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Jack Halford 2024-06-05 22:49:59 +02:00
parent 2388180ede
commit 17d835b692
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22 changed files with 626 additions and 581 deletions

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@ -161,3 +161,11 @@ to $-1/r^n$ with $n > 2$.
<!-- (m1+m2)x+m2) sin = constant, -->
<!-- (2) -->
<!-- which expresses the fact that the centre of mass of the system does not move horizontally. -->
<!-- Using (1), we find the energy in the form -->
<!-- E -->
<!-- (3) -->
<!-- Hence -->
<!-- Expressing the co-ordinates X2 sin o, y = l cos of the particle m2 in terms of -->
<!-- by means of (2), we find that its path is an arc of an ellipse with horizontal semi- -->
<!-- axis lm1/(m1+m2) and vertical semi-axis l. As M1 8 we return to the familiar simple pen- -->
<!-- dulum, which moves in an arc of a circle. -->

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1/equations/15.1.tex Normal file
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U=-\alpha/r

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1/equations/15.10.tex Normal file
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r=a(1-e\cos\xi),\qquad t=\sqrt{ma^3/\alpha}(\xi-e\sin\xi),

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1/equations/15.11.tex Normal file
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x=a(\cos\xi-e),\qquad y=a\sqrt{q-e^2}\sin\xi

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1/equations/15.12.tex Normal file
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\begin{align}
r &= a(e\ch\xi-1), & t&=\sqrt{ma^3/\alpha}(e\sh\xi-\xi), \\
x &= a(e-\ch\xi)), & t&=a\sqrt{e^2-1}\sh\xi,
\end{align}

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1/equations/15.13.tex Normal file
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U=\alpha/r,\quad(\alpha\gt0)

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1/equations/15.14.tex Normal file
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p/r=-1+e\cos\phi

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1/equations/15.15.tex Normal file
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r_\min=p/(e-1)=a(e+1)

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1/equations/15.16.tex Normal file
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\begin{align}
r &= a(e\ch\xi+1), & t&=\sqrt{ma^3/\alpha}(e\sh\xi+\xi), \\
x &= a(\ch\xi+e)), & t&=a\sqrt{e^2-1}\sh\xi,
\end{align}

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1/equations/15.17.tex Normal file
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\v{v}\times\v{M}+\alpha\v{r}/r

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1/equations/15.2.tex Normal file
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U_\text{eff}=-\frac{\alpha}{r}+\frac{M^2}{2mr^2}

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1/equations/15.3.tex Normal file
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U_{\text{eff,min}}=-m\alpha^2/2M^2

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1/equations/15.4.tex Normal file
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p=M^2/m\alpha,\qquad e=\sqrt{1+(2EM^2/m\alpha^2)}

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1/equations/15.5.tex Normal file
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p/r=1+e\cos\phi

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1/equations/15.6.tex Normal file
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a=p/(1-e^2)=\alpha/2|E|,\qquad b=p/\sqrt{1-e^2}=M/\sqrt{2m|E|}

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1/equations/15.7.tex Normal file
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r_\min=p/(1+e)=a(1-e),\qquad r_\max=p/(1-e)=a(1+e)

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1/equations/15.8.tex Normal file
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\begin{align}
T&=2\pi a^{3/2}\sqrt{m/\alpha} \\
&=\pi\alpha\sqrt{m/2|E|^3}
\end{align}

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1/equations/15.9.tex Normal file
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r_\min=p/(e+1)=a(e-1)

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@ -23,12 +23,12 @@ III. INTEGRATION OF THE EQUATIONS OF MOTION
12. [Determination of the potential energy from the period of oscillation](12-determination-of-the-potential-energy-from-the-period-of-oscillation.html)
13. [The reduced mass](13-the-reduced-mass.html)
14. [Motion in a central field](14-motion-in-a-central-field.html)
15. [Kepler's problem](15-keplers-problem.html)
<span style="background-color: yellow; color: white: width: 100%;">
🚧 WORK IN PROGRESS BELOW THIS POINT 🚧
</span>
15. [Kepler's problem](15-keplers-problem.html)
IV. COLLISION BETWEEN PARTICLES
16. [Disintegration of particles](16-disintegration-of-particles.html)
17. [Elastic collisions](17-elastic-collisions.html)

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@ -14,6 +14,7 @@
\newcommand{\ptag}[2][]{\label{#1/#2}\tag*{(#2)}}
\newcommand{\min}{\text{min}}
\newcommand{\max}{\text{max}}
\newcommand{\constant}{\text{constant}}
\DeclareMathOperator{\ch}{ch}
\DeclareMathOperator{\sh}{sh}

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@ -40,7 +40,7 @@ def action(elem, doc):
return elem
else:
# section ref
_pnum = text
pnum = text
try:
slug = [f for f in os.listdir(book) if f.startswith(pnum)][0]
except: