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add new notes and restructure
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@ -79,6 +79,9 @@ Viele Gruesse, Frank
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- [[file:prog/python/qqgg/analytical_xs.ipynb][Notebook mit Implementierung der XS]]
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- [[file:prog/python/qqgg/analytical_xs.ipynb][Notebook mit Implementierung der XS]]
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- Zeigte fehler in Rechnung auf
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- Zeigte fehler in Rechnung auf
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** Monte Carlo Methods
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- [[file:prog/python/qqgg/analytical_xs.org::*Numerical Integration][Integration]]
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- [[file:prog/python/qqgg/analytical_xs.org::*Sampling and Analysis][Sampling and Analysis]]
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* Clock Table
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* Clock Table
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#+BEGIN: clocktable :scope file :maxlevel 2
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#+BEGIN: clocktable :scope file :maxlevel 2
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#+CAPTION: Clock summary at [2020-03-18 Wed 21:01]
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#+CAPTION: Clock summary at [2020-03-18 Wed 21:01]
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<h2>Table of Contents</h2>
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<div id="text-table-of-contents">
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<ul>
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<li><a href="#org255850a">1. Init</a>
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<ul>
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<li><a href="#org2f3a4e9">1.1. Required Modules</a></li>
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<li><a href="#org2e97ca2">1.2. Utilities</a></li>
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<li><a href="#org468bdb4">2. Implementation</a></li>
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<li><a href="#org9989482">3. Calculations</a>
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<li><a href="#org9716522">3.1. XS qq -> gamma gamma</a></li>
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<h2 id="org255850a"><span class="section-number-2">1</span> Init</h2>
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<h3 id="org2f3a4e9"><span class="section-number-3">1.1</span> Required Modules</h3>
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<div class="org-src-container">
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<pre class="src src-ipython" id="org91f75e0"><span style="color: #859900; font-weight: bold;">import</span> numpy <span style="color: #859900; font-weight: bold;">as</span> np
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<h3 id="org2e97ca2"><span class="section-number-3">1.2</span> Utilities</h3>
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<pre class="src src-ipython" id="org41306d9">%run ../utility.py
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<h2 id="org468bdb4"><span class="section-number-2">2</span> Implementation</h2>
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<pre class="src src-ipython" id="org30462c1"><span style="color: #35a69c; font-style: italic;">"""</span>
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<span style="color: #35a69c; font-style: italic;">Implementation of the analytical cross section for q q_bar -></span>
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<span style="color: #35a69c; font-style: italic;">gamma gamma</span>
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<span style="color: #35a69c; font-style: italic;">Author: Valentin Boettcher <a href="mailto:hiro%40protagon.space"><hiro@protagon.space></a></span>
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<span style="color: #35a69c; font-style: italic;">"""</span>
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<span style="color: #859900; font-weight: bold;">import</span> numpy <span style="color: #859900; font-weight: bold;">as</span> np
