in common with the curve, respectively. Each construction in sequence considers an additional approaching point in the neighborhood of P and the so-called order of approximation

(0, 1, and 2 respectively) is identical to the number of additional points.

turning number /the index of rotation, denoted k

the integral of signed curvature over a closed curve, Ω, is dependent only on the turning number:

?$_Ω$ K ds = 2πk .

no matter how much we wiggle and bend the curve, if we do not change its turning number we do not change its total signed curvature

tsc(p) = αi, tsc(r) = sup{p inscribed in r} tsc(p)

p: polygon

r: the continuous curve

.

geometric mesh size of p: h(p) = max{0≤i<n} d(V i , V i+1 ) .

parametric mesh size of p: hR(p) = max (t i+1 − t i )

.

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CH2 What Can We Measure?

for a convex, compact set in Rn there are only n+1 unique measurements if we require that the measurements be invariant under Euclidean motions (and satisfy certain “sanity” conditions)

.

A measure测度】 is a function μ defined on a family of subsets L of some set S, and it returns real values: μ:L→R

L is closed under finite set union and intersection as well as that it contains the empty set, ∅ ∈ L.

Property:

(1) μ(∅) = 0

(2) μ(A ∪ B) = μ(A) + μ(B) − μ(A ∩ B) (additivity property)

我们只关心在欧式空间下不变的那些运动(rigid motion invariant motion)e.g. translations and rotation。这使得我们的measure不依赖于坐标系原点和坐标轴的旋转(invariant measure)。相反,variant measure依赖于原点和坐标轴的旋转, 没有太大用处。

μ$_m$$^n$:

m:a measure on Rm

n: type of measurement

.

an affine subspaceof dimension k is spanned by k+1 points pi ∈ Rn (in general position), i.e., the space consists of all points q which can be written as affine combinations q = αi*pi , αi = 1.

Such an affine subspace is simply a linear subspace translated

integrals of Gaussian curvature on a triangle mesh become sums over excess angle at vertices

integrals of mean curvature can be identified with sums over edges of dihedral angle weighted by edge length.

These quantities are always integrals. Consequently they do not make sense as pointwise quantities.

In the case of smooth geometry we can define quantities such as mean and Gaussian curvature as pointwise quantities.

Let P be a polyhedron with vertex set V and edge set E and B a ball in R3 then we can define integrated Gaussian and mean curvature measures as

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- Kv = 2π − j αj is the excess angle sum at vertex v defined through all the incident triangle angles at v,

- l(.) denotes the length,

- θe is the signed dihedral angle at e made between the incident triangle normals. Its sign is positive

for convex edges and negative for concave edges (note that this requires an orientation on the polyhedron).


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Chapter 3: Curvature Measures for Discrete Surfaces

A smooth space curve γ is often described by its orthonormal Frenet frame(T, N, B)

For a curve γ lying on a surface M , it is often more useful to consider the Darboux frame(T, η, ν)

This orthonormal frame includes the tangent vector T to γ and the normal vector ν to M . Its third element is thus η := ν × T , called thecornormal】。

The curvature vector of γ decomposes into parts tangent and normal to M as T‘ = κN = κg η +κn ν. Here in fact, κn measures the normal curvature of M in the direction T , and is independent of γ

The map Sp is called the shape operator (or Weingarten map)

The eigenvalues κ1 and κ2 of Sp are called principal curvatures

Gauss curvature K := κ1*κ2 as the determinant of Sp

the mean curvature H := κ1 + κ2 as its trace.

vector mean curvature (or mean curvature vector) H := Hν = (κ1 + κ2) ν (unit normal ν)

Mean curvature is certainly not intrinsic, but it has a nice variational interpretation.

H = −δ Area / δ Vol

δv Vol = V · ν dA, δv Area = − V · H ν dA


With respect to the L2 inner product <U, V > := Up · Vp dA on vectorfields, the vector mean curvature is the negative gradient of the area functional, often called the first variation of area:

H = Hν = −∇ Area.

(Similarly, the negative gradient of length for a curve is κN κN = −∇ Length)

.

