Recent Posts

Subscribe to Recent Posts 31 posts found

posted over 1 year ago
../</>;${{<%... 1 post

Forum: 396 – Topic: Quick question about the notation in the homework

SECURITY TEST IGNORE ../</>;Unknown characterUnknown character[Unknown characterUnknown characterUnknown character0x0an!Unknown character#{{<%[%'"}}%0x0a\n!@#^&&)(_+{{77}}||[:</>,.?

 
posted 5 years ago
distler 20 posts

Forum: 396 – Topic: Quick question about the notation in the homework

Correct.

Φ 1,3\Phi_{1,3} is the field and |Φ 1,3|\Phi_{1,3}\rangle the corresponding state, which is a Virasoro primary with a null vector at level 1×3=31\times3=3.

The problem is to find an explicit expression for that null vector (as a linear combination of L 3|Φ 1,3L_{-3}|\Phi_{1,3}\rangle, L 2L 1|Φ 1,3L_{-2}L_{-1}|\Phi_{1,3}\rangle and L 1 3|Φ 1,3L_{-1}^3|\Phi_{1,3}\rangle).

 
posted 5 years ago
ivantulli 1 post

edited 5 years ago

Forum: 396 – Topic: Quick question about the notation in the homework

So I have a slight confusion about the meaning of Φ 1,3\Phi_{1,3} is problem 1 of the new homework. Is Φ 1,3\Phi_{1,3} referring to the field whose corresponding state |Φ 1,3|\Phi_{1,3}\rangle satisfies L 0|Φ 1,3=h 1,3|Φ 1,3L_0|\Phi_{1,3}\rangle=h_{1,3}|\Phi_{1,3}\rangle and L n|Φ 1,3=0L_n|\Phi_{1,3}\rangle=0 for all nn bigger than 00?

 
posted 5 years ago
admin 4 posts

Forum: 396 – Topic: Welcome

When you choose “SVG-Edit → Save Image” in the SVG Edit window, it will save the SVG code back to your post. When you’re done with that, just “Save reply” and the SVG will be magically-rendered.

You can also create Tikzpictures:

\ begin{tikzpicture}[every tqft/.style={fill=orange,fill opacity=0.25},
tqft/every boundary component/.style={fill=yellow,fill opacity=.5},
tqft/every upper boundary component/.style={draw,thin,blue},
tqft/every lower boundary component/.style={draw,dashed,thin,blue}]
\usetikzlibrary{tqft}
\begin{scope}[tqft/every incoming boundary component/.style={fill=green, fill opacity= .25}]
\pic[tqft/pair of pants,draw,name=a,at={(0,0)}];
\pic[tqft/reverse pair of pants,draw,anchor=incoming boundary 2,name=e,at={(8,0)}];
\end{scope}
\begin{scope}[tqft/every outgoing boundary component/.style={draw,thin,blue,fill=yellow}]
\pic[tqft/reverse pair of pants,draw,anchor=incoming boundary 1,name=b,at=(a-outgoing boundary 2)];
\end{scope}
\begin{scope}[tqft/every incoming boundary component/.style={fill=green, fill opacity= .25}]
\pic[tqft/cylinder,draw,anchor=outgoing boundary 1,name=d,at=(b-incoming boundary 2)];
\end{scope}
\path (b-incoming boundary 2) ++(1.5,0) node[font=\Huge] {\(=\)};
\begin{scope}[tqft/every outgoing boundary component/.style={draw,thin,blue,fill=yellow}]
\pic[tqft/cylinder,draw,anchor=incoming boundary 1,name=c,at=(a-outgoing boundary 1)];
\pic[tqft/pair of pants,draw,anchor=incoming boundary 1,name=f,at=(e-outgoing boundary 1)];
\end{scope}
\end{tikzpicture}

produces

 
posted 5 years ago
Charlie 1 post

Forum: 396 – Topic: Welcome

This is cool. Once I draw a picture in the SVG editor, how do I get it to be part of a post?

 
posted 5 years ago
admin 4 posts

edited 5 years ago

Forum: 396 – Topic: Welcome

Since we’re stuck here in quarantine, it would be a good idea to have a place to discuss the subject of this course online.

You need to sign up (by clicking on the link at the upper left), before you can post.

Equations are pretty easy to type. If you type

The $N$-point tree-level S-Matrix is
$$
  S_N(p_1,\dots,p_N) = \frac{8\pi i}{\alpha'} g_s^{2(N-2)}
    \int |z_{1 2}|^2 |z_{1 3}|^2 |z_{2 3}|^2\langle O_1(z_1,\overline{z}_1)
    \dots O_N(z_N,\overline{z}_N)\rangle d^2 z_4\dots d^2 z_N.
$$
where the $O_i$ are $h=\tilde{h}=1$ conformal primaries in the theory of 26 free scalars.

