This is a space, easily accessible from the front page, where you can practice your LaTeX/MimeTeX commands for writing equations for adding to discussions, etc. You can see several people’s experiments at the earlier post here.

Instructions and examples are to be found at the mimeTeX site, and there is a place to practice there too. Their tutorial is here. (The part on pictures is here.)

The key thing for getting your equation to show up on the site in a comment is to enclose it between the following two delimiters:

[ tex] (LaTeX-like commands go here) [ /tex]

…but don’t include the spaces after the brackets. I had to do that just now to stop the blog machine from turning them into instructions to make an equation.

Beware that for some more technical things (such as pictures) the mimeTeX command set is a bit different from the LaTeX ones you might be familiar with. Consult the manual above.

From time to time I will come in here and clean up the mess, so don’t leave things here that you want to keep for too long. This is just for practice.

-cvj

134 Responses to “LaTeX Sandbox”


  1. 1 Clifford

    E=mc^2

    A test.

    -cvj

  2. 2 Carl Brannen

    The basic problem is that this feels more and more like work.

  3. 3 Clifford

    no… it is fun! not work!

    We’re all watching with anticipation, Carl….

    -cvj

  4. 4 Carl Brannen

    Ah, what the heck. Besides the Clifford algebra / idempotent structure of the fermions, the other physics thing I’ve been working on is a related coincidence in the masses of the leptons. The paper has the unusual attribute of being written by an obviously insane amateur, no PhD, doesn’t believe in relativity, never published, but nevertheless it is already referenced by various papers in the physics literature, one of these peer reviewed.

    The relation can be thought of as geometric, and anything geometric can also be put into holiday format. Hmmm…

    Yes, we can graph the lepton masses in “Star of David” form. Furthermore, the numbers are accurate to close to the center of current experimental measurements. Hope the boss doesn’t find out that I’m doing this.

  5. 5 Kea

    \setlength{\unitlength}{0.2mm}
\begin{picture}(400,400)
\put(125,20){\oval(80,40)} \put(275,20){\oval(80,40)}
\put(165,20){\line(1,0){68}} \put(125,70){\oval(50,60)[l]}
\put(275,70){\oval(50,60)[r]} \put(125,100){\line(-2,-1){55.9}}
\put(275,100){\line(2,-1){55.9}} \put(75,75){\line(1,1){80}}
\put(325,75){\line(-1,1){90}} \put(240,160){\line(0,1){68}}
\put(145,195){\oval(30,100)[l]} \put(145,245){\line(2,1){70}}
\put(100,245){\oval(90,90)[t]} \put(53,243){\circle{5.7}}
\put(180,130){\line(-1,3){20}} \put(180,130){\line(1,3){20}}
\put(160,190){\line(1,0){40}} \put(155,199){\oval(10,18)}
\put(205,199){\oval(10,18)} \put(157,199){\circle{6}} \put(203,199){\circle{6}}
\put(53,245){\line(0,1){50}} \put(53,295){\line(2,1){100}}
\put(200,270){\line(1,-1){40}} \put(158,345){\line(1,-1){60}}
\end{picture}

  6. 6 Kea

    Damn. It rescales things wrong.

  7. 7 Kea

    \begin{picture}(400,400)
\put(125,20){\oval(80,40)} \put(275,20){\oval(80,40)}
\put(165,20){\line(1,0){68}} \put(125,70){\oval(50,60)[l]}
\put(275,70){\oval(50,60)[r]} \put(125,100){\line(-2,-1){55.9}}
\put(275,100){\line(2,-1){55.9}} \put(75,75){\line(1,1){80}}
\put(325,75){\line(-1,1){90}} \put(240,160){\line(0,1){68}}
\put(145,195){\oval(30,100)[l]} \put(145,245){\line(2,1){70}}
\put(100,245){\oval(90,90)[t]} \put(53,243){\circle{5.7}}
\put(180,130){\line(-1,3){20}} \put(180,130){\line(1,3){20}}
\put(160,190){\line(1,0){40}} \put(155,199){\oval(10,18)}
\put(205,199){\oval(10,18)} \put(157,199){\circle{6}} \put(203,199){\circle{6}}
\put(53,245){\line(0,1){50}} \put(53,295){\line(2,1){100}}
\put(200,270){\line(1,-1){40}} \put(158,345){\line(1,-1){60}}
\end{picture}

  8. 8 Kea

    One last try:

    \begin{picture}(400,400) \unitlength{0.2} \put(125,20){\oval(80,40)}
\put(275,20){\oval(80,40)} \put(165,20){\line(1,0){68}}
\put(125,70){\oval(50,60)[l]} \put(275,70){\oval(50,60)[r]}
\put(125,100){\line(-2,-1){55.9}} \put(275,100){\line(2,-1){55.9}}
\put(75,75){\line(1,1){80}} \put(325,75){\line(-1,1){90}}
\put(240,160){\line(0,1){68}} \put(145,195){\oval(30,100)[l]}
\put(145,245){\line(2,1){70}} \put(100,245){\oval(90,90)[t]}
\put(53,243){\circle{5.7}} \put(180,130){\line(-1,3){20}}
\put(180,130){\line(1,3){20}} \put(160,190){\line(1,0){40}}
\put(155,199){\oval(10,18)} \put(205,199){\oval(10,18)}
\put(157,199){\circle{6}} \put(203,199){\circle{6}}
\put(53,245){\line(0,1){50}} \put(53,295){\line(2,1){100}}
\put(200,270){\line(1,-1){40}} \put(158,345){\line(1,-1){60}}
\end{picture}

  9. 9 Carl Brannen

    This is definitely becoming work. Here’s a link to a somewhat ugly Star of David plot of the lepton masses.

  10. 10 Plato

    This is tuff stuff and will be tackling when I get back. Maybe a good book some where? I’ve exhausted many sites looking for examples of trees :) I know that’s cheating.

    I was thinking a comparative construction look at the latex written, and beside it, the tree. Just to get the idea of building imagery alongside of latex.

    Merry Christmas.

  11. 11 Navneeth

    Kea, what’s a penguin got to do with Christams?

    Hmm…Christmas->Winter->Snow->Antarctica->Penguins…okay got it! :D

    ;)

  12. 12 Carl Brannen

    \begin{picture}(400,200)
\put(001,001){\line(399,001)}
\put(399,001){\line(399,199)}
\put(399,199){\line(001,199)}
\put(001,199){\line(001,001)}
\put(001,155){\line(150,145)}
\end{picture}

    Note to self: When writing a computer program, always begin with another computer program that is known to work.

  13. 13 Carl Brannen

    \begin{picture}(400,200)
\put(000,000){\line(400,000)}
\put(000,000){\line(000,200)}
\put(399,000){\line(000,200)}
\put(000,199){\line(400,000)}
\put(001,155){\line(150,-10)}
\end{picture}

    Oh yeah, line is relative, put is absolute

  14. 14 Carl Brannen

    \begin{picture}(400,200)
\put(000,000){\line(400,000)}
\put(000,000){\line(000,200)}
\put(399,000){\line(000,200)}
\put(000,199){\line(400,000)}
\put(000,155){\line(150,-10)}
\put(150,145){\line(140,+7)}
\put(290,152){\line(130,-4)}
\put(150,145){\line(130,-70)}{\line(125,-65)}
\put(150,145){\line(0,-60)}
\end{picture}

  15. 15 Carl Brannen

    \begin{picture}(440,250)
\put(000,000){\line(440,000)}
\put(000,000){\line(000,250)}
\put(439,000){\line(000,250)}
\put(000,249){\line(440,000)}
\put(000,155){\line(150,-10)}
\put(200,145){\line(140,+7)}
\put(340,152){\line(120,-4)}
\put(200,145){\line(130,-70)}
\put(330, 75){\line(125,-65)}
\put(200,145){\line(0,-60)}
\end{picture}

  16. 16 Carl Brannen

    \begin{picture}(440,250)
\put(000,000){\line(440,000)}
\put(000,000){\line(000,250)}
\put(439,000){\line(000,250)}
\put(000,249){\line(440,000)}
\put(000,205){\line(150,-10)}
\put(1500,195){\line(140,+7)}
\put(290,202){\line(120,-4)}
\put(150,195){\line(130,-70)}
\put(280,125){\line(125,-65)}
\put(150,195){\line(0,-60)}
\end{picture}

    Helps to remember the difference between sideways and up.