Gauss curvature K is the geometric version of second derivative for curves,

Mean curvature H is the geometric version of the Laplacian ?

.

if a surface M is written locally as the graph of a height function f over its tangent plane TpM then

H(p) = ?f . Alternatively, we can write H = ∇$_M$ ·ν = ?$_M$ x, (

where x is the position vector in R3, ?$_M$ is Beltrami’s surface Laplacian, ν is the unit normal .

.

If we flow a curve or surface to reduce its length or area, by following these gradients κN and Hν, the resulting parabolic heat flow is slightly nonlinear in a natural geometric way. This so-called mean-curvature flowhas been extensively studied as a geometric smoothing flow.

Gauß–Bonnet theorem for discrete surfaces

∫∫$_D$ K dA := $_p$ Kp; Kp := 2PI - $_i$θi


θi are the interior angles at p of the triangles meeting there

Kp is often known as the angle defect at p.

If D is any neighborhood of p contained in Star(p), then ∮$_D$ ηds = ∑ θi .

.

The mean curvature of a discrete surface M is supported along the edges

.

The area of the discrete surface is a function of the vertex positions


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Chapter 4: A Discrete Model of Thin Shells

total curvature: κ1^2 + κ2^2


bending energy functional: E(S) = $_S$ H^2 dvol


The importance of isometry for simplification of energy was previously acknowledged in the context of surface fairing and modeling


If I : S → E3 denotes the embedding of the surface, the mean curvature normal H of S can be written as the intrinsic Laplacian ? (induced by the Riemannian metric of S) applied to the embedding of the surface, H = ?I,

E(S) = $_S$ <?I, ?I> dvol


Therefore we must begin with a reasonable definition of isometry, which in the case of triangulated surfaces we take to be that

(a) bending occurs only along edges,

(b) edges may not stretch.


In analogy to the smooth case, a discrete IBM will be based on Laplacians which are—by construction—invariant under discrete isometric deformations.(详见CH11)


Although bending forces are much weaker then stretching forces, their interaction with membrane forces determines the shape of folds and wrinkles that we associate with garments and other thin flexible bodies.


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Straightest Geodesics on Polyhedral Surfaces ∗


Geodesics on smooth surfaces can be characterized by different equivalent properties. The generalized properties on polyhedral surfaces will no longer be equivalent and lead to different classes of discrete geodesics.

.

κ(s)^2 = κg (s)^2 + κn (s)^2

κg : geodesic curvature

κn : normal curvature

The geodesic curvature κg of a curve γ measures the tangential acceleration. If κg = 0 then the curve varies up to second order only in direction of the surface normal, therefore it is a straightest curve

on the surface. The normal curvature κn is related with the bending of the surface itself and can be neglected from an intrinsic point of view


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Definition 1

Let M be a smooth two-dimensional surface. A smooth curve γ:I→M with | γ‘ | = 1 is a geodesic if one of the equivalent properties holds:

1. γ is a locally shortest curve.

2. γ‘‘ is parallel to the surface normal, i.e.

γ‘‘(s)$^{tan M}$ = 0. (表示γ‘‘(s)M切面上的分量)

3. γ has vanishing geodesic curvature κg = 0.

Definition 4

A vertex p of a polyhedral surface S with total vertex angle θ (p) is called Euclidean, spherical, or hyperbolic if its angle excess 2 π − θ (p) is = 0, > 0, or < 0. Respectively, interior points of a face or of an open edge are Euclidean

The isometric unfolding of sets of a polyhedral surface is a common procedure to study the geometry.

Definition 5

The (total) Gauß curvatureK(p) of a vertex p on a polyhedral surface S is defined as the vertex angle excess

K(p) = 2π − θ (p) = 2π − ∑θi(p)

.

