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Liviu Nicolaescu
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In many variational problems one is given an action functional $f\mapsto S[f]$, described by an integral

$$ S[f]=\int_\Omega L\bigl(\;x,f(x),D f(x),\dotsc, D^k f(x)\;\bigr) dx $$

in which

  • $\Omega$ is a region in some Euclidean space $\mathbb{R}^n$, $x\in\Omega$,
  • $f$ is a $k$-times differentiable function $f: \Omega\to\mathbb{R}^m$, and
  • the Lagrangian $L$ is a function of the appropriate number of variables.

For example, in classical mechanics $n=1$, $\Omega\subset \mathbb{R}$ is an interval and the function

$$f:\Omega\to \mathbb{R}^m, \;\;\Omega\ni t\mapsto f(t)\in\mathbb{R}^m$$

describes a path in $\mathbb{R}^m$. The Lagrangian is a the functionLagrangia has the form $L: \mathbb{R}^m\times\mathbb{R}^m\to \mathbb{R}$, $\newcommand{\bR}{\mathbb{R}}$

$$L(y,v)=\frac{1}{2}|v|^2-U(y), \;\; (y,v)\in\bR^m\times\bR^m $$

where the potential $U$ is a function $U:\bR^m\to\bR$. Then

$$ L(f,\dot{f})= \frac{1}{2}|\dot{f}|^2-U(f), $$

where the dot indicates the derivative with respect to the time parameter $t$ on $\Omega\subset\mathbb{R}$.

The functional (or variational) derivative of $S$ calculated at $f_0:\Omega\to\mathbb{R}^m$ is a gadget $\delta S[f_0]$ that feeds on an infinitesimal deformation $\delta f$ of $f_0$ and returns a scalar

$$ \langle \delta S[f_0], \delta f\rangle =\lim_{h\to 0}\frac{1}{h} \bigl(S[f_0+h\delta f]-S[f_0]\;\bigr). \tag{1}$$

The deformation $\delta f$ is also a function $\Omega\to\mathbb{R}^m$. It is often desirable to identify $\delta S[f_0]$ with a function $g:\Omega\to\mathbb{R}^m$ which, if it exists, is uniquely determined by the equality

$$ \langle \delta S[f_0], \delta f\rangle=\langle g(x), \delta f(x)\rangle =\int_\Omega \bigl( g(x), \delta f(x) \bigr) dx,\tag{2} $$

where $(-,-)$ denotes the natural inner product on $\mathbb{R}^m$. The value of $g$ at $x_0$ can be obtained from the equality

$$ g(x_0)= \langle g(x), \delta(x-x_0)\rangle. \tag{3} $$

This means that the value of $g$ at $x_0$ is obtained by formally replacing $\delta f$ with $\delta(y-x_0)$ in (2).

Making the same formal replacement $\delta f(x)\to\delta(x-x_0)$ in (1) one obtains the physicists' functional derivative in your question.

How does one identify $\delta S[f_0]$ with a function? In the example from classical mechanics one has

$$ S[f_0](t)=-\frac{d}{dt}\frac{\partial L}{\partial v}(f_0(t), \dot{f_0}(t))+\frac{\partial L}{\partial y}(f_0,\dot{f}_0). $$

How can one see this? Fix a function (path) $f_0=f_0(t)$. For simplicity set $\alpha:=\delta f$ and assume $\Omega=[0,1]$. We have a Taylor approximation

$$ L(f_0+h \alpha, \dot{f}_0+h\dot{\alpha}) = L(f_0,\dot{f}_0)+ h\frac{\partial L}{\partial y}(f_0,\dot{f_0})\alpha+h\frac{\partial L}{\partial v}(f_0,\dot{f_0})\dot{\alpha} +O(h^2). $$

Hence $$\frac{1}{h} \bigl(\; S[f_0+h\alpha]-S[f_0]\;\bigr)=\int_0^1 \frac{\partial L}{\partial y}(f_0,\dot{f_0})\alpha+\frac{\partial L}{\partial v}(f_0,\dot{f_0})\dot \alpha dt +O(h). $$

Letting $h\to 0$ we deduce

$$\langle \delta S[f_0],\alpha\rangle = \int_0^1\frac{\partial L}{\partial y}(f_0,\dot{f_0})\alpha+\frac{\partial L}{\partial v}(f_0,\dot{f_0})\dot{\alpha} dt. $$

If we further assume that $\alpha(0)=\alpha(1)$ then upon integrating by parts we deduce

$$ \langle \delta S[f_0],\alpha\rangle=\int_0^1\Bigl(\frac{\partial L}{\partial y}(f_0,\dot{f_0}) -\frac{d}{dt}\frac{\partial L}{\partial v}(f_0,\dot{f_0})\Bigr) \alpha dt. $$

A good place to look for more details is the book "Calculus of Variations" by Gelfand and Fomin, Dover 2000.