  17. 17 Carl Brannen

    \begin{picture}(440,250)
\put(000,000){\line(440,000)}
\put(000,000){\line(000,250)}
\put(439,000){\line(000,250)}
\put(000,249){\line(440,000)}
\put(000,205){\line(150,-10)}
\put(150,195){\line(140,+7)}
\put(290,202){\line(120,-4)}
\put(150,195){\line(130,-70)}
\put(280,125){\line(125,-70)}
\put(150,195){\line(0,-60)}
\end{picture}

  18. 18 Carl Brannen

    \begin{picture}(440,250)
\put(000,000){\line(440,000)}
\put(000,000){\line(000,250)}
\put(439,000){\line(000,250)}
\put(000,249){\line(440,000)}
\put(000,205){\line(150,-10)}
\put(150,195){\line(140,+7)}
\put(290,202){\line(120,-4)}
\put(150,195){\line(130,-70)}
\put(280,125){\line(125,-85)}
\put(150,195){\line(0,-60)}
\end{picture}

  19. 19 Carl Brannen

    \begin{picture}(440,250)
(000,000){\line(440,000)}
(000,000){\line(000,250)}
(439,000){\line(000,250)}
(000,249){\line(440,000)}

(000,205;4,2;5){\line(150,-10)}
(000,206;3,2;2){\line(150,-10)}
(000,210;5,0;6){\line(8,40)}
(030,208;5,0;6){\line(8,40)}
(060,206;5,0;6){\line(10,40)}
(090,204;5,0;6){\line(12,40)}
(120,202;5,0;6){\line(12,40)}
(000,205;5,0;6){\line(8,-40)}
(030,203;5,0;6){\line(10,-40)}
(060,201;5,0;6){\line(10,-40)}
(090,199;5,0;6){\line(12,-40)}
(120,197;5,0;6){\line(15,-40)}

(150,195;3,2;3){\line(140,+7)}
(150,196;4,2;1){\line(140,+7)}
(150,195;4,0;10){\line(14,-38)}
(190,197;4,0;10){\line(15,-37)}
(230,199;4,0;15){\line(16,-36)}
(150,199;4,0;10){\line(15,38)}
(190,201;4,0;10){\line(16,37)}
(230,203;4,0;15){\line(16,36)}

(290,202;4,2;3){\line(120,-4)}
(290,203;2,2;1){\line(120,-4)}

(150,195;2,2;3){\line(130,-70)}
(151,196;4,2;2){\line(130,-70)}
(280,125;2,2;3){\line(125,-85)}
(281,126;4,2;2){\line(125,-85)}
(150,195;1,0;5){\line(0,-60)}
\end{picture}

    Fatten up the stems, add needles.

  20. 20 Carl Brannen

    \begin{picture}(440,250)
(000,000){\line(440,000)}
(000,000){\line(000,250)}
(439,000){\line(000,250)}
(000,249){\line(440,000)}

(000,205;4,2;5){\line(150,-10)}
(000,206;3,2;2){\line(150,-10)}
(000,210;5,0;6){\line(8,40)}
(030,208;5,0;6){\line(8,40)}
(060,206;5,0;6){\line(10,40)}
(090,204;5,0;6){\line(12,40)}
(120,202;5,0;6){\line(12,40)}
(000,205;5,0;6){\line(8,-40)}
(030,203;5,0;6){\line(10,-40)}
(060,201;5,0;6){\line(10,-40)}
(090,199;5,0;6){\line(12,-40)}
(120,197;5,0;6){\line(15,-40)}

(150,195;3,2;3){\line(140,+7)}
(150,196;4,2;1){\line(140,+7)}
(150,195;4,0;10){\line(14,-38)}
(190,197;4,0;10){\line(15,-37)}
(230,199;4,0;15){\line(16,-36)}
(150,199;4,0;10){\line(15,38)}
(190,201;4,0;10){\line(16,37)}
(230,203;4,0;15){\line(16,36)}

(290,202;4,2;3){\line(120,-4)}
(290,203;2,2;1){\line(120,-4)}
(290,201;4,0;8){\line(17,-35)}
(322,203;4,0;8){\line(18,-34)}
(354,205;4,0;8){\line(19,-32)}
(290,205;4,0;8){\line(17,35)}
(322,207;4,0;8){\line(18,34)}
(354,209;4,0;8){\line(19,32)}

(150,195;2,2;3){\line(130,-70)}
(151,196;4,2;2){\line(130,-70)}
(280,125;2,2;3){\line(125,-85)}
(281,126;4,2;2){\line(125,-85)}
(150,195;1,0;5){\line(0,-60)}
\end{picture}

    Ooops. Let’s see how many lines we can put on one drawing.

  21. 21 Carl Brannen

    \begin{picture}(440,250)
(000,000){\line(440,000)}
(000,000){\line(000,250)}
(439,000){\line(000,250)}
(000,249){\line(440,000)}

(000,205;4,2;5){\line(150,-10)}
(000,206;3,2;2){\line(150,-10)}
(000,210;5,0;6){\line(8,40)}
(030,208;5,0;6){\line(8,40)}
(060,206;5,0;6){\line(10,40)}
(090,204;5,0;6){\line(12,40)}
(120,202;5,0;6){\line(12,40)}
(000,205;5,0;6){\line(8,-40)}
(030,203;5,0;6){\line(10,-40)}
(060,201;5,0;6){\line(10,-40)}
(090,199;5,0;6){\line(12,-40)}
(120,197;5,0;6){\line(15,-40)}

(150,195;3,2;3){\line(140,+7)}
(150,196;4,2;1){\line(140,+7)}
(150,195;4,0;10){\line(14,-38)}
(190,197;4,0;10){\line(15,-37)}
(230,199;4,0;15){\line(16,-36)}
(150,199;4,0;10){\line(15,38)}
(190,201;4,0;10){\line(16,37)}
(230,203;4,0;15){\line(16,36)}

(290,202;4,2;3){\line(120,-4)}
(290,203;2,2;1){\line(120,-4)}

(290,201;4,0;8){\line(17,-35)}
(322,200;4,0;8){\line(18,-34)}
(354,199;4,0;8){\line(19,-32)}
(290,205;4,0;8){\line(17,35)}
(322,204;4,0;8){\line(18,34)}
(354,203;4,0;8){\line(19,32)}

(150,195;2,2;3){\line(130,-70)}
(151,196;4,2;2){\line(130,-70)}
(280,125;2,2;3){\line(125,-85)}
(281,126;4,2;2){\line(125,-85)}
(150,195;1,0;5){\line(0,-60)}
\end{picture}