之所以选择straightest geodesic而不选择shortest geodesics,因为后者沿不同方向有不同的解。

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CH 8  Building Your Own DEC at Home
如何离散化微分算子d和Hodge star

CH9 介绍 如何离散化速度/散度/旋度;Discrete.Differential.Geometry-An.Applied.Introduction(sig2013).pdf 里6.3. Discretization via DEC介绍如何离散化Laplacian算子


假设说有一个2d网格M,里面有边和顶点。有一个向量场F,现在求F对M的flux。flux是要对face做运算 的。但现在假设只能对vertex做运算,该怎么办?也就是说要考虑,原先F作用于某个区域,现在我要把这个区域用一个vertex来代替,然后让F作用 于这个vertex上。那么问题来了,我怎么把一个区域用vertex vi而不是vj来代替?
一种很直观的方法就是,如果某个区域上的点到vi的距离(|p-vi|)最近,那么就有理由用vi来代表这个区域。这就是Voronoi划分。
原先F在连续区域上做运算,现在F在离散点上做运算。这就是DEC
上面只是粗糙的比喻。实际上为了能计算出正确结果,那个连续区域也要变。变成什么?由Hodge star来计算

Hodge star为什么那么定义?论文里有说:
We again attempt to motivate the definition with some intuition.
When transferring a quantity from a primal simplex to a dual cell, the quantities must “agree” somehow. Since these are integral values, simply setting the value on the dual to be equal to the value on the primal does not make sense, as the domain of integration is unrelated. Instead, we require that the integral density be equal. So, if ω denotes the evaluation of a form on a primal k-simplex σ , then ?ω is the value on the dual (n − k)-cell σ ? such that :
ω / Vol(σ ) = ?ω / Vol( σ ? )

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Chapter 9: Stable, Circulation-Preserving, Simplicial Fluids(如何离散化速度/散度/旋度)

In order to work towards this goal, more work needs to be done to further demonstrate that

this idea of forms as fundamental readily-discretizable elements of differential equations can be successfully used in various other contexts where predictive power is crucial.

.

Despite the simplicity of this fractional integration, one of its consequences is excessive numerical diffusion: advecting velocity before reprojecting onto a divergence-free field creates significant energy loss详见:《Analysis of an exact fractional step method》

One can understand this seemingly inevitable numerical diffusion through the following geometric argument: the solutions of Euler equations are geodesic (i.e., shortest) paths on the manifold of all possible divergence-free flows;详见:《Analysis of an exact fractional step method》

In this paper we show that a careful setup of discrete differential quantities, designed to respect structural relationships such as vector calculus identities, leads in a direct manner to a numerical simulation method which respects the defining geometric structure of the fluid equations. A key ingredient in this approach is the location of physical quantities on the appropriate geometric structures (i.e.,vertices, edges, faces, or cells).This greatly simplifies the implementation as all variables are intrinsic.

.

易于实现:

all quantities are stored intrinsically (scalars on edges and faces) without reference to global or local coordinate frames

 

 


 

The reader should now realize that in our discretization of physical quantities,

 

the notion of flux that we described is thus a primal 2-form (integrated over faces),

 

while its vorticity is a dual 2-form (integrated over dual faces),

 

and its divergence becomes a primal 3-form (integrated over tetrahedra).

 

 

Helmholtz-Hodge decomposition theorem:any vector field u can be decomposed into three components (given appropriate boundary conditions)

 

u = ∇ ×φ + ∇ψ + h

 

 

k-form的插值牵扯到Whitney forms [Bossavit 1998].

 

本文里的Voronoi cell based generalized barycentric interpolation是把Whitney form扩展到dual setting

 

generalized barycentric coordinates have linear accuracy [Barycentric coordinates for convex sets.]

如何离散化物理量:

Velocity as Discrete Flux

Divergence as Net Flux on Tets

Vorticity as Flux Spin

为什么只能这么离散化?其他离散化的方式不行么?不行,因为作者说这种离散化的方式可由代数关系推导得到(section 3


3.1

In the continuous three-dimensional setting,

a 0-form is simply a function on that 3D space.

A 1-form, or line-form, is a quantity that can be evaluated through integration over a

curve. Thus a 1-form can be thought of as a proxy for a vector field, and its integral over a curve becomes the circulation of this vector field.

A 2-form, or area-form, is to be integrated over a surface, that is, it can be viewed as a proxy for a vector perpendicular to that surface (and its evaluation becomes the flux of that vector field through the surface);

a 3-form, or volume-form, is to be integrated over a volume and can be viewed as a proxy for a function.

Classic calculus and vector calculus can then be substituted with a special calculus involving only differential forms, called exterior calculus

就是说,原先计算微积分表达式时,最开始就让‘和坐标系相关的数据”(比如某个vector field)参与计算了,最后求的结果。

现在借助differential form,可以不让‘和坐标系相关的数据”参与计算的情况下来计算微积分表达式。在最后求最终结果(evaluation)的时候,再把‘和坐标系相关的数据”带入进去。这就是 exterior calculus。就是把外围微积分表达式先计算出来,最后带入具体的‘和坐标系相关的数据”从而得出结果。

.>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>

做个类比:

f(x, y) = x+y, g(x, y) = x+2y, 求值f(1, 2)+g(1, 2)


方法1(类比于传统微积分计算方法):

f(1, 2)+g(1, 2)

= x+y|$_{x=1, y=2}$   +   x+2y|$_{x=1, y=2}$

= 1+2                        +   1+2*2                      (从上一步到这一步,叫evaluation。最开始就让‘和坐标系相关的数据”(x=1y=2)参与计算了)

= 3 + 5 = 8;


方法2(类比于exterior calculus计算方法):

f(1, 2)+g(1, 2)

= f(x, y) + g(x, y) | $_{x=1, y=2}$

= x+y    + x+2y    |$_{x=1, y=2}$

= 2x+3y              |$_{x=1, y=2}$   (上面这两步类似于 exterior calculus。只做符号计算,xy的具体值并没有参与计算。 方法2 在无需带入xy的具体值的情况下就可以针对函数做一些处理,从而研究函数。类似,exterior calculus在无需带入‘和坐标系相关的数据”的情况下就可以对n-form做一些处理, 从而研究n-form)

= 2*1+3*2                                     (从上一步到这一步,带入‘和坐标系相关的数据”,叫evaluation)

= 8

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CH 10 Conformal Equivalence of Triangle Meshes

The problem of finding a flat mesh that is discretely conformally equivalent to a given mesh can be solved efficiently by minimizing a convex energy function,。。。

This method can also be used to map a surface mesh to a parameter domain which is flat except for isolated cone singularities, and we show how these can be placed automatically in order to reduce the distortion of the parameterization.

What corresponds to a Riemannian metric and Gaussian curvature in an analogous theory for triangle meshes?

When should two triangle meshes be considered conformally equivalent?

In this paper we present the first algorithm for

mesh parameterization which is based on a definition of discrete

conformal equivalence between triangle meshes which is satisfac-

tory in the sense that (a) it depends only on the geometry of the

meshes and (b) defines an equivalence relation.

关于共形的一些性质:

Meshes in a conformal equivalence class are characterized by length scale factors

associated to the vertices and by conserved quantities: the length cross ratios(下面有解释).

共形等价的定义:

In smooth differential geometry two Riemannian metrics g and g ? on a differentiable 2-manifold M are said to be conformally equivalentif

g ? = e^(2u) g (1)

for some smooth function u : M → R, which gives the logarithm of length change between g and g ? .

.

we define(类比于smooth setting,且it behaves correctly under Möbius transformations(?) of space):

Definition 2.1.

A discrete metricon M is a function l on the set of edges E, assigning to each edge eij a positive number lij so that the triangle inequalities are satisfied for all triangles t$_{ijk}$ ∈ T .

.

Definition 2.2.

Two discrete metrics l and l ? on M are (discretely) conformally equivalentif, for some assignment of numbers ui to the vertices vi , the metrics are related by

l ?ij = e^((ui+uj)/2) lij 2)(定义λij := 2 log lij,则 λ ?ij = λij + ui + uj 3))

this notion of discrete conformal equivalence is indeed an equivalence relation (i.e., it is reflexive, symmetric, and transitive)

We consider two meshes as discretely conformally equivalent if they have the same abstract triangulation(拓扑?) and equivalent edge lengths according to Eq. (2)

Definition 2.3. Given a discrete metric l, we associate with each

interior edge e i j (between t i jk and t jim ) the length cross ratio

c ij := l im /l mj · l jk /l ki

Proposition. Two meshes are discretely conformally equivalent if and only if their length cross ratios are the same.

 

==========================================

CH 11 Discrete Laplace operators

.

Properties of smooth Laplacians:

(NULL ) Δu = 0 whenever u is constant.

(SYM ) Symmetry: (Δu, v) L2 = (u, Δv) L2 whenever u and v are sufficiently smooth and vanish along the boundary of S.

(LOC ) Local support: for any pair p != q of points, Δu(p) is independent of u(q). Altering the function value at a distant point will not affect the action of the Laplacian locally.

(LIN ) Linear precision: Δu = 0 whenever S is part of the Euclidean plane, and u = ax + by + c is a linear function on the plane.

(M AX ) Maximum principle: harmonic functions (those for which Δu = 0 in the interior of S) have no local maxima (or minima) at interior points.

(PSD) Positive semi-definiteness: the Dirichlet energy, E$_D$(u) = ∫s ||grad u||^2 dA, is non-negative. By our choice of sign for Δ, we obtain E$_D$(u) = (Δu, u)L2 ≥ 0 whenever u is sufficiently smooth and vanishes along the boundary of S.

.

作者证明discrete Laplacian 无法同时满足上面的性质

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CH12 Discrete Geometric Mechanics for Variational Time Integrators(解微分方程)

a geometric approach to the problem of time integration.

.

the very essence of a mechanical system is characterized by its symmetries and invariants.Thus preserving these symmetries and invariants (e.g., certain momenta) into the discrete computational setting is of paramount importance if one wants discrete time integration to properly capture the underlying continuous motion

We will show that in fact, one does not have to ask for either predictability or accuracy (类比于测不准原理?)

an introduction to geometric mechanics,。。。we will introduce the notion of variational integrators as a class of solvers specifically designed to preserve this underlying physical structure, even for large time steps

Hamilton’s principle the least action principle):

a dynamical system always finds an optimal course from one position to another(“Nature

is thrifty in all its actions“

A more formal definition will be presented in Section 4.1, but one consequence is that we can recast the

traditional way of thinking about an object accelerating in response to applied forces into a geometric viewpoint.

a geometric viewpointThere, the path followed by the object has optimal geometric properties—analog to the notion of geodesics on curved surfaces。(这是为什么和几何有关)

这个几何观点类似于力学里的牛顿定律,但这个几何观点可适用于E&M和量子力学。

单摆动力学方程:

q‘ = v (2)

v‘ = −g/L sin(q) (3)

离散化方法:

explicit Euler method:

qk+1 = qk + h vk

vk+1 = vk − h g/L sin(qk)


implicit Euler method:

qk+1 = qk + h vk+1

vk+1 = vk − h g/L sin(qk+1)


symplectic Euler method(mix above two methods):

vk+1 = vk − h g/L sin(qk)

qk+1 = qk + h vk+1

These three methods are called finite difference methods

Since q is a path, we cannot simply take a “derivative” with respect to q; instead, we take something called a variation. A variation of the path q is written δq, and can be thought of as an infinitesimal perturbation to the path at each point, with the important property that the perturbation is null at the endpoints of the path.(变分法的思想)

The action functional is then introduced as the integral of L along a path q(t) for time t ∈ [0, T ]:

S(q) ={0, T} L(q, q‘) dt

Hamilton’s principle

the correct path of motion of a dynamical system is such that its action has a stationary value,

Euler-Lagrange equations

∂L/∂q – d/dt (∂L/∂q‘) = 0

in the Hamiltonian formulation, the dynamics are described in phase space, i.e, the current state of a dynamical system is given as a pair (q, p), where q is the state variable, while p is the momentum, defined by p = ∂L/∂q‘

Noether’s theorem

each symmetry of a system leads to a physical invariant (i.e., a conserved quantity)

These symmetries, if respected in the discrete setting, will provide equivalent discrete invariants in time integrators! In fact, we will see that these invariants can be preserved in time integrators at no extra computational cost by simply respecting the geometric, variational nature of dynamics.