In many variational problems one is given an action functional $f\mapsto S[f]$, described by an integral

$$ S[f]=\int_\Omega L\bigl(\;x,f(x),D f(x),\dotsc, D^k f(x)\;\bigr) dx $$

in which

  • $\Omega$ is a region in some Euclidean space $\mathbb{R}^n$, $x\in\Omega$,
  • $f$ is a $k$-times differentiable function $f: \Omega\to\mathbb{R}^m$, and
  • the Lagrangian $L$ is a function of the appropriate number of variables.

For example, in classical mechanics $n=1$, $\Omega\subset \mathbb{R}$ is an interval and the function

$$f:\Omega\to \mathbb{R}^m, \;\;\Omega\ni t\mapsto f(t)\in\mathbb{R}^m$$

describes a path in $\mathbb{R}^m$. The Lagrangian is a the function has the form $L: \mathbb{R}^m\times\mathbb{R}^m\to \mathbb{R}$, $\newcommand{\bR}{\mathbb{R}}$

$$L(y,v)=\frac{1}{2}|v|^2-U(y), \;\; (y,v)\in\bR^m\times\bR^m $$

where the potential $U$ is a function $U:\bR^m\to\bR$. Then

$$ L(f,\dot{f})= \frac{1}{2}|\dot{f}|^2-U(f), $$

where the dot indicates the derivative with respect to the time parameter $t$ on $\Omega\subset\mathbb{R}$.

The functional (or variational) derivative of $S$ calculated at $f_0:\Omega\to\mathbb{R}^m$ is a gadget $\delta S[f_0]$ that feeds on an infinitesimal deformation $\delta f$ of $f_0$ and returns a scalar

$$ \langle \delta S[f_0], \delta f\rangle =\lim_{h\to 0}\frac{1}{h} \bigl(S[f_0+h\delta f]-S[f_0]\;\bigr). \tag{1}$$

The deformation $\delta f$ is also a function $\Omega\to\mathbb{R}^m$. It is often desirable to identify $\delta S[f_0]$ with a function $g:\Omega\to\mathbb{R}^m$ which, if it exists, is uniquely determined by the equality

$$ \langle \delta S[f_0], \delta f\rangle=\langle g(x), \delta f(x)\rangle =\int_\Omega \bigl( g(x), \delta f(x) \bigr) dx,\tag{2} $$

where $(-,-)$ denotes the natural inner product on $\mathbb{R}^m$. The value of $g$ at $x_0$ can be obtained from the equality

$$ g(x_0)= \langle g(x), \delta(x-x_0)\rangle. \tag{3} $$

This means that the value of $g$ at $x_0$ is obtained by formally replacing $\delta f$ with $\delta(y-x_0)$ in (2).

Making the same formal replacement $\delta f(x)\to\delta(x-x_0)$ in (1) one obtains the physicists' functional derivative in your question.

How does one identify $\delta S[f_0]$ with a function? In the example from classical mechanics one has

$$ S[f_0](t)=-\frac{d}{dt}\frac{\partial L}{\partial v}(f_0(t), \dot{f_0}(t))+\frac{\partial L}{\partial y}(f_0,\dot{f}_0). $$

How can one see this? Fix a function (path) $f_0=f_0(t)$. For simplicity set $\alpha:=\delta f$ and assume $\Omega=[0,1]$. We have a Taylor approximation

$$ L(f_0+h \alpha, \dot{f}_0+h\dot{\alpha}) = L(f_0,\dot{f}_0)+ h\frac{\partial L}{\partial y}(f_0,\dot{f_0})\alpha+h\frac{\partial L}{\partial v}(f_0,\dot{f_0})\dot{\alpha} +O(h^2). $$

Hence $$\frac{1}{h} \bigl(\; S[f_0+h\alpha]-S[f_0]\;\bigr)=\int_0^1 \frac{\partial L}{\partial y}(f_0,\dot{f_0})\alpha+\frac{\partial L}{\partial v}(f_0,\dot{f_0})\dot \alpha dt +O(h). $$

Letting $h\to 0$ we deduce

$$\langle \delta S[f_0],\alpha\rangle = \int_0^1\frac{\partial L}{\partial y}(f_0,\dot{f_0})\alpha+\frac{\partial L}{\partial v}(f_0,\dot{f_0})\dot{\alpha} dt. $$

If we further assume that $\alpha(0)=\alpha(1)$ then upon integrating by parts we deduce

$$ \langle \delta S[f_0],\alpha\rangle=\int_0^1\Bigl(\frac{\partial L}{\partial y}(f_0,\dot{f_0}) -\frac{d}{dt}\frac{\partial L}{\partial v}(f_0,\dot{f_0})\Bigr) \alpha dt. $$

A good place to look for more details is the book "Calculus of Variations" by Gelfand and Fomin, Dover 2000.