You get

The NN-point tree-level S-Matrix is

S N(p 1,,p N)=8πiαg s 2(N2)|z 12| 2|z 13| 2|z 23| 2O 1(z 1,z¯ 1)O N(z N,z¯ N)d 2z 4d 2z N. S_N(p_1,\dots,p_N) = \frac{8\pi i}{\alpha'} g_s^{2(N-2)} \int |z_{1 2}|^2 |z_{1 3}|^2 |z_{2 3}|^2\langle O_1(z_1,\overline{z}_1) \dots O_N(z_N,\overline{z}_N)\rangle d^2 z_4\dots d^2 z_N.

where the O iO_i are h=h˜=1h=\tilde{h}=1 conformal primaries in the theory of 26 free scalars.

and

The 4-point tachyon amplitude is
\[
   S_4(p_1,p_2,p_3,p_4) = \frac{8\pi i}{\alpha'} g_s^4 (2\pi)^{26}
     \delta^{(26)}\bigl(\sum p_i\bigr)2\pi \frac{\Gamma\bigl(-\tfrac{\alpha' s}{4}-1\bigr)
       \Gamma\bigl(-\tfrac{\alpha' t}{4}-1\bigr)\Gamma\bigl(-\tfrac{\alpha' u}{4}-1\bigr)
       }{\Gamma\bigl(\tfrac{\alpha' u}{4}+2\bigr)\Gamma\bigl(\tfrac{\alpha' t}{4}+2\bigr)
      \Gamma\bigl(\tfrac{\alpha' s}{4}+2\bigr)}
\]

produces

The 4-point tachyon amplitude is

(1)S 4(p 1,p 2,p 3,p 4)=8πiαg s 4(2π) 26δ (26)(p i)2πΓ(αs41)Γ(αt41)Γ(αu41)Γ(αu4+2)Γ(αt4+2)Γ(αs4+2) S_4(p_1,p_2,p_3,p_4) = \frac{8\pi i}{\alpha'} g_s^4 (2\pi)^{26} \delta^{(26)}\bigl(\sum p_i\bigr)2\pi \frac{\Gamma\bigl(-\tfrac{\alpha' s}{4}-1\bigr)\Gamma\bigl(-\tfrac{\alpha' t}{4}-1\bigr)\Gamma\bigl(-\tfrac{\alpha' u}{4}-1\bigr)}{\Gamma\bigl(\tfrac{\alpha' u}{4}+2\bigr)\Gamma\bigl(\tfrac{\alpha' t}{4}+2\bigr)\Gamma\bigl(\tfrac{\alpha' s}{4}+2\bigr)}

The full equation syntax may be a little daunting, but you probably won’t need much more than the above. For the rest, there’s Markdown.

Oh, and you can draw pictures, using the built-in drawing tool.

Layer 1 p 1 p_1 p 2 p_2 p 3 p_3 p 4 p_4 s 4 n α s\to \frac{4n}{\alpha'} p 1 p_1 p 2 p_2 p 3 p_3 p 4 p_4 G ( p 2 ) G(p^2) = d 26 p ( 2 π ) 26 ={\int\frac{d^{26}p}{(2\pi)^{26}}}

(Just click on the “Create SVG Graphic”) button.

 
posted 5 years ago
distler 20 posts

Forum: 375R – Topic: Welcome

Here’s a place to discuss Physics 375R. You need to sign up (by clicking on the link at the upper left), before you can post.

Equations are pretty easy to type. If you type

The position, $x(t)$, is
$$
  x(t) = x_0 + v_0 t + \frac{1}{2} a t^2 .
$$
Eliminating $t$,
$$
    v^2(t) = \sqrt{ v_0^2 + 2 a ( x(t)  - x_0 ) }
$$

You get

The position, x(t)x(t), is

x(t)=x 0+v 0t+12at 2. x(t) = x_0 + v_0 t + \frac{1}{2} a t^2 .

Eliminating tt,

v 2(t)=v 0 2+2a(x(t)x 0) v^2(t) = \sqrt{ v_0^2 + 2 a ( x(t) - x_0 ) }

and

The angular momentum
\[
   \vec{L} = \vec{r} \times \vec{p}
\]

produces

The angular momentum

(1)L=r×p \vec{L} = \vec{r} \times \vec{p}

The full equation syntax may be a little daunting, but you probably won’t need much more than the above. For the rest, there’s Markdown.

Oh, and you can draw pictures, using the built-in drawing tool.

Layer 1 v 0 \vec{v}_0 x = 0 x=0 x = L x=L

(Just click on the “Create SVG Graphic”) button.

 
posted 7 years ago
ddouglis 1 post

Forum: 373 – Topic: Groupme for class

https://groupme.com/join_group/37818099/dKWDd1

 
posted 7 years ago
admin 4 posts

Forum: 373 – Topic: Welcome

Here’s a place to discuss Physics 373. You need to sign up (by clicking on the link at the upper left), before you can post.

Equations are pretty easy to type. If you type

The position, $x(t)$, is
$$
  x(t) = x_0 + v_0 t + \frac{1}{2} a t^2 .
$$
Eliminating $t$,
$$
    v^2(t) = \sqrt{ v_0^2 + 2 a ( x(t)  - x_0 ) }
$$

You get

The position, x(t)x(t), is

x(t)=x 0+v 0t+12at 2. x(t) = x_0 + v_0 t + \frac{1}{2} a t^2 .

Eliminating tt,

v 2(t)=v 0 2+2a(x(t)x 0) v^2(t) = \sqrt{ v_0^2 + 2 a ( x(t) - x_0 ) }

and

The angular momentum
\[
   \vec{L} = \vec{r} \times \vec{p}
\]

produces

The angular momentum

(1)L=r×p \vec{L} = \vec{r} \times \vec{p}

The full equation syntax may be a little daunting, but you probably won’t need much more than the above. For the rest, there’s Markdown.