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<span style="color: #859900; font-weight: bold;">from</span> scipy.constants <span style="color: #859900; font-weight: bold;">import</span> alpha
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<span style="color: #96A7A9; font-style: italic;"># </span><span style="color: #96A7A9; font-style: italic;">NOTE: a more elegant solution would be a decorator</span>
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<span style="color: #859900; font-weight: bold;">def</span> <span style="color: #b58900;">energy_factor</span>(charge, esp):
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<span style="color: #35a69c; font-style: italic;">"""</span>
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<span style="color: #35a69c; font-style: italic;"> Calculates the factor common to all other values in this module</span>
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|
||||||
<span style="color: #35a69c; font-style: italic;"> Arguments:</span>
|
|
||||||
<span style="color: #35a69c; font-style: italic;"> esp -- center of momentum energy in GeV</span>
|
|
||||||
<span style="color: #35a69c; font-style: italic;"> charge -- charge of the particle in units of the elementary charge</span>
|
|
||||||
<span style="color: #35a69c; font-style: italic;"> """</span>
|
|
||||||
|
|
||||||
<span style="color: #859900; font-weight: bold;">return</span> charge**4*(alpha/esp)**2/6
|
|
||||||
|
|
||||||
|
|
||||||
<span style="color: #859900; font-weight: bold;">def</span> <span style="color: #b58900;">diff_xs</span>(theta, charge, esp):
|
|
||||||
<span style="color: #35a69c; font-style: italic;">"""</span>
|
|
||||||
<span style="color: #35a69c; font-style: italic;"> Calculates the differential cross section as a function of the</span>
|
|
||||||
<span style="color: #35a69c; font-style: italic;"> azimuth angle theta in units of 1/GeV^2.</span>
|
|
||||||
|
|
||||||
<span style="color: #35a69c; font-style: italic;"> Arguments:</span>
|
|
||||||
<span style="color: #35a69c; font-style: italic;"> theta -- azimuth angle</span>
|
|
||||||
<span style="color: #35a69c; font-style: italic;"> esp -- center of momentum energy in GeV</span>
|
|
||||||
<span style="color: #35a69c; font-style: italic;"> charge -- charge of the particle in units of the elementary charge</span>
|
|
||||||
<span style="color: #35a69c; font-style: italic;"> """</span>
|
|
||||||
|
|
||||||
<span style="color: #268bd2;">f</span> = energy_factor(charge, esp)
|
|
||||||
<span style="color: #859900; font-weight: bold;">return</span> f*((np.cos(theta)**+1)/np.sin(theta)**2)
|
|
||||||
|
|
||||||
<span style="color: #859900; font-weight: bold;">def</span> <span style="color: #b58900;">diff_xs_eta</span>(eta, charge, esp):
|
|
||||||
<span style="color: #35a69c; font-style: italic;">"""</span>
|
|
||||||
<span style="color: #35a69c; font-style: italic;"> Calculates the differential cross section as a function of the</span>
|
|
||||||
<span style="color: #35a69c; font-style: italic;"> pseudo rapidity of the photons in units of 1/GeV^2.</span>
|
|
||||||
|
|
||||||
<span style="color: #35a69c; font-style: italic;"> Arguments:</span>
|
|
||||||
<span style="color: #35a69c; font-style: italic;"> eta -- pseudo rapidity</span>
|
|
||||||
<span style="color: #35a69c; font-style: italic;"> esp -- center of momentum energy in GeV</span>
|
|
||||||
<span style="color: #35a69c; font-style: italic;"> charge -- charge of the particle in units of the elementary charge</span>
|
|
||||||
<span style="color: #35a69c; font-style: italic;"> """</span>
|
|
||||||
|
|
||||||
<span style="color: #268bd2;">f</span> = energy_factor(charge, esp)
|
|
||||||
<span style="color: #859900; font-weight: bold;">return</span> f*(2*np.cosh(eta)**2 - 1)
|
|
||||||
|
|
||||||
<span style="color: #859900; font-weight: bold;">def</span> <span style="color: #b58900;">total_xs_eta</span>(eta, charge, esp):
|
|
||||||
<span style="color: #35a69c; font-style: italic;">"""</span>
|
|
||||||
<span style="color: #35a69c; font-style: italic;"> Calculates the total cross section as a function of the pseudo</span>
|
|
||||||