In many variational problems one is given an action functional $f\mapsto S[f]$, described by an integral

$$ S[f]=\int_\Omega L\bigl(\;x,f(x),D f(x),\dotsc, D^k f(x)\;\bigr) dx $$

in which

  • $\Omega$ is a region in some Euclidean space $\mathbb{R}^n$, $x\in\Omega$,
  • $f$ is a $k$-times differentiable function $f: \Omega\to\mathbb{R}^m$, and
  • the Lagrangian $L$ is a function of the appropriate number of variables.

For example, in classical mechanics $n=1$, $\Omega\subset \mathbb{R}$ is an interval and the function

$$f:\Omega\to \mathbb{R}^m, \;\;\Omega\ni t\mapsto f(t)\in\mathbb{R}^m$$

describes a path in $\mathbb{R}^m$. The Lagrangia has the form $L: \mathbb{R}^m\times\mathbb{R}^m\to \mathbb{R}$, $\newcommand{\bR}{\mathbb{R}}$

$$L(y,v)=\frac{1}{2}|v|^2-U(y), \;\; (y,v)\in\bR^m\times\bR^m $$

where the potential $U$ is a function $U:\bR^m\to\bR$. Then

$$ L(f,\dot{f})= \frac{1}{2}|\dot{f}|^2-U(f), $$

where the dot indicates the derivative with respect to the time parameter $t$ on $\Omega\subset\mathbb{R}$.

The functional (or variational) derivative of $S$ calculated at $f_0:\Omega\to\mathbb{R}^m$ is a gadget $\delta S[f_0]$ that feeds on an infinitesimal deformation $\delta f$ of $f_0$ and returns a scalar

$$ \langle \delta S[f_0], \delta f\rangle =\lim_{h\to 0}\frac{1}{h} \bigl(S[f_0+h\delta f]-S[f_0]\;\bigr). \tag{1}$$

The deformation $\delta f$ is also a function $\Omega\to\mathbb{R}^m$. It is often desirable to identify $\delta S[f_0]$ with a function $g:\Omega\to\mathbb{R}^m$ which, if it exists, is uniquely determined by the equality

$$ \langle \delta S[f_0], \delta f\rangle=\langle g(x), \delta f(x)\rangle =\int_\Omega \bigl( g(x), \delta f(x) \bigr) dx,\tag{2} $$

where $(-,-)$ denotes the natural inner product on $\mathbb{R}^m$. The value of $g$ at $x_0$ can be obtained from the equality

$$ g(x_0)= \langle g(x), \delta(x-x_0)\rangle. \tag{3} $$

This means that the value of $g$ at $x_0$ is obtained by formally replacing $\delta f$ with $\delta(y-x_0)$ in (2).

Making the same formal replacement $\delta f(x)\to\delta(x-x_0)$ in (1) one obtains the physicists' functional derivative in your question.

How does one identify $\delta S[f_0]$ with a function? In the example from classical mechanics one has

$$ S[f_0](t)=-\frac{d}{dt}\frac{\partial L}{\partial v}(f_0(t), \dot{f_0}(t))+\frac{\partial L}{\partial y}(f_0,\dot{f}_0). $$

How can one see this? Fix a function (path) $f_0=f_0(t)$. For simplicity set $\alpha:=\delta f$ and assume $\Omega=[0,1]$. We have a Taylor approximation

$$ L(f_0+h \alpha, \dot{f}_0+h\dot{\alpha}) = L(f_0,\dot{f}_0)+ h\frac{\partial L}{\partial y}(f_0,\dot{f_0})\alpha+h\frac{\partial L}{\partial v}(f_0,\dot{f_0})\dot{\alpha} +O(h^2). $$

Hence $$\frac{1}{h} \bigl(\; S[f_0+h\alpha]-S[f_0]\;\bigr)=\int_0^1 \frac{\partial L}{\partial y}(f_0,\dot{f_0})\alpha+\frac{\partial L}{\partial v}(f_0,\dot{f_0})\dot \alpha dt +O(h). $$

Letting $h\to 0$ we deduce

$$\langle \delta S[f_0],\alpha\rangle = \int_0^1\frac{\partial L}{\partial y}(f_0,\dot{f_0})\alpha+\frac{\partial L}{\partial v}(f_0,\dot{f_0})\dot{\alpha} dt. $$

If we further assume that $\alpha(0)=\alpha(1)$ then upon integrating by parts we deduce

$$ \langle \delta S[f_0],\alpha\rangle=\int_0^1\Bigl(\frac{\partial L}{\partial y}(f_0,\dot{f_0}) -\frac{d}{dt}\frac{\partial L}{\partial v}(f_0,\dot{f_0})\Bigr) \alpha dt. $$

A good place to look for more details is the book "Calculus of Variations" by Gelfand and Fomin, Dover 2000.