  22. 22 Carl Brannen

    \begin{picture}(440,250)
(000,000){\line(440,000)}
(000,000){\line(000,250)}
(439,000){\line(000,250)}
(000,249){\line(440,000)}
(150,195;3,2;3){\line(140,+7)}
(150,196;4,2;1){\line(140,+7)}
(150,195;4,0;10){\line(14,-38)}
(190,197;4,0;10){\line(15,-37)}
(230,199;4,0;15){\line(16,-36)}
(150,199;4,0;10){\line(15,38)}
(190,201;4,0;10){\line(16,37)}
(230,203;4,0;15){\line(16,36)}
(000,205;4,2;5){\line(150,-10)}
(000,206;3,2;2){\line(150,-10)}
(000,210;5,0;6){\line(8,40)}
(030,208;5,0;6){\line(8,40)}
(060,206;5,0;6){\line(10,40)}
(090,204;5,0;6){\line(12,40)}
(120,202;5,0;6){\line(12,40)}
(000,205;5,0;6){\line(8,-40)}
(030,203;5,0;6){\line(10,-40)}
(060,201;5,0;6){\line(10,-40)}
(090,199;5,0;6){\line(12,-40)}
(120,197;5,0;6){\line(15,-40)}
(290,202;4,2;3){\line(96,-3)}
(290,203;2,2;1){\line(96,-3)}
(290,201;4,0;8){\line(17,-35)}
(322,200;4,0;8){\line(18,-34)}
(354,199;4,0;8){\line(19,-32)}
(290,205;4,0;8){\line(17,35)}
(322,204;4,0;8){\line(18,34)}
(354,203;4,0;8){\line(19,32)}
(280,125;2,2;3){\line(125,-85)}
(281,126;4,2;2){\line(125,-85)}
(280,125;4,-2;8){\line(-6,-35)}
(311,104;4,-2;8){\line(-6,-34)}
(342,083;4,-2;8){\line(-4,-33)}
(373,062;4,-2;10){\line(-2,-32)}
(282,127;4,-2;9){\line(26,20)}
(313,106;4,-2;9){\line(26,19)}
(344,085;4,-2;9){\line(26,18)}
(375,064;4,-2;10){\line(26,16)}
(150,195;2,2;3){\line(130,-70)}
(151,196;4,2;2){\line(130,-70)}
(150,195;4,-2;10){\line(-12,-35)}
(190,175;4,-2;10){\line(-10,-35)}
(230,155;4,-2;13){\line( -8,-35)}
(152,197;4,-2;10){\line(24,22)}
(192,177;4,-2;10){\line(25,22)}
(232,157;4,-2;13){\line(26,22)}
(150,195;1,0;2){\line(0,-70)}
(121,111;1,0;4){\line( 19,-79)}
(121,111;0,1;5){\line( 79,-24)}
(140,32;0,1;5){\line( 60,55)}
(112,53;1,0;5){\line( 38,72)}
(112,53;0,1;4){\line( 81,03)}
(150,125;1,0;5){\line( 43,-69)}
\end{picture}

    Let’s see if this blows up the element buffer…

  23. 23 Carl Brannen

    Okay, here’s some advice:

    (1) Read the Mimetex notes on picture, and take advantage of all the features.
    (2) To get decent shading, you have to use the multiput command, which goes something like (x,y;dx,dy;N).
    (3) The practice sandbox over on Mimetex only allows you to draw simple figures, so to practice a complicated figure you have to only draw part of at a time.
    (4) Mimetex is sufficiently different from the usual LaTex language that you should do your drawing in the Mimetex itself, rather than trying to do it in your favorite language and then transfering over.
    (5) Maybe it’s just me, but I had a lot of bit noise. If you figure out how to avoid that, do tell. Maybe I should have scaled things smaller, and got more bits.

  24. 24 Donlad E. Knutz

    \frac{1}{1+ \frac{1}{1+ \frac{1}{1 + \cdots}}}

  25. 25 Clifford

    Yes! My favourite continued fraction!! See here:

    http://asymptotia.com/2006/10/04/irrational-memories/

    -cvj

  26. 26 Plato

    I was wondering whether it was right to place the tools in the sandbox?

    
\huge\textstyle \begin{array}{|l98c28c28|l98c28c28|l98c28c28|} \hline \; \\ \hspace{10}\backslash\textrm{cdot} & \cdot & & \hspace{10}\backslash\textrm{times} & \times & & \hspace{10}\backslash\textrm{ast} & \ast & \\ \hspace{10}\backslash\textrm{div} & \div & & \hspace{10}\backslash\textrm{diamond} & \diamond & & \hspace{10}\backslash\textrm{pm} & \pm & \\ \hspace{10}\backslash\textrm{mp} & \mp & & \hspace{10}\backslash\textrm{oplus} & \oplus & \Bigoplus & \hspace{10}\backslash\textrm{ominus} & \ominus & \\ \hspace{10}\backslash\textrm{otimes} & \otimes & \Bigotimes & \hspace{10}\backslash\textrm{oslash} & \oslash & & \hspace{10}\backslash\textrm{odot} & \odot & \Bigodot \\ \hspace{10}\backslash\textrm{bigcirc} & \bigcirc & & \hspace{10}\backslash\textrm{circ} & \circ & & \hspace{10}\backslash\textrm{bullet} & \bullet & \\ \hspace{10}\backslash\textrm{asymp} & \asymp & & \hspace{10}\backslash\textrm{equiv} & \equiv & & \hspace{10}\backslash\textrm{subseteq} & \subseteq & \\ \hspace{10}\backslash\textrm{supseteq} & \supseteq & & \hspace{10}\backslash\textrm{leq} & \leq & & \hspace{10}\backslash\textrm{geq} & \geq & \\ \hspace{10}\backslash\textrm{preceq} & \preceq & & \hspace{10}\backslash\textrm{succeq} & \succeq & & \hspace{10}\backslash\textrm{sim} & \sim & \\ \hspace{10}\backslash\textrm{approx} & \approx & & \hspace{10}\backslash\textrm{subset} & \subset & & \hspace{10}\backslash\textrm{supset} & \supset & \\ \hspace{10}\backslash\textrm{ll} & \ll & & \hspace{10}\backslash\textrm{gg} & \gg & & \hspace{10}\backslash\textrm{prec} & \prec & \\ \hspace{10}\backslash\textrm{succ} & \succ & & \hspace{10}\normalsize\backslash\textrm{leftarrow} & \leftarrow & & \hspace{10}\normalsize\backslash\textrm{rightarrow} & \rightarrow & \\ \hspace{10}\normalsize\backslash\textrm{uparrow} & \uparrow & & \hspace{10}\normalsize\backslash\textrm{downarrow} & \downarrow & & \hspace{10}\normalsize\backslash\textrm{leftrightarrow}&&\leftrightarrow\\ \hspace{10}\backslash\textrm{nearrow} & \nearrow & & \hspace{10}\backslash\textrm{searrow} & \searrow & & \hspace{10}\backslash\textrm{simeq} & \simeq & \\ \hspace{10}\normalsize\backslash\textrm{Leftarrow} & \Leftarrow & & \hspace{10}\normalsize\backslash\textrm{Rightarrow} & \Rightarrow & & \hspace{10}\normalsize\backslash\textrm{Uparrow} & \Uparrow & \\ \hspace{10}\normalsize\backslash\textrm{Downarrow} & \Downarrow & & \hspace{10}\normalsize\backslash\textrm{Leftrightarrow}&&\Leftrightarrow& \hspace{10}\backslash\textrm{nwarrow} & \nwarrow & \\ \hspace{10}\backslash\textrm{swarrow} & \swarrow & & \hspace{10}\backslash\textrm{propto} & \propto & & \hspace{10}\backslash\textrm{prime} & \prime & \\ \hspace{10}\backslash\textrm{infty} & \infty & & \hspace{10}\backslash\textrm{in} & \in & & \hspace{10}\backslash\textrm{ni} & \ni & \\ \hspace{10}\backslash\textrm{triangle} & \triangle & & \hspace{10}\normalsize\backslash\textrm{bigtriangledown}&&\bigtriangledown& \hspace{10}\backslash^\prime & \’ & \\ \hspace{10}\textrm{/} & / & & \hspace{10}\backslash\textrm{forall} & \forall & & \hspace{10}\backslash\textrm{exists} & \exists & \\ \hspace{10}\backslash\textrm{neg} & \neg & & \hspace{10}\backslash\textrm{emptyset} & \emptyset & & \hspace{10}\backslash\textrm{Re} & \Re & \\ \hspace{10}\backslash\textrm{Im} & \Im & & \hspace{10}\backslash\textrm{top} & \top & & \hspace{10}\backslash\textrm{bot} & \bot & \\ \hspace{10}\backslash\textrm{aleph} & \aleph & & \hspace{10}\normalsize\backslash\textrm{mathcal\lbrace A\rbrace}&\;\mathcal{A}&….& …. \normalsize\backslash\textrm{mathcal\lbrace Z\rbrace}&\;\mathcal{Z}&\\ \; \\ \hline \end{array}