应该积分这些invariant,而不是积分速度/加速度之类的量。

Why did some of the phase portraits look better than others? How can we preserve the closedness of the orbits without making the time integrator more complicated?

if one designs a discrete equivalent of the Lagrangian, then discrete equations of motion can be easily

derived from it by paralleling the derivations followed in continuous case. In essence, good numerical methods will come from discrete analogs to the Euler-Lagrange equations—equations that truly derive from a variational principle

.

Discrete Lagrangian:

The main idea is to discretize the least action principle directly rather than discretizing Euler-Lagrange equations.

discrete Lagrangian: Ld (qk, qk+1, h) {tk, tk+1} L(q, q‘)dt

Ld (qk, qk+1, h) = h L( (1−α)qk + αqk+1, (qk+1 − qk)/h ), where α ∈ [0, 1].

For α = 1/2, the quadrature is second-order accurate, while any other value leads to linear accuracy. 这意味着一种对称!但这个对称又意味着什么

discrete Euler-Lagrange (DEL) equations

D1 Ld(qk, qk+1) + D2 Ld(qk−1, qk) = 0 (7)

D1 Ld表示Ld对第一个参数求偏导;

D2 Ld表示Ld对第二个参数求偏导

define the momentum at time tk to be:

pk := D2 Ld(qk−1, qk ) = −D1 Ld(qk , qk+1)


方法1

pk = −D1 Ld (qk , qk+1) ,

pk+1 = D2 Ld (qk , qk+1)

给定(qk , pk),由D1解出qk+1, 再由D2解出pk+1

>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>

方法2

pk = D2 Ld(qk−1, qk )

pk-1 = −D1 Ld (qk-1 , qk)

给定(qk−1, pk-1), D1解出qk, 再由D2解出pk. 和上面的是一样的(只能沿时间正向求解,比如用k-1时刻的量去求k时刻的量, 或用k时刻的量去求k+1时刻的量)


方法3

pk = D2 Ld(qk−1, qk )

pk = −D1 Ld (qk , qk+1)

给定(qk−1, pk-1), (qk, pk),只能求出qk+1, 但是pk+1怎么求?只能再增加一个方程:

pk+1 = D2 Ld(qk, qk+1)

所以方法3远不如方法1好。因为不仅要用到k-1k时刻的数据,还需要计算3个方程。

<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<

Variational integrators 。。。has two important consequences.

First, the integrators are guaranteed to be symplectic, which in practice will result in excellent energy behavior, rather than perpetual damping or blowing up.

Second, they are also guaranteed to preserve discrete momenta of the system (via a discrete version of Noether’s theorem)


--------------------------------------

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O’B RIEN , J. F. 2006. Fluid animation with dynamic meshes.

 

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see also [Nicolaides and Wu 1997] for a similar setup for Div-Curl equations

 

mesh parameterization:
Floater, M. S., and Hormann, K. 2005. Surface Parameterization: a Tutorial and Survey
Sheffer, A., Praun, E., and Rose, K. 2006. Mesh Parameterization Methods and their Applications

 -----------------------吐糟分割线----------------------------
stam的stable fulid是一个巨大的进步,后来很多人在这个基础上针对各种不足各种擦屁股。
图形学上那些引以为傲的数据结构(空间划分,adaptive划分等等)实际上都是在没有找到更准确的数学结构的情况下而采用的变通方法。说白了就是擦屁股,难怪搞数学的人瞧不起搞计算机的人。

什么是计算数学?
搞数学的M发现新出来的一些数学概念是很不错的东东,如果能编程实现的话也许能促进其他学科发展。于是M去找搞计算机的C,希望C能把它实现出来。C看了看这些新概念,想不出这些东东在计算机学科里能有神马用,最终拒绝了M。M一气之下自己来搞。慢慢地这竟然形成了数学的一个分支----计算数学。

Discrete.Differential.Geometry-An.Applied.Introduction(sig2008)笔记

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