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Source Link
Liviu Nicolaescu
  • 34.7k
  • 2
  • 91
  • 165

In many variational problems one is given an action functional $f\mapsto S[f]$, described by an integral

$$ S[f]=\int_\Omega L\bigl(\;x,f(x),D f(x),\dotsc, D^k f(x)\;\bigr) dx $$

in which

  • $\Omega$ is a region in some Euclidean space $\mathbb{R}^n$, $x\in\Omega$,
  • $f$ is a $k$-times differentiable function $f: \Omega\to\mathbb{R}^m$, and
  • the Lagrangian $L$ is a function of the appropriate number of variables.

For example, in classical mechanics $n=1$, $\Omega\subset \mathbb{R}$ is an interval and the function

$$f:\Omega\to \mathbb{R}^m, \;\;\Omega\ni t\mapsto f(t)\in\mathbb{R}^m$$

describes a path in $\mathbb{R}^m$. The Lagrangian is a the function has the form $L: \mathbb{R}^m\times\mathbb{R}^m\to \mathbb{R}$, $\newcommand{\bR}{\mathbb{R}}$

$$L(y,v)=\frac{1}{2}|v|^2-U(y), \;\; (y,v)\in\bR^m\times\bR^m $$

where the potential $U$ is a function $U:\bR^m\to\bR$. Then

$$ L(f,\dot{f})= \frac{1}{2}|\dot{f}|^2-U(f), $$

where the dot indicates the derivative with respect to the time parameter $t$ on $\Omega\subset\mathbb{R}$.

The functional (or variational) derivative of $S$ calculated at $f_0:\Omega\to\mathbb{R}^m$ is a gadget $\delta S[f_0]$ that feeds on an infinitesimal deformation $\delta f$ of $f_0$ and returns a scalar

$$ \langle \delta S[f_0], \delta f\rangle =\lim_{h\to 0}\frac{1}{h} \bigl(S[f_0+h\delta f]-S[f_0]\;\bigr). \tag{1}$$

The deformation $\delta f$ is also a function $\Omega\to\mathbb{R}^m$. It is often desirable to identify $\delta S[f_0]$ with a function $g:\Omega\to\mathbb{R}^m$ which, if it exists, is uniquely determined by the equality

$$ \langle \delta S[f_0], \delta f\rangle=\langle g(x), \delta f(x)\rangle =\int_\Omega \bigl( g(x), \delta f(x) \bigr) dx,\tag{2} $$

where $(-,-)$ denotes the natural inner product on $\mathbb{R}^m$. The value of $g$ at $x_0$ can be obtained from the equality

$$ g(x_0)= \langle g(x), \delta(x-x_0)\rangle. \tag{3} $$

This means that the value of $g$ at $x_0$ is obtained by formally replacing $\delta f$ with $\delta(y-x_0)$ in (2).

Making the same formal replacement $\delta f(x)\to\delta(x-x_0)$ in (1) one obtains the physicists' functional derivative in your question.

How does one identify $\delta S[f_0]$ with a function? In the example from classical mechanics one has

$$ S[f_0](t)=\frac{d}{dt}\frac{\partial L}{\partial v}(f_0(t), \dot{f_0}(t))-\frac{\partial L}{\partial x}(f_0,\dot{f}_0). $$$$ S[f_0](t)=-\frac{d}{dt}\frac{\partial L}{\partial v}(f_0(t), \dot{f_0}(t))+\frac{\partial L}{\partial y}(f_0,\dot{f}_0). $$

How can one see this? Fix a function (path) $f_0=f_0(t)$. For simplicity set $\alpha:=\delta f$ and assume $\Omega=[0,1]$. We have a Taylor approximation

$$ L(f_0+h \alpha, \dot{f}_0+h\dot{\alpha}) = L(f_0,\dot{f}_0)+ h\frac{\partial L}{\partial y}(f_0,\dot{f_0})\alpha+h\frac{\partial L}{\partial v}(f_0,\dot{f_0})\dot{\alpha} +O(h^2). $$

Hence $$\frac{1}{h} \bigl(\; S[f_0+h\alpha]-S[f_0]\;\bigr)=\int_0^1 \frac{\partial L}{\partial y}(f_0,\dot{f_0})\alpha+\frac{\partial L}{\partial v}(f_0,\dot{f_0})\dot \alpha dt +O(h). $$