    [Click here for larger image... click again once you get there for full magnification. -cvj]

  27. 27 Plato

    \huge\textstyle \begin{array}{|l98c28c28|l98c28c28|l98c28c28|}    \hline \; \\    \hspace{10}\backslash\textrm{Gamma}      & \Gamma   &\,\,\, \mathbb{\Gamma}  &    \hspace{10}\backslash\textrm{Delta}      & \Delta   & \mathbb{\Delta}  &    \hspace{10}\backslash\textrm{Theta}      & \Theta   & \mathbb{\Theta}  \\    \hspace{10}\backslash\textrm{Lambda}     & \Lambda  & \mathbb{\Lambda} &    \hspace{10}\backslash\textrm{Xi}         & \Xi      & \mathbb{\Xi}     &    \hspace{10}\backslash\textrm{Pi}         & \Pi      & \mathbb{\Pi}     \\    \hspace{10}\backslash\textrm{Sigma}      & \Sigma   & \mathbb{\Sigma}  &    \hspace{10}\backslash\textrm{Upsilon}    & \Upsilon & \mathbb{\Upsilon}&    \hspace{10}\backslash\textrm{Phi}        & \Phi     & \mathbb{\Phi}    \\    \hspace{10}\backslash\textrm{Psi}        & \Psi     & \mathbb{\Psi}    &    \hspace{10}\backslash\textrm{Omega}      & \Omega   & \mathbb{\Omega}  \\    \; \\ \hline \; \\    \hspace{10}\backslash\textrm{alpha}      & \alpha   & \mathbb{\alpha}  &    \hspace{10}\backslash\textrm{beta}       & \beta    & \mathbb{\beta}   &    \hspace{10}\backslash\textrm{gamma}      & \gamma   & \mathbb{\gamma}  \\    \hspace{10}\backslash\textrm{delta}      & \delta   & \mathbb{\delta}  &    \hspace{10}\backslash\textrm{epsilon}    & \epsilon & \mathbb{\epsilon}&    \hspace{10}\backslash\textrm{zeta}       & \zeta    & \mathbb{\zeta}   \\    \hspace{10}\backslash\textrm{eta}        & \eta     & \mathbb{\eta}    &    \hspace{10}\backslash\textrm{theta}      & \theta   & \mathbb{\theta}  &    \hspace{10}\backslash\textrm{iota}       & \iota    & \mathbb{\iota}   \\    \hspace{10}\backslash\textrm{kappa}      & \kappa   & \mathbb{\kappa}  &    \hspace{10}\backslash\textrm{lambda}     & \lambda  & \mathbb{\lambda} &    \hspace{10}\backslash\textrm{mu}         & \mu      & \mathbb{\mu}     \\    \hspace{10}\backslash\textrm{nu}         & \nu      & \mathbb{\nu}     &    \hspace{10}\backslash\textrm{xi}         & \xi      & \mathbb{\xi}     &    \hspace{10}\backslash\textrm{pi}         & \pi      & \mathbb{\pi}     \\    \hspace{10}\backslash\textrm{rho}        & \rho     & \mathbb{\rho}    &    \hspace{10}\backslash\textrm{sigma}      & \sigma   & \mathbb{\sigma}  &    \hspace{10}\backslash\textrm{tau}        & \tau     & \mathbb{\tau}    \\    \hspace{10}\backslash\textrm{upsilon}    & \upsilon & \mathbb{\upsilon}&    \hspace{10}\backslash\textrm{phi}        & \phi     & \mathbb{\phi}    &    \hspace{10}\backslash\textrm{chi}        & \chi     & \mathbb{\chi}    \\    \hspace{10}\backslash\textrm{psi}        & \psi     & \mathbb{\psi}    &    \hspace{10}\backslash\textrm{omega}      & \omega   & \mathbb{\omega}  \\    \; \\ \hline \; \\    \hspace{10}\backslash\textrm{varepsilon} & \varepsilon & &    \hspace{10}\backslash\textrm{vartheta}   & \vartheta   & &    \hspace{10}\backslash\textrm{varpi}      & \varpi      & \\    \hspace{10}\backslash\textrm{varrho}     & \varrho     & &    \hspace{10}\backslash\textrm{varsigma}   & \varsigma   & &    \hspace{10}\backslash\textrm{varphi}     & \varphi     & \\    \; \\ \hline    \end{array}

    [Click here for larger image -cvj]

  28. 28 Plato

    \large    \begin{array}{|c+57|c|c|c0|c|c|c|c|c| C25 C+15} \hline    \large \textrm{a-z} & \small \backslash\textrm{text} &    \small \backslash\textrm{mathbb} & &    \large \textrm{A-Z} & \small \backslash\textrm{text} &    \small \backslash\textrm{mathbb} & \small \backslash\textrm{mathcal} &    \small \backslash\textrm{mathscr} \\ \hline    a&\text{a}&\mathbb{a}& &A&\text{A}&\mathbb{A}&\mathcal{A}&\mathscr{A}\\    b&\text{b}&\mathbb{b}& &B&\text{B}&\mathbb{B}&\mathcal{B}&\mathscr{B}\\    c&\text{c}&\mathbb{c}& &C&\text{C}&\mathbb{C}&\mathcal{C}&\mathscr{C}\\    d&\text{d}&\mathbb{d}& &D&\text{D}&\mathbb{D}&\mathcal{D}&\mathscr{D}\\    e&\text{e}&\mathbb{e}& &E&\text{E}&\mathbb{E}&\mathcal{E}&\mathscr{E}\\    f&\text{f}&\mathbb{f}& &F&\text{F}&\mathbb{F}&\mathcal{F}&\mathscr{F}\\    g&\text{g}&\mathbb{g}& &G&\text{G}&\mathbb{G}&\mathcal{G}&\mathscr{G}\\    h&\text{h}&\mathbb{h}& &H&\text{H}&\mathbb{H}&\mathcal{H}&\mathscr{H}\\    i&\text{i}&\mathbb{i}& &I&\text{I}&\mathbb{I}&\mathcal{I}&\mathscr{I}\\    j&\text{j}&\mathbb{j}& &J&\text{J}&\mathbb{J}&\mathcal{J}&\mathscr{J}\\    k&\text{k}&\mathbb{k}& &K&\text{K}&\mathbb{K}&\mathcal{K}&\mathscr{K}\\    l&\text{l}&\mathbb{l}& &L&\text{L}&\mathbb{L}&\mathcal{L}&\mathscr{L}\\    m&\text{m}&\mathbb{m}& &M&\text{M}&\mathbb{M}&\mathcal{M}&\mathscr{M}\\    n&\text{n}&\mathbb{n}& &N&\text{N}&\mathbb{N}&\mathcal{N}&\mathscr{N}\\    o&\text{o}&\mathbb{o}& &O&\text{O}&\mathbb{O}&\mathcal{O}&\mathscr{O}\\    p&\text{p}&\mathbb{p}& &P&\text{P}&\mathbb{P}&\mathcal{P}&\mathscr{P}\\    q&\text{q}&\mathbb{q}& &Q&\text{Q}&\mathbb{Q}&\mathcal{Q}&\mathscr{Q}\\    r&\text{r}&\mathbb{r}& &R&\text{R}&\mathbb{R}&\mathcal{R}&\mathscr{R}\\    s&\text{s}&\mathbb{s}& &S&\text{S}&\mathbb{S}&\mathcal{S}&\mathscr{S}\\    t&\text{t}&\mathbb{t}& &T&\text{T}&\mathbb{T}&\mathcal{T}&\mathscr{T}\\    u&\text{u}&\mathbb{u}& &U&\text{U}&\mathbb{U}&\mathcal{U}&\mathscr{U}\\    v&\text{v}&\mathbb{v}& &V&\text{V}&\mathbb{V}&\mathcal{V}&\mathscr{V}\\    w&\text{w}&\mathbb{w}& &W&\text{W}&\mathbb{W}&\mathcal{W}&\mathscr{W}\\    x&\text{x}&\mathbb{x}& &X&\text{X}&\mathbb{X}&\mathcal{X}&\mathscr{X}\\    y&\text{y}&\mathbb{y}& &Y&\text{Y}&\mathbb{Y}&\mathcal{Y}&\mathscr{Y}\\    z&\text{z}&\mathbb{z}& &Z&\text{Z}&\mathbb{Z}&\mathcal{Z}&\mathscr{Z}\\    \hline \end{array}

    [Click here for larger image. -cvj]

  29. 29 Mouseover

    Delete after implementation.