<span style="color: #35a69c; font-style: italic;"> rapidity of the photons in units of 1/GeV^2. If the rapditiy is</span>
|
|
||||||
<span style="color: #35a69c; font-style: italic;"> specified as a tuple, it is interpreted as an interval. Otherwise</span>
|
|
||||||
<span style="color: #35a69c; font-style: italic;"> the interval [-eta, eta] will be used.</span>
|
|
||||||
|
|
||||||
<span style="color: #35a69c; font-style: italic;"> Arguments:</span>
|
|
||||||
<span style="color: #35a69c; font-style: italic;"> eta -- pseudo rapidity (tuple or number)</span>
|
|
||||||
<span style="color: #35a69c; font-style: italic;"> esp -- center of momentum energy in GeV</span>
|
|
||||||
<span style="color: #35a69c; font-style: italic;"> charge -- charge of the particle in units of the elementar charge</span>
|
|
||||||
<span style="color: #35a69c; font-style: italic;"> """</span>
|
|
||||||
|
|
||||||
<span style="color: #268bd2;">f</span> = energy_factor(charge, esp)
|
|
||||||
<span style="color: #859900; font-weight: bold;">if</span> <span style="color: #859900; font-weight: bold;">not</span> <span style="color: #d33682; font-style: italic;">isinstance</span>(eta, <span style="color: #d33682; font-style: italic;">tuple</span>):
|
|
||||||
<span style="color: #268bd2;">eta</span> = (-eta, eta)
|
|
||||||
|
|
||||||
<span style="color: #859900; font-weight: bold;">if</span> <span style="color: #d33682; font-style: italic;">len</span>(eta) != 2:
|
|
||||||
<span style="color: #859900; font-weight: bold;">raise</span> <span style="color: #b58900; font-style: italic;">ValueError</span>(<span style="color: #2aa198;">'Invalid eta cut.'</span>)
|
|
||||||
|
|
||||||
<span style="color: #859900; font-weight: bold;">def</span> <span style="color: #b58900;">F</span>(x):
|
|
||||||
<span style="color: #859900; font-weight: bold;">return</span> np.tanh(x) - 2*x
|
|
||||||
|
|
||||||
<span style="color: #859900; font-weight: bold;">return</span> 2*np.pi*f*(F(eta[0]) - F(eta[1]))
|
|
||||||
</pre>
|
|
||||||
</div>
|
|
||||||
</div>
|
|
||||||
</div>
|
|
||||||
|
|
||||||
<div id="outline-container-org9989482" class="outline-2">
|
|
||||||
<h2 id="org9989482"><span class="section-number-2">3</span> Calculations</h2>
|
|
||||||
<div class="outline-text-2" id="text-3">
|
|
||||||
</div>
|
|
||||||
<div id="outline-container-org9716522" class="outline-3">
|
|
||||||
<h3 id="org9716522"><span class="section-number-3">3.1</span> XS qq -> gamma gamma</h3>
|
|
||||||
<div class="outline-text-3" id="text-3-1">
|
|
||||||
<p>
|
|
||||||
First, set up the input parameters.
|
|
||||||
</p>
|
|
||||||
<div class="org-src-container">
|
|
||||||
<pre class="src src-ipython" id="org9135f0f"><span style="color: #268bd2;">eta</span> = 2.5
|
|
||||||
<span style="color: #268bd2;">charge</span> = 1/3
|
|
||||||
<span style="color: #268bd2;">esp</span> = 200 <span style="color: #96A7A9; font-style: italic;"># </span><span style="color: #96A7A9; font-style: italic;">GeV</span>
|
|
||||||
</pre>
|
|
||||||
</div>
|
|
||||||
|
|
||||||
<p>
|
|
||||||
And now calculate the cross section in picobarn.
|
|
||||||
</p>
|
|
||||||
<div class="org-src-container">
|
|
||||||
<pre class="src src-ipython" id="org1b205cb"><span style="color: #268bd2;">xs_gev</span> = total_xs_eta(eta, charge, esp)
|
|
||||||
<span style="color: #268bd2;">xs_pb</span> = gev_to_pb(xs_gev)
|
|
||||||
<span style="color: #859900; font-weight: bold;">print</span>(tex_value(xs_pb, unit=r<span style="color: #2aa198;">'\pico\barn'</span>, prefix=r<span style="color: #2aa198;">'\eta = '</span>))
|
|
||||||
</pre>
|
|
||||||
</div>
|
|
||||||
|
|
||||||
<p>
|
|
||||||
<a href="../../../results/xs/xs.tex">../../../results/xs/xs.tex</a>
|
|
||||||
</p>
|
|
||||||
|
|
||||||
<p>
|
|
||||||
Compared to sherpa, it's pretty close.
|
|
||||||
</p>
|
|
||||||
<div class="org-src-container">
|
|
||||||
<pre class="src src-ipython" id="org2bcb666"><span style="color: #268bd2;">sherpa</span> = 0.0538009
|
|
||||||
xs_pb/sherpa
|
|
||||||
</pre>
|
|
||||||
</div>
|
|
||||||
|
|
||||||
<p>
|
|
||||||
0.9998585425137037
|
|
||||||
</p>
|
|
||||||
|
|
||||||
|
|
||||||
|
|
||||||
<p>
|
|
||||||
I had to set the runcard option <code>EW_SCHEME: alpha0</code> to use the pure
|
|
||||||
QED coupling constant.