Letting $h\to 0$ we deduce

$$\langle \delta S[f_0],\alpha\rangle = \int_0^1\frac{\partial L}{\partial y}(f_0,\dot{f_0})\alpha+\frac{\partial L}{\partial v}(f_0,\dot{f_0})\dot{\alpha} dt. $$

If we further assume that $\alpha(0)=\alpha(1)$ then upon integrating by parts we deduce

$$ \langle \delta S[f_0],\alpha\rangle=\int_0^1\Bigl(\frac{\partial L}{\partial y}(f_0,\dot{f_0}) -\frac{d}{dt}\frac{\partial L}{\partial v}(f_0,\dot{f_0})\Bigr) \alpha dt. $$

A good place to look for more details is the book "Calculus of Variations" by Gelfand and Fomin, Dover 2000.

In many variational problems one is given an action functional $f\mapsto S[f]$, described by an integral

$$ S[f]=\int_\Omega L\bigl(\;x,f(x),D f(x),\dotsc, D^k f(x)\;\bigr) dx $$

in which

  • $\Omega$ is a region in some Euclidean space $\mathbb{R}^n$, $x\in\Omega$,
  • $f$ is a $k$-times differentiable function $f: \Omega\to\mathbb{R}^m$, and
  • the Lagrangian $L$ is a function of the appropriate number of variables.

For example, in classical mechanics $n=1$, $\Omega\subset \mathbb{R}$ is an interval and the function

$$f:\Omega\to \mathbb{R}^m, \;\;\Omega\ni t\mapsto f(t)\in\mathbb{R}^m$$

describes a path in $\mathbb{R}^m$. The Lagrangian is a the function has the form $L: \mathbb{R}^m\times\mathbb{R}^m\to \mathbb{R}$, $\newcommand{\bR}{\mathbb{R}}$

$$L(y,v)=\frac{1}{2}|v|^2-U(y), \;\; (y,v)\in\bR^m\times\bR^m $$

where the potential $U$ is a function $U:\bR^m\to\bR$. Then

$$ L(f,\dot{f})= \frac{1}{2}|\dot{f}|^2-U(f), $$

where the dot indicates the derivative with respect to the time parameter $t$ on $\Omega\subset\mathbb{R}$.

The functional (or variational) derivative of $S$ calculated at $f_0:\Omega\to\mathbb{R}^m$ is a gadget $\delta S[f_0]$ that feeds on an infinitesimal deformation $\delta f$ of $f_0$ and returns a scalar

$$ \langle \delta S[f_0], \delta f\rangle =\lim_{h\to 0}\frac{1}{h} \bigl(S[f_0+h\delta f]-S[f_0]\;\bigr). \tag{1}$$

The deformation $\delta f$ is also a function $\Omega\to\mathbb{R}^m$. It is often desirable to identify $\delta S[f_0]$ with a function $g:\Omega\to\mathbb{R}^m$ which, if it exists, is uniquely determined by the equality

$$ \langle \delta S[f_0], \delta f\rangle=\langle g(x), \delta f(x)\rangle =\int_\Omega \bigl( g(x), \delta f(x) \bigr) dx,\tag{2} $$

where $(-,-)$ denotes the natural inner product on $\mathbb{R}^m$. The value of $g$ at $x_0$ can be obtained from the equality

$$ g(x_0)= \langle g(x), \delta(x-x_0)\rangle. \tag{3} $$

This means that the value of $g$ at $x_0$ is obtained by formally replacing $\delta f$ with $\delta(y-x_0)$ in (2).

Making the same formal replacement $\delta f(x)\to\delta(x-x_0)$ in (1) one obtains the physicists' functional derivative in your question.

How does one identify $\delta S[f_0]$ with a function? In the example from classical mechanics one has

$$ S[f_0](t)=\frac{d}{dt}\frac{\partial L}{\partial v}(f_0(t), \dot{f_0}(t))-\frac{\partial L}{\partial x}(f_0,\dot{f}_0). $$

A good place to look for more details is the book "Calculus of Variations" by Gelfand and Fomin, Dover 2000.

In many variational problems one is given an action functional $f\mapsto S[f]$, described by an integral

$$ S[f]=\int_\Omega L\bigl(\;x,f(x),D f(x),\dotsc, D^k f(x)\;\bigr) dx $$

in which

  • $\Omega$ is a region in some Euclidean space $\mathbb{R}^n$, $x\in\Omega$,
  • $f$ is a $k$-times differentiable function $f: \Omega\to\mathbb{R}^m$, and
  • the Lagrangian $L$ is a function of the appropriate number of variables.