    When you put mouse cursor over top of images one notices the latex language written.

    IN the “upper three boxes” you wouldn’t want to see the whole box, yet in image production it’s not a bad idea.

    This information is specified to a certain “title” html length, so we only see so much of the title aspect of that language. Can you increase the “title length” to include however large that image or equation is, to include all of the latex language?

    Also, the duration time of appearance of “title length” to allow for a greater absorption time.

    Thanks

  30. 30 Clifford

    Where do I implement that change of length and duration, mr/ms mouseover? And syntax?

    Thanks,

    -cvj

  31. 31 dasdasf

    \frac {d^2x} {dt^2} * \frac {dx} {dt} = -kx *\frac {dx} {dt}

  32. 32 Amara

    P = \sqrt {\frac{{4\pi ^2 a^3 }}{{GM_S }}}

  33. 33 Carl Brannen

    A_n = (n-1)!\left(1 + \sum_{k=2}^{n-2}\frac{A_k}{k!}\right)

  34. 34 Carl Brannen

    \frac{A_n}{n!} = \frac{1}{n}\left(1 + \sum_{k=2}^{n-2}\frac{A_k}{k!}\right)

  35. 35 Carl Brannen

    B(x) = \sum_{n=0}^{n=\infty}x^n B(x)

  36. 36 Carl Brannen

    B(x) = \int x B’ \;dx + x^2B(x)

  37. 37 Carl Brannen

    B(x) = \int x \frac{dB}{dx} \;dx + x^2B(x)

  38. 38 Tester John

    [ tex] (LaTeX-like commands go here) \delta [ /tex]

  39. 39 Plato
  40. 40 Plato

    Help!

    1 \begin{fmfgraph*}(50,60)
 2  \fmfbottom{P1,P2} \fmftop{P1′,H’,P2′}
 3  \fmf{fermion,tension=2,lab=$P_1$}{P1,g1}
 4  \fmf{fermion,tension=2,lab=$P_2$}{P2,g2}
 5  \fmfblob{.16w}{g1,g2}
 6  \fmf{gluon,lab.side=right,
 7      lab=$x_1P_1$}{g1,v1}
 8  \fmf{gluon,lab.side=right,
 9     lab=$x_2P_2$}{v2,g2}
10  \fmf{fermion,tension=.6}{H,v1,v2,H}
11  \fmfdot{H,v1,v2}
12  \fmf{dbl_dots,lab=$H$}{H,H’}
13  \fmf{fermion}{g1,P1′}
14  \fmf{fermion}{g2,P2′}
15  \fmfv{lab=$g(x_1,,Q^2)$,lab.dist=.1w}{g1}
16  \fmfv{lab=$g(x_2,,Q^2)$,lab.dist=.1w}{g2}
17  \fmffreeze
18  \renewcommand{\P}[3]{\fmfi{plain}{%
19    vpath(__#1,__#2) shifted (thick*(#3))}}
20  \P{P1}{g1}{2,0} \P{P1}{g1}{-2,1}
21  \P{P2}{g2}{2,1} \P{P2}{g2}{-2,0}
22  \P{g1}{P1′}{-2,-1} \P{g1}{P1′}{2,0}
23  \P{g2}{P2′}{-2,0} \P{g2}{P2′}{2,-1}
24 \end{fmfgraph*}

  41. 41 Plato

    last one sorry

    \picture(size){pic_elems}
 \begin{fmfgraph*}(50,60)
   \fmfbottom{P1,P2} \fmftop{P1′,H’,P2′}
   \fmf{fermion,tension=2,lab=$P_1$}{P1,g1}
   \fmf{fermion,tension=2,lab=$P_2$}{P2,g2}
   \fmfblob{.16w}{g1,g2}
   \fmf{gluon,lab.side=right,
       lab=$x_1P_1$}{g1,v1}
   \fmf{gluon,lab.side=right,
      lab=$x_2P_2$}{v2,g2}
  \fmf{fermion,tension=.6}{H,v1,v2,H}
  \fmfdot{H,v1,v2}
 \fmf{dbl_dots,lab=$H$}{H,H’}
  \fmf{fermion}{g1,P1′}
  \fmf{fermion}{g2,P2′}
  \fmfv{lab=$g(x_1,,Q^2)$,lab.dist=.1w}{g1}
  \fmfv{lab=$g(x_2,,Q^2)$,lab.dist=.1w}{g2}
  \fmffreeze
  \renewcommand{\P}[3]{\fmfi{plain}{%
    vpath(__#1,__#2) shifted (thick*(#3))}}
  \P{P1}{g1}{2,0} \P{P1}{g1}{-2,1}
  \P{P2}{g2}{2,1} \P{P2}{g2}{-2,0}
  \P{g1}{P1′}{-2,-1} \P{g1}{P1′}{2,0}
  \P{g2}{P2′}{-2,0} \P{g2}{P2′}{2,-1}
 \end{fmfgraph*}

  42. 42 'nonymous

    3SAT \in NP \\ P

  43. 43 'nonymous

    3SAT \in NP \setminus P

  44. 44 'nonymous

    3SAT \in NP \setminus P

  45. 45 Carl Brannen

    \left(\begin{array}{cc}1&0\&0\end{array}\right)
    \frac{1}{2}\left(\begin{array}{cc}1&1\\1&1\end{array}\right)

    and twice their product:

    \left\begin{array}{cc}1&0\\1&0\end{array}\right)

  46. 46 Carl Brannen

    \left(\begin{array}{cc}1&0\&0\end{array}\right)

  47. 47 Carl Brannen

    Hmmm. Latex matrices aren’t working anymore…

    \left|   \begin{matrix} a_1 & a_2 \\ 
          b_1 & b_2 \end{matrix}   \right|

  48. 48 Carl Brannen

    \left(\begin{matrix}1&0\&0\end{array}\right)
    \frac{1}{2}\left(\begin{matrix}1&1\\1&1\end{array}\right)

    and twice their product:

    \left\begin{matrix}1&0\\1&0\end{array}\right)

  49. 49 Carl Brannen

    \left| \begin{matrix}1&0\&0\end{matrix} \right|
    \frac{1}{2} \left| \begin{matrix}1&1\\1&1\end{marix} \right|

    and twice their product:

    \left|  begin{matrix}1&0\\1&0\end{matrix} \right|

  50. 50 Carl Brannen

    \left( \begin{matrix}1&0\&0\end{matrix} \right)

    \frac{1}{2} \left( \begin{matrix}1&1\\1&1\end{matrix} \right)

    and twice their product:

    \left(  \begin{matrix}1&0\\1&0\end{matrix} \right)

    what a pain

  51. 51 Carl Brannen

     \left( \begin{matrix}1&0\&0\end{matrix}  \right)

    \frac{1}{2} \left( \begin{matrix}1&1\\1&1\end{matrix} \right)

    and twice their product:

    \left(  \begin{matrix}1&0\\1&0\end{matrix} \right)

  52. 52 Carl Brannen

    \frac{1}{2} \left( \begin{matrix}2&0\&0\end{matrix} \right)

    \frac{1}{2} \left( \begin{matrix}1&1\\1&1\end{matrix} \right)

    and twice their product:

    \left(  \begin{matrix}1&0\\1&0\end{matrix} \right)

  53. 53 Carl Brannen

    \frac{1}{2} \left( \begin{matrix}1&1\\1&1\end{matrix} \right)

    \frac{1}{2} \left( \begin{matrix}1&1\\1&1\end{matrix} \right)

    and twice their product:

    \left(  \begin{matrix}1&0\\1&0\end{matrix} \right)

  54. 54 Carl Brannen

    Dude, your LaTex is seriously broken…

    \left( \begin{matrix}1.0&0.0\.0&0.0\end{matrix} \right)

    \left( \begin{matrix}0.5&0.5\.5&0.5\end{matrix} \right)

    and twice their product is the non Hermitian projection operator:

    \left( \begin{matrix}1.0&0.0\.0&0.0\end{matrix} \right)

  55. 55 [tex]\sigma[/tex]

    \sigma

  56. 56 Carl Brannen

    \begin{array}{rcl|r}\ddot{x} &=&-\sqrt{2}\dot{x}(\dot{x}^2+\dot{y}^2)/r^{1.5}&1.5\\&&+1.5\sqrt{2}\dot{x}(x\dot{x}+y\dot{y})^2/r^{3.5}&1.5\\ \hline&&-x/r^3&2.0\\&&+3x(x\dot{x}+y\dot{y})^2/r^5&2.0\\&&-2\dot{y}(x\dot{y}-y\dot{x})/r^3&2.0\\ \hline&&+3\sqrt{2}\dot{x}/r^{2.5}&2.5\\&&+2\sqrt{2}y(x\dot{y}-y\dot{x})/r^{4.5}\;\;\;\;\;&2.5\\ \hline&&+2x/r^4&3.0\\ \hline\end{array}

    \begin{array}{rcl|r}\ddot{y} &=&-\sqrt{2}\dot{y}(\dot{x}^2+\dot{y}^2)/r^{1.5}&1.5\\&&+1.5\sqrt{2}\dot{y}(x\dot{x}+y\dot{y})^2/r^{3.5}&1.5\\ \hline&&-y/r^3&2.0\\&&+3y(x\dot{x}+y\dot{y})^2/r^5&2.0\\&&+2\dot{x}(x\dot{y}-y\dot{x})/r^3&2.0\\ \hline&&+3\sqrt{2}\dot{y}/r^{2.5}&2.5\\&&-2\sqrt{2}x(x\dot{y}-y\dot{x})/r^{4.5}\;\;\;\;\;&2.5\\ \hline&&+2y/r^4&3.0\\ \hline\end{array}

  57. 57 it

    Just checking…
    $\nabla \psi = \left( \begin{array}[c] \partial_1 \psi \\ \vdots \\ \partial_N\psi\end{array}\right)$

  58. 58 Hank

    This is a lot of fun. How can you do LaTeX in high resolution in order to make a t-shirt with equations on them?

    My graphics program doesn’t have Greek lettering or that kind of formatting.

    Best,

    Hank

  59. 59 a

    1

    2

    \sqrt{3}

    \sqrt{2}

  60. 60 Rusty

    $\xymatrix{
& R \ar@{-}[d] & \\
& \ar@{-}[dl] A + I \ar@{-}@[dr] \ar@{~}@[dr]& \\
A \ar@{-}@[dr] \ar@{~}@[dr]& & I\ar@{-}[dl] \\
& A \cap I &
}$

  61. 61 Zhuf

    \[ \begin{array}{ll}
    E & = \sum_I \left(y'_i-y_i\right)^2 \\
    & = \sum_I \left(mx_i+c-y_i\right) \\
    & = \sum_I \left(mx_i+c\right)^2 + \sum_I y_i^2 + 2\sum_I \left(mx_i+c\right)y_i \\ \]

  62. 62 Zhuf

    oops wrong tag >

  63. 63 Zhuf

     \begin{array}{ll}
E & = \sum_I \left(y’_i-y_i\right)^2 \\
& = \sum_I \left(mx_i+c-y_i\right) \\
& = \sum_I \left(mx_i+c\right)^2 + \sum_I y_i^2 + 2\sum_I \left(mx_i+c\right)y_i \\

  64. 64 Zhuf

     \[ \begin{array}{ll}
E & = \sum_I \left(y'_i-y_i\right)^2 \\
& = \sum_I \left(mx_i+c-y_i\right) \\
& = \sum_I \left(mx_i+c\right)^2 + \sum_I y_i^2 + 2\sum_I \left(mx_i+c\right)y_i \\ \]

  65. 65 Zhuf

    Hmm?
     P\left(A|B\right) = \frac {P\left(B|A\right)P\left(A)\right)} {P\left(B\right)}

  66. 66 Ryan Vilim

     e^{-x/2} \text{Ai}\left(\frac{\frac{1}{4}-l x}{(-l)^{2/3}}\right)
    C+e^{-x/2} \text{Bi}\left(\frac{\frac{1}{4}-l x}{(-l)^{2/3}}\right)D

    Not for anything, just sending an email and have no latex installed

  67. 67 test

    [tex][tex]

  68. 68 sasa

     12 + \sqrt(12) = 7 
\begin{gather}12 + \sqrt(12) = 7 \end{gather}

  69. 69 rob

    g_{ab} = \left(\begin{array}{cc} \frac{{\Delta-a^2 sin^2\theta}}{\rho^2} & 0 & 0 & \frac{2a sin^2\theta (r^2+a^2-\Delta}}{\rho^2} \\ 0 & -\frac{\rho^2}{\Delta} & 0 & 0 \\ 0 & 0 & \rho^2 & 0 \\ \frac{2a sin^2\theta (r^2+a^2-\Delta}}{\rho^2} & 0 & 0 & \frac{sin^2 \theta (\Delta a^2 -(r^2 + a^2)^2}{\rho^2} \end{array}\right)

  70. 70 rob

    g_{ab} = \left(\begin{array}{cccc} \frac{{\Delta-a^2 sin^2\theta}}{\rho^2} & 0 & 0 & \frac{2a sin^2\theta (r^2+a^2-\Delta}}{\rho^2} \\ 0 & -\frac{\rho^2}{\Delta} & 0 & 0 \\ 0 & 0 & \rho^2 & 0 \\ \frac{2a sin^2\theta (r^2+a^2-\Delta}}{\rho^2} & 0 & 0 & \frac{sin^2 \theta (\Delta a^2 -(r^2 + a^2)^2}{\rho^2} \end{array}\right)

  71. 71 yrst

    \newcommand{\nucl}[3]{
    \ensuremath{
    \phantom{\ensuremath{^{#1}_{#2}}}
    \llap{\ensuremath{^{#1}}}
    \llap{\ensuremath{_{\rule{0pt}{.75em}#2}}}
    \mbox{#3}
    }
    }
    \nucl{n}{0}{1}

  72. 72 el loco

    \int (x^2+1)^2

  73. 73 Plato

    Gravity and the Photon

    The relativistic energy expression attributes a mass to any energetic particle, and for the photon

    E=mc^2=hv

    The gravitational potential energy is then

    \LARGE U=\frac{-GMm}r=\frac{-GMh}{rc^2}{vo}

    When the photon escapes the gravity field, it will have a different frequency

    \large hv=hv_o[{1-}\frac{GM}{rc^2}] \hspace9  v=v_o[{1-}\frac{GM}{rc^2}] \hspace9 \frac{\bigtriangledown v} {v_o}={-}\frac{GM}{rc^2}

    Since it is reduced in frequency, this is called the gravitational red shift or the Einstein red shift.

    ————————————————–
    Escape Energy for Photon

    If the gravitational potential energy of the photon is exactly equal to the photon energy then

    \normal hv_o=\frac{GM}{rc^2}{v_o} \hspace9 \text or r=\frac {GM}{c^2}\\ \text so if Mass M collapses to radius r a photon will be redshifted to zero frequency

    Note that this condition is independent of the frequency, and for a given mass M establishes a critical radius. Actually, Schwarzchilds’s calculated gravitational radius differs from this result by a factor of 2 and is coincidently equal to the non-relativistic escape velocity expression

    [tex]v_e_s_c_a_p_e_ = \sqrt {\frac{2GM}{r}} \hspace9 \\ \text which if V is set equal\\to c gives a radius r=\frac {2GM}{c^2}\hspace9 \text Schwarzchild Radius[\tex]

    This equivalence is used as a mnenomic, but does not imply this is a valid way to derive the Schwarzchild Radius

    You can delete from your tipping light thread. Have a nice day. I acknowledge fully I am the student. While we see tipping light cones there is an actual qualitative understanding for the determination of the blackhole in this context?