|
|
||||||
</p>
|
|
||||||
</div>
|
|
||||||
</div>
|
|
||||||
</div>
|
|
||||||
</div>
|
|
||||||
<div id="postamble" class="status">
|
|
||||||
<p class="date">Created: 2020-03-28 Sat 11:30</p>
|
|
||||||
<p class="validation"><a href="http://validator.w3.org/check?uri=referer">Validate</a></p>
|
|
||||||
</div>
|
|
||||||
</body>
|
|
||||||
</html>
|
|
||||||
|
|
@ -142,11 +142,19 @@ charge = 1/3
|
||||||
esp = 200 # GeV
|
esp = 200 # GeV
|
||||||
#+END_SRC
|
#+END_SRC
|
||||||
|
|
||||||
|
Set up the integration and plot intervals.
|
||||||
|
#+begin_src ipython :session :exports both :results raw drawer
|
||||||
|
interval_η = [-η, η]
|
||||||
|
interval = η_to_θ([-η, η])
|
||||||
|
interval_cosθ = np.cos(interval)
|
||||||
|
interval_pt = η_to_pt([0, η], esp/2)
|
||||||
|
plot_interval = [0.1, np.pi-.1]
|
||||||
|
#+end_src
|
||||||
|
|
||||||
#+RESULTS: 7e62918a-2935-41ac-94e0-f0e7c3af8e0d
|
#+RESULTS: 7e62918a-2935-41ac-94e0-f0e7c3af8e0d
|
||||||
:RESULTS:
|
:RESULTS:
|
||||||
:END:
|
:END:
|
||||||
|
|
||||||
|
|
||||||
*** Analytical Integratin
|
*** Analytical Integratin
|
||||||
And now calculate the cross section in picobarn.
|
And now calculate the cross section in picobarn.
|
||||||
#+NAME: cf853fb6-d338-482e-bc55-bd9f8e796495
|
#+NAME: cf853fb6-d338-482e-bc55-bd9f8e796495
|
||||||
|
|
@ -175,19 +183,7 @@ Compared to sherpa, it's pretty close.
|
||||||
|
|
||||||
I had to set the runcard option ~EW_SCHEME: alpha0~ to use the pure
|
I had to set the runcard option ~EW_SCHEME: alpha0~ to use the pure
|
||||||
QED coupling constant.
|
QED coupling constant.
|
||||||
*** Numerical Integration and Sampling
|
*** Numerical Integration
|
||||||
Set up the integration and plot intervals.
|
|
||||||
#+begin_src ipython :session :exports both :results raw drawer
|
|
||||||
interval_η = [-η, η]
|
|
||||||
interval = η_to_θ([-η, η])
|
|
||||||
interval_cosθ = np.cos(interval)
|
|
||||||
interval_pt = η_to_pt([0, η], esp/2)
|
|
||||||
plot_interval = [0.1, np.pi-.1]
|
|
||||||
#+end_src
|
|
||||||
|
|
||||||
#+RESULTS:
|
|
||||||
:RESULTS:
|
|
||||||
:END:
|
|
||||||
|
|
||||||
Plot our nice distribution:
|
Plot our nice distribution:
|
||||||
#+begin_src ipython :session :exports both :results raw drawer
|
#+begin_src ipython :session :exports both :results raw drawer
|
||||||
|
|
@ -257,6 +253,7 @@ print(tex_value(xs_pb_mc, unit=r'\pico\barn', prefix=r'\sigma = ', prec=5))
|
||||||
[[file:results/xs_mc.tex]]
|
[[file:results/xs_mc.tex]]
|
||||||
:END:
|
:END:
|
||||||
|
|
||||||
|
*** Sampling and Analysis
|
||||||
Now we monte-carlo sample our distribution.
|
Now we monte-carlo sample our distribution.
|
||||||
#+begin_src ipython :session :exports both :results raw drawer
|
#+begin_src ipython :session :exports both :results raw drawer
|
||||||
cosθ_sample = sample(lambda x: diff_xs_cosθ(x, charge, esp), interval_cosθ)
|
cosθ_sample = sample(lambda x: diff_xs_cosθ(x, charge, esp), interval_cosθ)
|
||||||
|
|
|
||||||
Loading…
Add table
Reference in a new issue