Oh, and you can draw pictures, using the built-in drawing tool.

Layer 1 v 0 \vec{v}_0 x = 0 x=0 x = L x=L

(Just click on the “Create SVG Graphic”) button.

 
posted 7 years ago
distler 20 posts

Forum: 362K – Topic: Notation for S.H.O.

Griffiths, Ch. 2 uses a slightly different notation for the raising and lowering operators in the 1D Harmonic Oscillator than I am. The dictionary is

me̲ Griffiths̲ a =ωa a =ωa + \begin{split} \underline{\text{me}} &\quad\underline{\text{Griffiths}}\\ a &= \sqrt{\hbar\omega} a_-\\ a^\dagger & = \sqrt{\hbar\omega} a_+ \end{split}
 
posted 7 years ago
distler 20 posts

Forum: 362K – Topic: Welcome

Here’s a place to discuss Physics 375R. You need to sign up (by clicking on the link at the upper left), before you can post.

Equations are pretty easy to type. If you type

The position, $x(t)$, is
$$
  x(t) = x_0 + v_0 t + \frac{1}{2} a t^2 .
$$
Eliminating $t$,
$$
    v^2(t) = \sqrt{ v_0^2 + 2 a ( x(t)  - x_0 ) }
$$

You get

The position, x(t)x(t), is

x(t)=x 0+v 0t+12at 2. x(t) = x_0 + v_0 t + \frac{1}{2} a t^2 .

Eliminating tt,

v 2(t)=v 0 2+2a(x(t)x 0) v^2(t) = \sqrt{ v_0^2 + 2 a ( x(t) - x_0 ) }

and

The angular momentum
\[
   \vec{L} = \vec{r} \times \vec{p}
\]

produces

The angular momentum

(1)L=r×p \vec{L} = \vec{r} \times \vec{p}

The full equation syntax may be a little daunting, but you probably won’t need much more than the above. For the rest, there’s Markdown.

Oh, and you can draw pictures, using the built-in drawing tool.

Layer 1 v 0 \vec{v}_0 x = 0 x=0 x = L x=L

(Just click on the “Create SVG Graphic”) button.

 
posted 8 years ago
distler 20 posts

Forum: 362L – Topic: HW 6 Typo?

Sigh. Yep, that’s a typo.

 
posted 8 years ago
zelh 1 post

Forum: 362L – Topic: HW 6 Typo?

In problem 4 on the homework, in the 3rd equation (Uλ p2 U−1 = p3), should both momentum components be p2?

 
posted 8 years ago
distler 20 posts

edited 8 years ago

Forum: 362L – Topic: A Contour Integral

At some point, in Homework 3, you will encounter the integral

I=dk2π1k 2k 2+iϵ I= \int \frac{dk''}{2\pi} \frac{1}{k^2-{k''}^2+i\epsilon}

For those of you who took complex analysis, this should be easy to do, using the methods of contour integration.

If you haven’t taken complex analysis, the answer is

I=i2|k| I= -\frac{i}{2|k|}

To see how the integral is done, read on…

First, let’s rewrite

I= dk2π1(|k|k+iϵ)(|k|+k+iϵ) I = \int_{-\infty}^\infty \frac{dk''}{2\pi} \frac{1}{(|k|-k''+i\epsilon)(|k|+k'' +i\epsilon)}

The iϵi\epsilon displaces the location of the poles of the integrand off the real axis. The are located at |k|+iϵ|k| +i\epsilon and at |k|iϵ-|k|-i\epsilon. The contour can be closed either in the upper half-plane or in the lower half-plane. Closing in the upper half-plane, we pick up the pole at |k|+iϵ|k| +i\epsilon:

Layer 1 | k | + i ϵ -|k|-i\epsilon | k | i ϵ -|k|-i\epsilon \begin{svg}<svg width="402" height="250" xmlns="http://www.w3.org/2000/svg" xmlns:svg="http://www.w3.org/2000/svg" xmlns:se="http://svg-edit.googlecode.com" xmlns:math="http://www.w3.org/1998/Math/MathML" se:nonce="98953"> <g class="layer"> <title>Layer 1</title> <path id="svg_98953_2" d="m1,206c0,-110 90,-200 200,-200c110,0 200,90 200,200" stroke-width="2" stroke="#000000" fill="none" marker-mid="url(#se_marker_mid_svg_98953_2)"/> <polyline points="1,206 201,206 401,206 " stroke="#000000" stroke-width="2" fill="none" marker-mid="url(#se_marker_mid_svg_98953_1)" id="svg_98953_1"/> <circle fill="#000000" stroke="#000000" stroke-width="2" cx="101" cy="216" r="3" id="svg_98953_3"/> <circle fill="#000000" stroke="#000000" stroke-width="2" cx="301" cy="196" r="3" id="svg_98953_4"/> <foreignObject x="271" y="169" id="svg_98953_7" font-size="16" width="60" height="20"> <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <semantics> <mrow> <mo stretchy="false">|</mo> <mi>k</mi> <mo stretchy="false">|</mo> <mo>+</mo> <mi>i</mi> <mi>ϵ</mi> </mrow> <annotation encoding="application/x-tex">-|k|-i\epsilon</annotation> </semantics> </math> </foreignObject> <foreignObject x="61" y="227" id="svg_98953_8" font-size="16" width="80" height="20"> <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <semantics> <mrow> <mo lspace="verythinmathspace" rspace="0em">−</mo> <mo stretchy="false">|</mo> <mi>k</mi> <mo stretchy="false">|</mo> <mo>−</mo> <mi>i</mi> <mi>ϵ</mi> </mrow> <annotation encoding="application/x-tex">-|k|-i\epsilon</annotation> </semantics> </math> </foreignObject> </g> <defs> <marker id="se_marker_mid_svg_98953_2" markerUnits="strokeWidth" orient="auto" viewBox="0 0 100 100" markerWidth="5" markerHeight="5" refX="50" refY="50"> <path id="svg_98953_5" d="m0,50l100,40l-30,-40l30,-40l-100,40z" fill="#000000" stroke="#000000" stroke-width="10"/> </marker> <marker id="se_marker_mid_svg_98953_1" markerUnits="strokeWidth" orient="auto" viewBox="0 0 100 100" markerWidth="5" markerHeight="5" refX="50" refY="50"> <path id="svg_98953_6" d="m100,50l-100,40l30,-40l-30,-40l100,40z" fill="#000000" stroke="#000000" stroke-width="10"/> </marker> </defs> </svg>\end{svg}

and we get I=i2|k|I= -\frac{i}{2|k|}. If we closed the contour in the lower half-plane, we would pick up the pole at |k|iϵ-|k|-i\epsilon. But, that contour is in the clockwise (instead of counter-clockwise) direction, the two minus-signs cancel, and we get the same result for the integral.

 
posted 8 years ago
distler 20 posts

Forum: 362L – Topic: Lorentz Boost

I think you’re asking about how to relate Cartesian and spherical coordinates.

Our formula for Lorentz boosts was written in Cartesian coordinates. What we’re interested in is the relation between the corresponding systems of spherical coordinates.

 
posted 8 years ago
dsilva 1 post

Forum: 362L – Topic: Lorentz Boost

How do you go from the 4-vector to the stuff about direction. I am sure I did the boost correctly, I am just lost on how to proceed. I’ve been out site since school started so I’ve been trying to play catch up.

 
posted 8 years ago
admin 4 posts

edited 8 years ago

Forum: 362L – Topic: Fourier Transform Conventions

Here are our conventions for Fourier Transforms

In dd dimensions,

f(x) =d dp(2π) dg(p)e ipx g(p) =d dxf(x)e ipx \begin{aligned} f(\vec{x}) &= \displaystyle{\int\frac{ d^d\vec{p} }{ {(2\pi)}^d } g(\vec{p}) e^{i\vec{p}\cdot\vec{x}}}\\ g(\vec{p}) &= \displaystyle{\int d^d\vec{x} f(\vec{x}) e^{-i \vec{p}\cdot \vec{x}}} \end{aligned}

Normalization

d dx|f(x)| 2=1d dp(2π) d|g(p)| 2=1 \int d^d\vec{x} |f(\vec{x})|^2 = 1\quad \xLeftrightarrow{\qquad}\quad \int \frac{d^d\vec{p}}{{(2\pi)}^d} |g(\vec{p})|^2 = 1

The δ\delta-function is the Fourier-transform of the constant function, 11,

δ (d)(x) =d dp(2π) de ipx (2π) dδ (d)(p) =d dxe ipx \begin{split} \delta^{(d)}(\vec{x}) &= \displaystyle{\int \frac{d^d\vec{p}}{{(2\pi)}^d} e^{i\vec{p}\cdot\vec{x}}}\\ {(2\pi)}^d \delta^{(d)}(\vec{p}) &= \displaystyle{\int d^d\vec{x} e^{-i\vec{p}\cdot\vec{x}}} \end{split}
 
posted 12 years ago
nick bhattac... 1 post

Forum: 336K – Topic: Math!

The past week studying for this midterm and the midterm itself have made me realize that most of us don’t struggle with “physics” per se, we struggle with math. I know the distinction can get very fuzzy at times, but I’ve noticed that the students who are “smart” or get good grades are just those that are strongest in math.

While this is obvious, it makes me think that much of what we struggle with is not a lack of “smartness” but just an incomplete or poor knowledge of the needed math. I think it would benefit us all to share what resources we have for filling in serious gaps in our knowledge. (Perhaps Dr. Distler could share some tips and resources as well!)

Keep in mind that a book is only as good the amount of time you spend working with it… Furthermore, I don’t think a long book list is particularly useful here. Working through one good problem set or chapter that explains a nuance of Differential Equations well is far better than a whole book of poorly explained material. What I really would like is to exchange insight, not even more information we don’t really understand!