For example, in classical mechanics $n=1$, $\Omega\subset \mathbb{R}$ is an interval and the function

$$f:\Omega\to \mathbb{R}^m, \;\;\Omega\ni t\mapsto f(t)\in\mathbb{R}^m$$

describes a path in $\mathbb{R}^m$. The Lagrangian is a the function has the form $L: \mathbb{R}^m\times\mathbb{R}^m\to \mathbb{R}$, $\newcommand{\bR}{\mathbb{R}}$

$$L(y,v)=\frac{1}{2}|v|^2-U(y), \;\; (y,v)\in\bR^m\times\bR^m $$

where the potential $U$ is a function $U:\bR^m\to\bR$. Then

$$ L(f,\dot{f})= \frac{1}{2}|\dot{f}|^2-U(f), $$

where the dot indicates the derivative with respect to the time parameter $t$ on $\Omega\subset\mathbb{R}$.

The functional (or variational) derivative of $S$ calculated at $f_0:\Omega\to\mathbb{R}^m$ is a gadget $\delta S[f_0]$ that feeds on an infinitesimal deformation $\delta f$ of $f_0$ and returns a scalar

$$ \langle \delta S[f_0], \delta f\rangle =\lim_{h\to 0}\frac{1}{h} \bigl(S[f_0+h\delta f]-S[f_0]\;\bigr). \tag{1}$$

The deformation $\delta f$ is also a function $\Omega\to\mathbb{R}^m$. It is often desirable to identify $\delta S[f_0]$ with a function $g:\Omega\to\mathbb{R}^m$ which, if it exists, is uniquely determined by the equality

$$ \langle \delta S[f_0], \delta f\rangle=\langle g(x), \delta f(x)\rangle =\int_\Omega \bigl( g(x), \delta f(x) \bigr) dx,\tag{2} $$

where $(-,-)$ denotes the natural inner product on $\mathbb{R}^m$. The value of $g$ at $x_0$ can be obtained from the equality

$$ g(x_0)= \langle g(x), \delta(x-x_0)\rangle. \tag{3} $$

This means that the value of $g$ at $x_0$ is obtained by formally replacing $\delta f$ with $\delta(y-x_0)$ in (2).

Making the same formal replacement $\delta f(x)\to\delta(x-x_0)$ in (1) one obtains the physicists' functional derivative in your question.

How does one identify $\delta S[f_0]$ with a function? In the example from classical mechanics one has

$$ S[f_0](t)=-\frac{d}{dt}\frac{\partial L}{\partial v}(f_0(t), \dot{f_0}(t))+\frac{\partial L}{\partial y}(f_0,\dot{f}_0). $$

How can one see this? Fix a function (path) $f_0=f_0(t)$. For simplicity set $\alpha:=\delta f$ and assume $\Omega=[0,1]$. We have a Taylor approximation

$$ L(f_0+h \alpha, \dot{f}_0+h\dot{\alpha}) = L(f_0,\dot{f}_0)+ h\frac{\partial L}{\partial y}(f_0,\dot{f_0})\alpha+h\frac{\partial L}{\partial v}(f_0,\dot{f_0})\dot{\alpha} +O(h^2). $$

Hence $$\frac{1}{h} \bigl(\; S[f_0+h\alpha]-S[f_0]\;\bigr)=\int_0^1 \frac{\partial L}{\partial y}(f_0,\dot{f_0})\alpha+\frac{\partial L}{\partial v}(f_0,\dot{f_0})\dot \alpha dt +O(h). $$

Letting $h\to 0$ we deduce

$$\langle \delta S[f_0],\alpha\rangle = \int_0^1\frac{\partial L}{\partial y}(f_0,\dot{f_0})\alpha+\frac{\partial L}{\partial v}(f_0,\dot{f_0})\dot{\alpha} dt. $$

If we further assume that $\alpha(0)=\alpha(1)$ then upon integrating by parts we deduce

$$ \langle \delta S[f_0],\alpha\rangle=\int_0^1\Bigl(\frac{\partial L}{\partial y}(f_0,\dot{f_0}) -\frac{d}{dt}\frac{\partial L}{\partial v}(f_0,\dot{f_0})\Bigr) \alpha dt. $$

A good place to look for more details is the book "Calculus of Variations" by Gelfand and Fomin, Dover 2000.

An extra backslash was spoiling the rendering, creating red text
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In many variational problems one is given an action functional $f\mapsto S[f]$, where describeddescribed by an integral

$$ S[f]=\int_\Omega L\bigl(\;x,f(x),D f(x),\dotsc, D^k f(x)\;\bigr) dx $$

in which

  • $\Omega$ is a region in some Euclidean space $\mathbb{R}^n$, $x\in\Omega$,
  • $f$ is a $k$-times differentiable function $f: \Omega\to\mathbb{R}^m$, and
  • the Lagrangian $L$ is a function of the appropriate number of variables.