  74. 74 Nathan

    \frac{\deltaI_{0}}{I_{0}}

  75. 75 dog

    \`{a} bient\^{o} = à bientô

  76. 76 Zylinder

    f(r, \phi, z)=\left(\array{rcos(\phi)\\rsin(\phi)\\z}\right)

    f’(r,\phi, z)= \left(\matrix{cos(\phi)&-rsin(\phi)&0 \cr sin(\phi)&rcos(\phi)&0 \cr 0&0&1}\right)

  77. 77 Plareplane

    For Tom Petty
    
\int_1^{15} xe^(ax) dx = xe^(ax)/a - e^(ax)/a^2 \rvert_1^{15} = (15e^(a15)/a - e^(a15)/a^2) - (e^a/a - e^a/a^2)

  78. 78 erik

    (\f.(\x.f (x x)) (\x.f (x x))

  79. 79 test

    \begin{eqnarray}
    E &=& mc^2 \\
    m &=& \frac{m_0}{\sqrt{1-\frac{v^2}{c^2}}}
    \end{eqnarray}

  80. 80 Pepe

     \vec{a}

  81. 81 Cozmo

    =f(\tau)

  82. 82 Cozmo

    =f(\tau)

  83. 83 test

    sum_{k=1}^n k!

  84. 84 test

    [tex]\displaystyle \sum_{k=1}^{n} k! [\tex]

  85. 85 test

    \displaystyle \sum_{k=1}^{n} k!

  86. 86 Payman

    a test \frac{x}{y}

  87. 87 Frank

    Hallo!!
    Trying to quote

  88. 88 Frank

    Quote

  89. 89 yosef

    \star

    \bigstar

  90. 90 Yosef

    

\star

\bigstar

  91. 91 Yosef

    
   \star \star \star

    
    \bigtriangledown

    
   \bigtriangle

  92. 92 Yosef

    \stackrel{\bigtriangle}{bigtriangledown}

    
   \stackrel{\bigtriangle}{bigtriangledown}

  93. 93 Yosef

    \stackrel{\bigtriangle}{\bigtriangledown}
    
\stackrel{\bigtriangle}{\bigtriangledown}

  94. 94 Yosef

    \buildrel{\bigtriangle}{\bigtriangledown}
    
\ buildrel{\bigtriangle}{\bigtriangledown}

  95. 95 Yosef

    
   \bigtriangle \hspace{-10pt} \bigtriangledown

  96. 96 Yosef

    
   \bigtriangle \hspace{-5pt} \bigtriangledown

  97. 97 bobo

    N = q_1, q_2, q_3, …, q_s \Rightarrow p_i \neq q_j \forall i,j \in {1,2,3,…}

  98. 98 mao

     C_4 [g^{\mu\nu} g^{\rho\sigma} + g^{\mu\rho} g^{\nu\sigma} + g^{\mu\sigma} g^{\nu\rho}] \int {d^d q q^4 f(q^2)}

  99. 99 David

    This is a test: n^{-2}(n\sigma^2) = \sigma^2/(2n)

  100. 100 David

    Oops: n^{-2}(n\sigma^2) = \sigma^2/(2n)

  101. 101 Davd

    n^{-2}(n\sigma^2) = \sigma^2/{2n}

  102. 102 me

    $$sin\left( \frac{7\,pi}{8}\right) $$

  103. 103 brennan

    \int_a^b\left[\int_a^b\left|\begin{array}{cc}
f(x) & g(x) \\
f(y) & g(y)\end{array}\right|^2\,d\alpha(x)\right]\,d\alpha(y)

  104. 104 me

    test

  105. 105 me

    \begin{tabular}{|l|l|l|}
    \hline
    \multicolumn{3}{|c|}{Team sheet} \\
    \hline
    Goalkeeper & GK & Paul Robinson \\ \hline
    \multirow{4}{*}{Defenders} & LB & Lucus Radebe \\
    & DC & Michael Duberry \\
    & DC & Dominic Matteo \\
    & RB & Didier Domi \\ \hline
    \multirow{3}{*}{Midfielders} & MC & David Batty \\
    & MC & Eirik Bakke \\
    & MC & Jody Morris \\ \hline
    Forward & FW & Jamie McMaster \\ \hline
    \multirow{2}{*}{Strikers} & ST & Alan Smith \\
    & ST & Mark Viduka \\
    \hline
    \end{tabular}

  106. 106 azn

    [tex]$\displaystyle{\lim_{n \rightarrow \infty} \sum_{i=1}^{n}{\left(\frac{8}{n} \cdot f(-1+\frac{8}{n} i)\right)}}$[\tex]

  107. 107 azn

    [tex]\displaystyle{\lim_{n \rightarrow \infty} \sum_{i=1}^{n}{\left(\frac{8}{n} \cdot f(-1+\frac{8}{n} i)\right)}}[\tex]

  108. 108 test

    $$\vec(v)=\dot{\theta}\sqrt{\genfrac{}{}{}{0}{v^2}{\rho}}$$

  109. 109 test

    $$\vec(v)=\dot{\theta}\sqrt{\genfrac{}{}{}{0}{v^2}{\rho}}$$

  110. 110 test

    $$\vec(v)=\dot{\theta}\sqrt{\frac{v^2}{\rho}}$$

  111. 111 test

    $$\vec{v}=\dot{\theta}\sqrt{\frac{v^2}{\rho}}$$

  112. 112 test

    $$\vec{v}=\dot{\theta}\sqrt{\frac{v^2}{\rho}}$$
    test

  113. 113 Michael

    Dirichlet Conditions lead to Sines for X
    Neumann Conditions lead to Cosines for X

  114. 114 jay

    [.tex]test[/tex]

  115. 115 jay

    [code]test[/code]

  116. 116 Philip Maton

    \begin{array}{c | c c c c}
    \mbox{eye colour} & blue & green & brown & grey \
    \hline
    blue & 10&5&2&1\
    green & 5&10&3&2\
    brown & 2&3&10&4\
    grey & 1&2&4&10\
    \end{array}

  117. 117 eismcsqrd

    he he this is cool, wish i saw this before doing my stings project in latex!
    love this website tho!!!

  118. 118 eismcsqrd

    oh i mean ’strings project’ not sting….i guess i have written the word far too many times, its escaped my memory as to how to spell it! oops!!

  119. 119 Philip

    \font\newfont=cmr10 at 12pt
    \newfont
    \nopagenumbers
    \phantom{a}
    \vskip2cm
    \magnification 1200
    \centerline{\bf CAIUS MATHEMATICIANS}
    \bigskip
    \centerline{\bf END OF EXAMS PARTY}
    \vskip1cm

    \centerline{Come and have some wine, strawberies etc.} \vskip1cm
    \centerline{Harvey Court Garden and Dinning Room, Monday 8 June, 4 — 6.30.}
    \bigskip

    \centerline{See you there!}
    \bigskip
    \bigskip
    \bigskip
    %\noindent

    \hfill EJB\par
    \hfill JS\phantom{J}\par
    \end

  120. 120 Bliggity

    P(f, a | e) = prod_i P(a_i = j | |e|) * P(f_i | e_j)

  121. 121 Author

    P(f, a | e) = prod_i P(a_i = j | |e|) * P(f_i | e_j)

  122. 122 rr

    [ tex] (LaTeX-like commands go here) [ /tex]

  123. 123 rr

    [ tex]x^3[ /tex]

  124. 124 rr

    x^3

  125. 125 jenkins

    p(\frac{desired outcomes}{possible outcomes})