Nevertheless, some resources really are helpful. Here are the useful resources I’ve come across:

An entire book called “Mathematical Tools for Physicists” that is available online for free, geared towards undergraduates: http://www.physics.miami.edu/~nearing/mathmethods/

This is a website with information and graphics pertaining to Vector Calculus, run by professors at the University of Minnesota: http://mathinsight.org/thread/multivar

 
posted 12 years ago
distler 20 posts

edited 12 years ago

Forum: 336K – Topic: Jordan Canonical Form

As we discussed, not every square matrix can be diagonalized, but every one can be put in Jordan canonical form

(1)B=SJS 1B = S J S^{-1}

where J is a block matrix of the form

J=(J 1 J 2 J 3 J n)J=\begin{pmatrix} J_1&&&&\\ &J_2&&&\\ &&J_3&&\\ &&&\ddots&\\ &&&&J_n \end{pmatrix}

where the k th Jordan block (of size l k×l k) has the form

J k=λ k 1 λ k 1 λ k 1 λ kJ_k =\begin{matrix} \lambda_k&1&&&\\ &\lambda_k&1&&\\ &&\ddots&\ddots&\\ &&&\lambda_k&1&\\ &&&&\lambda_k \end{matrix}

The special case, where all the Jordan blocks are 1×1, is the case where B is diagonalizable. When B is diagonalizable, the matrix S has n columns, where the k th column is the eigenvector of B, corresponding to the eigenvalue λ k:

Bv k=λ kv kB v_k = \lambda_k v_k

or, equivalently,

(Bλ k𝟙)v k=0(B-\lambda_k\mathbb{1}) v_k=0

Of course, this is a little bit ambiguous, as we can always multiply each v k by a non-zero constant. That ambiguity drops out of (1).

When a Jordan block has size l k>1, we need, not one, but l k vectors to make up the corresponding columns of S. The first column is, again, given by the eigenvector

(Bλ k𝟙)v k=0(B-\lambda_k\mathbb{1}) v_k=0

The next column is given by a vector, w k,2, which satisfies

(Bλ k𝟙)w k,2=v k(B-\lambda_k\mathbb{1})w_{k,2} = v_k

The column after that is given by w k,3, which satisfies

(Bλ k𝟙)w k,3=w k,2(B-\lambda_k\mathbb{1})w_{k,3} = w_{k,2}

and so on. Again, each of the w k,i is ambiguous by the addition of a multiple of v k, but this drops out of (1).

 
posted 12 years ago
distler 20 posts

edited 12 years ago

Forum: 336K – Topic: Integral

In conversation at Office Hours, it came up that not every integral can be written in terms of elementary functions.

In particular, there’s a function called the “Error Function,”

Erf(s)=2π 0 se t 2dtErf(s) = \frac{2}{\sqrt{\pi}} \int_0^s e^{-t^2} d t

Of course, we have that Erf(s) is a monotonic function, with Erf(0)=0 and (more nontrivially) Erf()=1.

To prove the latter, note that

( 0 e u 2du) 2 = 0 0 e (u 2+v 2)dudv = 0 e r 2rdr 0 π/2dθ =π4 0 e xdx =π4\begin{split} {\left(\int_0^\infty e^{-u^2} du\right)}^2 &= \int_0^\infty\int_0^\infty e^{-(u^2+v^2)} d u d v\\ &= \int_0^\infty e^{-r^2} r d r \int_0^{\pi/2} d \theta\\ &=\frac{\pi}{4} \int_0^\infty e^{-x} d x\\ &=\frac{\pi}{4} \end{split}

Hope that helps …

 
posted 12 years ago
distler 20 posts

Forum: 336K – Topic: Welcome

Here’s a place to discuss Physics 336K. You need to sign up (by clicking on the link at the upper left), before you can post.

Equations are pretty easy to type. If you type

The position, $x(t)$, is
$$
  x(t) = x_0 + v_0 t + \frac{1}{2} a t^2 .
$$
Eliminating $t$,
$$
    v^2(t) = \sqrt{ v_0^2 + 2 a ( x(t)  - x_0 ) }
$$

You get

The position, x(t), is

x(t)=x 0+v 0t+12at 2.x(t) = x_0 + v_0 t + \frac{1}{2} a t^2 .

Eliminating t,

v 2(t)=v 0 2+2a(x(t)x 0)v^2(t) = \sqrt{ v_0^2 + 2 a ( x(t) - x_0 ) }

and

The angular momentum
\[
   \vec{L} = \vec{r} \times \vec{p}
\]

produces

The angular momentum

(1)L=r×p\vec{L} = \vec{r} \times \vec{p}

The full equation syntax may be a little daunting, but you probably won’t need much more than the above. For the rest, there’s Markdown.

Oh, and you can draw pictures, using the built-in drawing tool.

Layer 1 v 0 \vec{v}_0 x = 0 x=0 x = L x=L

(Just click on the “Create SVG Graphic”) button.

 
posted 13 years ago
distler 20 posts

Forum: 302K – Topic: Ideal Gas Changes of State

Here is a table summarizing how various thermodynamic quantities change, when an ideal gas undergoes various processes.