For example, in classical mechanics $n=1$, $\Omega\subset\bR$$\Omega\subset \mathbb{R}$ is an interval and the function

$$f:\Omega\to \mathbb{R}^m, \;\;\Omega\ni t\mapsto f(t)\in\mathbb{R}^m$$

describes a path in $\mathbb{R}^m$. The Lagrangian is a the function has the form $L: \mathbb{R}^m\times\mathbb{R}^m\to \mathbb{R}$, $\newcommand{\bR}{\mathbb{R}}$

$$L(y,v)=\frac{1}{2}|v|^2-U(y), \;\; (y,v)\in\bR^m\times\bR^m $$

where the potential $U$ is a function $U:\bR^m\to\bR$. Then

$$ L(f,\dot{f})= \frac{1}{2}|\dot{f}|^2-U(f), $$

where the dot indicates the derivative with respect to the time parameter $t$ on $\Omega\subset\mathbb{R}$.

The functional (or variational) derivative of $S$ calculated at $f_0:\Omega\to\mathbb{R}^m$ is a gadget $\delta S[f_0]$ that feeds on an infinitesimal deformation $\delta f$ of $f_0$ and returns a scalar

$$ \langle \delta S[f_0], \delta f\rangle =\lim_{h\to 0}\frac{1}{h} \bigl(S[f_0+h\delta f]-S[f_0]\;\bigr). \tag{1}$$

The deformation $\delta f$ is also a function $\Omega\to\mathbb{R}^m$. It is often desirable to identify $\delta S[f_0]$ with a function $g:\Omega\to\mathbb{R}^m$ which, if it exists, is uniquely determined by the equality

$$ \langle \delta S[f_0], \delta f\rangle=\langle g(x), \delta f(x)\rangle =\int_\Omega \bigl( g(x), \delta f(x) \bigr) dx,\tag{2} $$

where $(-,-)$ denotes the natural inner product on $\mathbb{R}^m$. The value of $g$ at $x_0$ can be obtained from the equality

$$ g(x_0)= \langle g(x), \delta(x-x_0)\rangle. \tag{3} $$

This means that the value of $g$ at $x_0$ is obtained by formally replacing $\delta f$ with $\delta(y-x_0)$ in (2).

Making the same formal replacement $\delta f(x)\to\delta(x-x_0)$ in (1) one obtains the physicists' functional derivative in your question.

How does one identify $\delta S[f_0]$ with a function? In the example from classical mechanics one has

$$ S[f_0](t)=\frac{d}{dt}\frac{\partial L}{\partial v}(f_0(t), \dot{f_0}(t))-\frac{\partial L}{\partial x}(f_0,\dot{f}_0). $$

A good place to look for more details is the book "Calculus of Variations" by Gelfand and Fomin,Dover Dover 2000.

In many variational problems one is given an action functional $f\mapsto S[f]$, where described by an integral

$$ S[f]=\int_\Omega L\bigl(\;x,f(x),D f(x),\dotsc, D^k f(x)\;\bigr) dx $$

in which

  • $\Omega$ is a region in some Euclidean space $\mathbb{R}^n$, $x\in\Omega$,
  • $f$ is a $k$-times differentiable function $f: \Omega\to\mathbb{R}^m$, and
  • the Lagrangian $L$ is a function of the appropriate number of variables.

For example, in classical mechanics $n=1$, $\Omega\subset\bR$ is an interval and the function

$$f:\Omega\to \mathbb{R}^m, \;\;\Omega\ni t\mapsto f(t)\in\mathbb{R}^m$$

describes a path in $\mathbb{R}^m$. The Lagrangian is a the function has the form $L: \mathbb{R}^m\times\mathbb{R}^m\to \mathbb{R}$, $\newcommand{\bR}{\mathbb{R}}$

$$L(y,v)=\frac{1}{2}|v|^2-U(y), \;\; (y,v)\in\bR^m\times\bR^m $$

where the potential $U$ is a function $U:\bR^m\to\bR$. Then

$$ L(f,\dot{f})= \frac{1}{2}|\dot{f}|^2-U(f), $$

where the dot indicates the derivative with respect to the time parameter $t$ on $\Omega\subset\mathbb{R}$.