  126. 126 Bliggity

    $latex \[
    \frac{y+z/2}{y^{2}+1}
    \] $$

  127. 127 nick

    \hat{p}+\frac{1}{2n}z_{1-\alpha/2}^{2} + z_{1-\alpha/2}^{2}\sqrt{\frac{\hat{p}(1-\hat{p})}{n}-\frac{z_{1-\alpha/2}}{4n^{2}}}

  128. 128 antidesitter

     
\frac{1}{2} \, m^2 \varphi^2

  129. 129 Diego

    \begin{center}
\begin{tabular}{ccc}	
\hline
 &$m_{i}$ [g] & $m_{f}$ [g] \\
\hline\hline
 1 &$54.45\pm 0.05$ & $54.13\pm 0.05$ \\
\hline
\end{tabular}
\end{center}

  130. 130 Fel

    \begin{equation}
    m \lambda = sin \theta
    \end{equation}

  131. 131 marco

    (A \left( \cases{\cases{0&$t\leq 0$\cr {\frac {1}{1536}}\, \left( 256\,{\pi }^{3}{t}^{3}+3\,{T}^{3}\sin \left( 8\,{\frac {\pi \,t}{T}} \right) -24\,{T}^{2}t\pi  \right) {\pi }^{-3}&$t\leq 1/4\,T$\cr {\frac {1}{768}}\,{\frac {T \left( 96\,{\pi }^{2}{t}^{2}-24\,{\pi }^{2}Tt-3\,{T}^{2}+2\,{\pi }^{2}{T}^{2} \right) }{{\pi }^{2}}}&$1/4\,T<t$\cr}&$0<1/4\,T$\cr \cases{0&$t\leq 1/4\,T$\cr {\frac {1}{1536}}\, \left( -256\,{\pi }^{3}{t}^{3}-3\,{T}^{3}\sin \left( 8\,{\frac {\pi \,t}{T}} \right) +192\,{\pi }^{3}T{t}^{2}-48\,{T}^{2}t{\pi }^{3}+24\,{T}^{2}t\pi -6\,{T}^{3}\pi +4\,{T}^{3}{\pi }^{3} \right) {\pi }^{-3}&$t\leq 0$\cr {\frac {1}{768}}\,{\frac {T \left( 96\,{\pi }^{2}{t}^{2}-24\,{\pi }^{2}Tt-3\,{T}^{2}+2\,{\pi }^{2}{T}^{2} \right) }{{\pi }^{2}}}&$0<t$\cr}&otherwise\cr}-\cases{\cases{0&$t\leq 1/4\,T$\cr -{\frac {1}{1536}}\, \left( -256\,{\pi }^{3}{t}^{3}-3\,{T}^{3}\sin \left( 8\,{\frac {\pi \,t}{T}} \right) +192\,{\pi }^{3}T{t}^{2}-48\,{T}^{2}t{\pi }^{3}+24\,{T}^{2}t\pi -6\,{T}^{3}\pi +4\,{T}^{3}{\pi }^{3} \right) {\pi }^{-3}&$t\leq 1/2\,T$\cr {\frac {1}{768}}\,{\frac {T \left( 96\,{\pi }^{2}{t}^{2}-72\,{\pi }^{2}Tt-3\,{T}^{2}+14\,{\pi }^{2}{T}^{2} \right) }{{\pi }^{2}}}&$1/2\,T<t$\cr}&$1/4\,T<1/2\,T$\cr \cases{0&$t\leq 1/2\,T$\cr {\frac {1}{1536}}\, \left( -256\,{\pi }^{3}{t}^{3}+384\,{\pi }^{3}T{t}^{2}-3\,{T}^{3}\sin \left( 8\,{\frac {\pi \,t}{T}} \right) -192\,{T}^{2}t{\pi }^{3}+24\,{T}^{2}t\pi -12\,{T}^{3}\pi +32\,{T}^{3}{\pi }^{3} \right) {\pi }^{-3}&$t\leq 1/4\,T$\cr {\frac {1}{768}}\,{\frac {T \left( 96\,{\pi }^{2}{t}^{2}-72\,{\pi }^{2}Tt-3\,{T}^{2}+14\,{\pi }^{2}{T}^{2} \right) }{{\pi }^{2}}}&$1/4\,T<t$\cr}&otherwise\cr}-\cases{\cases{0&$t\leq 1/2\,T$\cr -{\frac {1}{1536}}\, \left( -256\,{\pi }^{3}{t}^{3}+384\,{\pi }^{3}T{t}^{2}-3\,{T}^{3}\sin \left( 8\,{\frac {\pi \,t}{T}} \right) -192\,{T}^{2}t{\pi }^{3}+24\,{T}^{2}t\pi -12\,{T}^{3}\pi +32\,{T}^{3}{\pi }^{3} \right) {\pi }^{-3}&$t\leq 3/4\,T$\cr {\frac {1}{768}}\,{\frac {T \left( 96\,{\pi }^{2}{t}^{2}-120\,{\pi }^{2}Tt-3\,{T}^{2}+38\,{\pi }^{2}{T}^{2} \right) }{{\pi }^{2}}}&$3/4\,T<t$\cr}&$1/2\,T<3/4\,T$\cr \cases{0&$t\leq 3/4\,T$\cr {\frac {1}{1536}}\, \left( -256\,{\pi }^{3}{t}^{3}+576\,{\pi }^{3}T{t}^{2}-3\,{T}^{3}\sin \left( 8\,{\frac {\pi \,t}{T}} \right) -432\,{T}^{2}t{\pi }^{3}+24\,{T}^{2}t\pi +108\,{T}^{3}{\pi }^{3}-18\,{T}^{3}\pi  \right) {\pi }^{-3}&$t\leq 1/2\,T$\cr {\frac {1}{768}}\,{\frac {T \left( 96\,{\pi }^{2}{t}^{2}-120\,{\pi }^{2}Tt-3\,{T}^{2}+38\,{\pi }^{2}{T}^{2} \right) }{{\pi }^{2}}}&$1/2\,T<t$\cr}&otherwise\cr}+\cases{\cases{0&$t\leq 3/4\,T$\cr -{\frac {1}{1536}}\, \left( -256\,{\pi }^{3}{t}^{3}+576\,{\pi }^{3}T{t}^{2}-3\,{T}^{3}\sin \left( 8\,{\frac {\pi \,t}{T}} \right) -432\,{T}^{2}t{\pi }^{3}+24\,{T}^{2}t\pi +108\,{T}^{3}{\pi }^{3}-18\,{T}^{3}\pi  \right) {\pi }^{-3}&$t\leq T$\cr {\frac {1}{768}}\,{\frac {T \left( 96\,{\pi }^{2}{t}^{2}-168\,{\pi }^{2}Tt-3\,{T}^{2}+74\,{\pi }^{2}{T}^{2} \right) }{{\pi }^{2}}}&$T<t$\cr}&$3/4\,T<T$\cr \cases{0&$t\leq T$\cr {\frac {1}{1536}}\, \left( -256\,{\pi }^{3}{t}^{3}+768\,{\pi }^{3}T{t}^{2}-3\,{T}^{3}\sin \left( 8\,{\frac {\pi \,t}{T}} \right) -768\,{T}^{2}t{\pi }^{3}+24\,{T}^{2}t\pi -24\,{T}^{3}\pi +256\,{T}^{3}{\pi }^{3} \right) {\pi }^{-3}&$t\leq 3/4\,T$\cr {\frac {1}{768}}\,{\frac {T \left( 96\,{\pi }^{2}{t}^{2}-168\,{\pi }^{2}Tt-3\,{T}^{2}+74\,{\pi }^{2}{T}^{2} \right) }{{\pi }^{2}}}&$3/4\,T<t$\cr}&otherwise\cr} \right) )

  132. 132 test

    test

  133. 133 Plato

    \left|\uparrow\uparrow\right\rangle, \left|\uparrow\downarrow\right\rangle, \left|\downarrow\uparrow\right\rangle, \left|\downarrow\downarrow\right\rangle

    To construct all possible states of two qubits one can add the four possibilities.

  1. 1 LaTeX Holiday Fun! - Asymptotia