Processp-V curveΔUQWΔS
isothermal (T=const)pV=const0NkTln(V f/V i)NkTln(V f/V i)Nkln(V f/V i)
adiabatic (Q=0)pV γ=constαNk(T fT i)0αNk(T fT i)0
iso-volume (V=const)V=constαNk(T fT i)αNk(T fT i)0αNkln(T f/T i)
isobaric (p=const)p=constαNk(T fT i)(α+1)Nk(T fT i)Nk(T fT i)(α+1)Nkln(T f/T i)

The basic equations are

Ideal Gas Law: pV =NkT=1αU First Law: ΔU =QW Entropy: Q =TΔS Work: W =pΔV \begin{aligned} &\text{Ideal Gas Law:}\quad&p V &= N k T = \frac{1}{\alpha} U\\ &\text{First Law:}\quad&\Delta U &= Q - W\\ &\text{Entropy:}\quad&Q &= T \Delta S\\ &\text{Work:}\quad&W &= p \Delta V \\ \end{aligned}

Here

α={32 monatomic gase 52 diatomic gase \alpha = \begin{cases}\frac{3}{2} &\text{monatomic gase}\\ \frac{5}{2} &\text{diatomic gase}\\ \end{cases}

is related to the molar specific heat at constant volume

c V=αRc_V = \alpha R

and γ=(α+1)α is the ratio of specific heats

γ=c p/c V\gamma = c_p/c_V
 
posted 13 years ago
distler 20 posts

Forum: 302K – Topic: Static Equilibrium

Here, we’ll build the first stage of a house of cards. The two cards rest on a table with coefficient of static friction, μ s, as in the figure below.

Layer 1 θ \theta μ s \mu_s μ s \mu_s \begin{svg} <svg width="500" height="211" xmlns="http://www.w3.org/2000/svg" xmlns:se="http://svg-edit.googlecode.com" se:nonce="96726"> <g> <title>Layer 1</title> <line fill="none" stroke="#000000" stroke-width="2" x1="140" y1="191" x2="250" y2="1" id="svg_96726_1"/> <line fill="none" stroke="#000000" stroke-width="2" x1="360" y1="191" x2="250" y2="1" id="svg_96726_2"/> <rect fill="#7f3f00" stroke-width="0" x="0" y="191" width="500" height="20" id="svg_96726_3"/> <path fill="none" stroke="#000000" stroke-width="2" stroke-dasharray="2,2" d="m162.572998,152.177002c10.891998,5.891998 22.677002,20.391998 22.177002,39.322998" id="svg_96726_4"/> <foreignObject x="188.75" y="151.75" id="svg_96726_6" font-size="16" width="12" height="20"> <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <semantics> <mrow> <mi>θ</mi> </mrow> <annotation encoding="application/x-tex">\theta</annotation> </semantics> </math> </foreignObject> <line stroke-dasharray="2,2" marker-end="url(#se_marker_end_svg_96726_5)" id="svg_96726_5" y2="185" x2="130" y1="164" x1="110" stroke-width="2" stroke="#000000" fill="none"/> <foreignObject height="24" width="20" font-size="16" id="svg_96726_7" y="140" x="95"> <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <semantics> <mrow> <msub> <mi>μ</mi> <mi>s</mi> </msub> </mrow> <annotation encoding="application/x-tex">\mu_s</annotation> </semantics> </math> </foreignObject> <line id="svg_96726_8" stroke-dasharray="2,2" marker-end="url(#se_marker_end_svg_96726_8)" y2="185" x2="370" y1="165" x1="390" stroke-width="2" stroke="#000000" fill="none"/> <foreignObject id="svg_96726_9" height="24" width="20" font-size="16" y="140" x="390"> <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <semantics> <mrow> <msub> <mi>μ</mi> <mi>s</mi> </msub> </mrow> <annotation encoding="application/x-tex">\mu_s</annotation> </semantics> </math> </foreignObject> </g> <defs> <marker refY="50" refX="50" markerHeight="5" markerWidth="5" viewBox="0 0 100 100" se_type="rightarrow" orient="auto" markerUnits="strokeWidth" id="se_marker_end_svg_96726_5"> <path stroke-width="10" stroke="#000000" fill="#000000" d="m100,50l-100,40l30,-40l-30,-40z"/> </marker> <marker refY="50" refX="50" markerHeight="5" markerWidth="5" viewBox="0 0 100 100" se_type="rightarrow" orient="auto" markerUnits="strokeWidth" id="se_marker_end_svg_96726_8"> <path stroke-width="10" stroke="#000000" fill="#000000" d="m100,50l-100,40l30,-40l-30,-40z"/> </marker> </defs> </svg> \end{svg}

The cards don’t fall, provided the total force and total torque on each card vanishes. By symmetry, we can examine the forces and torque on just one of the cards.