The functional (or variational) derivative of $S$ calculated at $f_0:\Omega\to\mathbb{R}^m$ is a gadget $\delta S[f_0]$ that feeds on an infinitesimal deformation $\delta f$ of $f_0$ and returns a scalar

$$ \langle \delta S[f_0], \delta f\rangle =\lim_{h\to 0}\frac{1}{h} \bigl(S[f_0+h\delta f]-S[f_0]\;\bigr). \tag{1}$$

The deformation $\delta f$ is also a function $\Omega\to\mathbb{R}^m$. It is often desirable to identify $\delta S[f_0]$ with a function $g:\Omega\to\mathbb{R}^m$ which, if it exists, is uniquely determined by the equality

$$ \langle \delta S[f_0], \delta f\rangle=\langle g(x), \delta f(x)\rangle =\int_\Omega \bigl( g(x), \delta f(x) \bigr) dx,\tag{2} $$

where $(-,-)$ denotes the natural inner product on $\mathbb{R}^m$. The value of $g$ at $x_0$ can be obtained from the equality

$$ g(x_0)= \langle g(x), \delta(x-x_0)\rangle. \tag{3} $$

This means that the value of $g$ at $x_0$ is obtained by formally replacing $\delta f$ with $\delta(y-x_0)$ in (2).

Making the same formal replacement $\delta f(x)\to\delta(x-x_0)$ in (1) one obtains the physicists' functional derivative in your question.

How does one identify $\delta S[f_0]$ with a function? In the example from classical mechanics one has

$$ S[f_0](t)=\frac{d}{dt}\frac{\partial L}{\partial v}(f_0(t), \dot{f_0}(t))-\frac{\partial L}{\partial x}(f_0,\dot{f}_0). $$

A good place to look for more details is the book "Calculus of Variations" by Gelfand and Fomin,Dover 2000.

In many variational problems one is given an action functional $f\mapsto S[f]$, described by an integral

$$ S[f]=\int_\Omega L\bigl(\;x,f(x),D f(x),\dotsc, D^k f(x)\;\bigr) dx $$

in which

  • $\Omega$ is a region in some Euclidean space $\mathbb{R}^n$, $x\in\Omega$,
  • $f$ is a $k$-times differentiable function $f: \Omega\to\mathbb{R}^m$, and
  • the Lagrangian $L$ is a function of the appropriate number of variables.

For example, in classical mechanics $n=1$, $\Omega\subset \mathbb{R}$ is an interval and the function

$$f:\Omega\to \mathbb{R}^m, \;\;\Omega\ni t\mapsto f(t)\in\mathbb{R}^m$$

describes a path in $\mathbb{R}^m$. The Lagrangian is a the function has the form $L: \mathbb{R}^m\times\mathbb{R}^m\to \mathbb{R}$, $\newcommand{\bR}{\mathbb{R}}$

$$L(y,v)=\frac{1}{2}|v|^2-U(y), \;\; (y,v)\in\bR^m\times\bR^m $$

where the potential $U$ is a function $U:\bR^m\to\bR$. Then

$$ L(f,\dot{f})= \frac{1}{2}|\dot{f}|^2-U(f), $$

where the dot indicates the derivative with respect to the time parameter $t$ on $\Omega\subset\mathbb{R}$.

The functional (or variational) derivative of $S$ calculated at $f_0:\Omega\to\mathbb{R}^m$ is a gadget $\delta S[f_0]$ that feeds on an infinitesimal deformation $\delta f$ of $f_0$ and returns a scalar

$$ \langle \delta S[f_0], \delta f\rangle =\lim_{h\to 0}\frac{1}{h} \bigl(S[f_0+h\delta f]-S[f_0]\;\bigr). \tag{1}$$

The deformation $\delta f$ is also a function $\Omega\to\mathbb{R}^m$. It is often desirable to identify $\delta S[f_0]$ with a function $g:\Omega\to\mathbb{R}^m$ which, if it exists, is uniquely determined by the equality

$$ \langle \delta S[f_0], \delta f\rangle=\langle g(x), \delta f(x)\rangle =\int_\Omega \bigl( g(x), \delta f(x) \bigr) dx,\tag{2} $$

where $(-,-)$ denotes the natural inner product on $\mathbb{R}^m$. The value of $g$ at $x_0$ can be obtained from the equality

$$ g(x_0)= \langle g(x), \delta(x-x_0)\rangle. \tag{3} $$

This means that the value of $g$ at $x_0$ is obtained by formally replacing $\delta f$ with $\delta(y-x_0)$ in (2).

Making the same formal replacement $\delta f(x)\to\delta(x-x_0)$ in (1) one obtains the physicists' functional derivative in your question.

How does one identify $\delta S[f_0]$ with a function? In the example from classical mechanics one has

$$ S[f_0](t)=\frac{d}{dt}\frac{\partial L}{\partial v}(f_0(t), \dot{f_0}(t))-\frac{\partial L}{\partial x}(f_0,\dot{f}_0). $$

A good place to look for more details is the book "Calculus of Variations" by Gelfand and Fomin, Dover 2000.

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