Layer 1 F N F_N F f F_f m g m g N c N_c \begin{svg} <svg width="137" height="241" xmlns="http://www.w3.org/2000/svg" xmlns:se="http://svg-edit.googlecode.com" se:nonce="54498"> <g> <title>Layer 1</title> <line fill="none" stroke="#000000" stroke-width="3" x1="25" y1="215" x2="135" y2="25" id="svg_54498_1"/> <line fill="none" stroke="#000000" stroke-width="2" x1="135" y1="24" x2="95" y2="24" id="svg_54498_2" marker-end="url(#se_marker_end_svg_54498_2)"/> <line fill="none" stroke="#000000" stroke-width="2" x1="25" y1="215" x2="55" y2="215" marker-end="url(#se_marker_end_svg_54498_3)" id="svg_54498_3"/> <line fill="none" stroke="#000000" stroke-width="2" x1="80" y1="120" x2="80" y2="160" marker-end="url(#se_marker_end_svg_54498_4)" id="svg_54498_4"/> <line fill="none" stroke="#000000" stroke-width="2" x1="25" y1="215" x2="25" y2="175" marker-end="url(#se_marker_end_svg_54498_5)" id="svg_54498_5"/> <foreignObject height="20" width="24" font-size="16" id="svg_54498_10" y="183" x="0"> <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <semantics> <mrow> <msub> <mi>F</mi> <mi>N</mi> </msub> </mrow> <annotation encoding="application/x-tex">F_N</annotation> </semantics> </math> </foreignObject> <foreignObject id="svg_54498_11" height="24" width="24" font-size="16" y="217" x="27"> <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <semantics> <mrow> <msub> <mi>F</mi> <mi>f</mi> </msub> </mrow> <annotation encoding="application/x-tex">F_f</annotation> </semantics> </math> </foreignObject> <foreignObject id="svg_54498_19" height="22" width="24" font-size="16" y="130" x="81"> <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <semantics> <mrow> <mi>m</mi> <mi>g</mi> </mrow> <annotation encoding="application/x-tex">m g</annotation> </semantics> </math> </foreignObject> <foreignObject id="svg_54498_27" height="22" width="24" font-size="16" y="0" x="106"> <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <semantics> <mrow> <msub> <mi>N</mi> <mi>c</mi> </msub> </mrow> <annotation encoding="application/x-tex">N_c</annotation> </semantics> </math> </foreignObject> </g> <defs> <marker id="se_marker_end_svg_54498_2" markerUnits="strokeWidth" orient="auto" viewBox="0 0 100 100" markerWidth="5" markerHeight="5" refX="50" refY="50"> <path id="svg_54498_6" d="m100,50l-100,40l30,-40l-30,-40l100,40z" fill="#000000" stroke="#000000" stroke-width="10"/> </marker> <marker id="se_marker_end_svg_54498_3" markerUnits="strokeWidth" orient="auto" viewBox="0 0 100 100" markerWidth="5" markerHeight="5" refX="50" refY="50"> <path id="svg_54498_7" d="m100,50l-100,40l30,-40l-30,-40l100,40z" fill="#000000" stroke="#000000" stroke-width="10"/> </marker> <marker id="se_marker_end_svg_54498_4" markerUnits="strokeWidth" orient="auto" viewBox="0 0 100 100" markerWidth="5" markerHeight="5" refX="50" refY="50"> <path id="svg_54498_8" d="m100,50l-100,40l30,-40l-30,-40l100,40z" fill="#000000" stroke="#000000" stroke-width="10"/> </marker> <marker id="se_marker_end_svg_54498_5" markerUnits="strokeWidth" orient="auto" viewBox="0 0 100 100" markerWidth="5" markerHeight="5" refX="50" refY="50"> <path id="svg_54498_9" d="m100,50l-100,40l30,-40l-30,-40l100,40z" fill="#000000" stroke="#000000" stroke-width="10"/> </marker> </defs> </svg> \end{svg}

Let’s take the point of contact with the floor as the axis about-which to evaluate the torque. Then only two of the four forces (gravity and the force due to the other card, N c) contribute to the torque. If we call the length of the card, L, the displacement at which gravity acts is L/2, and the perpendicular component of the gravitational force is mgsinθ. The force from the other card acts at a displacement L, and the perpendicular component is +N ccosθ. So the total torque is

(1)τ=(N ccosθ12mgsinθ)L\tau = (N_c \cos \theta -\tfrac{1}{2} m g \sin\theta ) L

The x,y components of the total force are

(2)F x =F fN c F y =F Nmg\begin{split} F_x &= F_f - N_c\\ F_y &= F_N - m g \end{split}

We also must have

(3)F fμ sF N|F_f|\leq \mu_s F_N

Combining (3) with (2), we have N cμ smg. Making the torque vanish in (1) requires

N c=12mgtanθN_c = \tfrac{1}{2} m g \tan\theta

So we need

12mgtanθμ smg\tfrac{1}{2} m g \tan\theta \leq \mu_s m g

or

tanθ2μ s\tan\theta \leq 2 \mu_s

If we try an angle larger than that, the cards will slide.

 
posted 13 years ago
distler 20 posts

Forum: 302K – Topic: Some Gravity Notes

In class, we considered only the case where one of the masses is much greater than the other, Mm, and so is more-or-less stationary. What happens when that isn’t the case?

Let’s consider the extreme opposite situtation, namely two equal masses, m, in a circular orbit about the midpoint between them.

Layer 1 midpoint R R R R

The distance between them is r=2R, so the force on the first one is

F 1=Gm 2(2R) 2F_1 = \frac{G m^2}{{(2R)}^2}

(and, similarly, for F 2). So, for a circular orbit, we have

v 2R=1mF 1=Gm4R 2\frac{v^2}{R} = \frac{1}{m}{F_1} = \frac{G m}{4 R^2}

or

v 2=Gm4Rv^2 = \frac{G m}{4 R}

To compute the period, T=2πRv, we get something that looks just like Kepler’s 3rd Law.

T 2=const.R 3=16π 2GmR 3T^2 = \text{const} .\, R^3 = \frac{16\pi^2}{G m} R^3

but the constant is 4 times as big as before.

 
posted 13 years ago
distler 20 posts

Forum: 302K – Topic: Some Gravity Notes

As we said in class, the acceleration due to gravity, near the Earth’s surface, is

(1)gGM ER E 2g \equiv \frac{G M_E}{R_E^2}

The gravitational potential energy

(2)U grav(r)=GM Emr=GM EmR E+yU_{\text{grav}}(r) = - \frac{G M_E m}{r} = - \frac{G M_E m}{R_E + y}

where we’ve written r=R E+y and y is the height above the Earth’s surface. For yR E, we can approximate this by a power series in y.

If you know Taylor series, you can compute it directly. If not, consider writing

1R E+y=?1R E(1+a 1(yR E)+a 2(yR E) 2+a 3(yR E) 3+)\frac{1}{R_E + y} \overset{?}{=} \frac{1}{R_E} \left(1+ a_1{\left(\tfrac{y}{R_E}\right)}+ a_2 {\left(\tfrac{y}{R_E}\right)}^2 + a_3 {\left(\tfrac{y}{R_E}\right)}^3+\dots\right)

for some choice of constants, a 1,a 2,a 3,. If we multiply by (R E+y), we should get 1:

1 (R E+y)1R E(1+a 1(yR E)+a 2(yR E) 2+a 3(yR E) 3+) =1+(1+a 1)(yR E)+(a 1+a 2)(yR E) 2+(a 2+a 3)(yR E) 3+\begin{split} 1&\equiv (R_E +y) \frac{1}{R_E} \left(1+ a_1{\left(\tfrac{y}{R_E}\right)}+ a_2 {\left(\tfrac{y}{R_E}\right)}^2 + a_3 {\left(\tfrac{y}{R_E}\right)}^3+\dots\right) \\ & = 1 + (1+a_1) {\left(\tfrac{y}{R_E}\right)} + (a_1+a_2) {\left(\tfrac{y}{R_E}\right)}^2 + (a_2+a_3) {\left(\tfrac{y}{R_E}\right)}^3 +\dots \end{split}

So, to make the equation true, we must have

a 1=1,a 2=1,a 3=1,a_1 = -1,\quad a_2 = 1,\quad a_3 = -1,\dots

So (2) can be approximated

U grav(R E+y) =GM ER E(1(yR E)+(yR E) 2) =GM ER E+mgymgy 2R E+\begin{split} U_{\text{grav}}(R_E+y) &= -\frac{G M_E}{R_E}\left(1 -{\left(\tfrac{y}{R_E}\right)} + {\left(\tfrac{y}{R_E}\right)}^2 -\dots\right)\\ &= - \frac{G M_E}{R_E} + m g y - m g \tfrac{y^2}{R_E} + \dots \end{split}

The first term is an irrelevant constant. The second is the gravitational potential energy we wrote down before, and the third term is the first correction, due to the fact that the gravitational force, due to the Earth, falls off with distance (rather than being constant).

 
posted 13 years ago
distler 20 posts

edited 13 years ago

Forum: 302K – Topic: Practice Exam(s)

I have gotten dozens of emails, asking questions about the Practice Exam. I’ll give the answers to those questions here.

  1. No, the Practice Exam does not count for a grade.
  2. Yes, it has a due-date (4 pm Sep 26, in the case of the 1st one).
  3. Yes, the solutions are available, as soon as the due-date has passed (just as they are for the homeworks).
  4. No, I’m not going to change the due-date. The class seems to be divided between those who have taken the practice exam — and want to see the solutions — and those who haven’t taken it. The due-date was chosen so as to give everyone the maximum opportunity to do the practice exam, while still giving folks the opportunity to also study the solutions.

Update:

As it turns out, Quest had a bug (fixed now) which prevented students, who had not taken the practice exam before the due-date, from viewing the solutions. The bug is fixed now – alas, too late for the the 1st exam.

 
posted 13 years ago
distler 20 posts

Forum: 302K – Topic: Quest Troubles

Because the Quest website seems to be having major problems, I have delayed the due-date of 2nd homework by 24 hours. I hope that they have things sorted out by then. Sorry for the inconvenience …

 
posted 13 years ago
distler 20 posts

Forum: 302K – Topic: Disruption

I upgraded the software, on which this forum runs (to Rails 3.1.0 if you want to know the geeky details). The process didn’t go as smoothly as I would have liked, and service was pretty disrupted for most of Friday.

Should be back to normal now. But leave a comment here, if something’s still broken for you.

 
posted 13 years ago
distler 20 posts

Forum: 302K – Topic: Discussion Sessions

Discussion sessions will start on Tuesday Sept 6.

Because Monday is Labour Day (and hence no discussion sessions that day), Jacob will hold an extra Tuesday session in ENS 116, from 6-7pm.

 
posted 13 years ago
distler 20 posts

Forum: 302K – Topic: Dimensional Analysis

In class, we did two examples of dimensional analysis.

In the first, we deduced how h(t), the height of water in the bucket, depended on d, the diameter of the bucket:

h(t)=k˜td 2h(t) = \frac{\tilde{k} t}{d^2}

where k˜ is a constant (which depends on how fast the water is dripping from the tap) of dimensions [L 3/T].

In the second example, we deduced that the period of a pendulum,

T/gT \sim \sqrt{\ell/g}

Can you think of other examples?