better compatibility through greater accuracy

This commit is contained in:
hiro98 2020-06-04 21:39:44 +02:00
parent c6fc696128
commit 55e4ca50c3
33 changed files with 13737 additions and 13742 deletions

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@ -489,14 +489,14 @@ draw_histogram(ax, part_hist)
Now, it would be interesting to know the total cross section.
So let's define the increments for VEGAS.
#+begin_src jupyter-python :exports both :results raw drawer
increments = np.array([3, 100, 100])
increments = np.array([4, 100, 100])
tex_value(
np.prod(increments), prefix=r"K=", prec=0, save=("results/pdf/", "num_increments.tex")
)
#+end_src
#+RESULTS:
: \(K=30000\)
: \(K=40000\)
And calculate the XS.
#+begin_src jupyter-python :exports both :results raw drawer
@ -511,14 +511,14 @@ And calculate the XS.
xs_int_res = monte_carlo.integrate_vegas_nd(
dist_η_vec,
[interval_η, [pdf.xMin, 1], [pdf.xMin, 1]],
epsilon=1e-11,
[interval_η, [pdf.xMin, pdf.xMax], [pdf.xMin, pdf.xMax]],
epsilon=1e-11/2,
proc=1,
increment_epsilon=.02,
alpha=1.8,
num_increments=increments,
num_points_per_cube=10,
cache="cache/pdf/total_xs_2_5_20_take20",
cache="cache/pdf/total_xs_2_5_20_take22",
)
total_xs = gev_to_pb(np.array(xs_int_res.combined_result)) * 2 * np.pi
@ -528,7 +528,7 @@ And calculate the XS.
#+RESULTS:
:RESULTS:
: Loading Cache: integrate_vegas_nd
: array([3.86911687e+01, 1.96651183e-02])
: array([3.86891167e+01, 9.39243388e-03])
:END:
#+begin_src jupyter-python :exports both :results raw drawer
@ -547,7 +547,7 @@ there are two identical protons.
#+end_src
#+RESULTS:
: -0.0012964079498659457
: 0.006924228292849407
The efficiency will be around:
#+begin_src jupyter-python :exports both :results raw drawer
@ -555,7 +555,7 @@ The efficiency will be around:
#+end_src
#+RESULTS:
: 32.89204347314658
: 36.68699853098365
Let's export those results for TeX:
#+begin_src jupyter-python :exports both :results raw drawer
@ -691,7 +691,7 @@ Lets plot how the pdf looks.
Overestimating the upper bounds helps with bias.
#+begin_src jupyter-python :exports both :results raw drawer
overestimate = 1.1
overestimate = 1.0
tex_value(
(overestimate - 1) * 100,
unit=r"\percent",
@ -702,7 +702,7 @@ Overestimating the upper bounds helps with bias.
#+RESULTS:
:RESULTS:
: \(\SI{10}{\percent}\)
: \(\SI{0}{\percent}\)
[[file:./.ob-jupyter/542b03d025920448ba653b470ec6492cbdd1e4a7.png]]
[[file:./.ob-jupyter/d47db0dde9ae59979f271a7cba8dfc46be3f1dd3.png]]
[[file:./.ob-jupyter/7fe9d3bd60427cf20af835649efbcbaafefbb3e0.png]]
@ -718,7 +718,7 @@ figure out the cpu mapping.
cubes=xs_int_res.cubes,
proc="auto",
report_efficiency=True,
cache="cache/pdf/total_xs_10000_000_2_5_take8",
cache="cache/pdf/total_xs_10000_000_2_5_take11",
status_path="/tmp/status1",
overestimate_factor=overestimate,
)
@ -728,7 +728,7 @@ figure out the cpu mapping.
#+RESULTS:
:RESULTS:
: Loading Cache: sample_unweighted_array
: 0.29610040880251154
: 0.3615754237122427
:END:
That does look pretty good eh? So lets save it along with the sample size.
@ -744,7 +744,7 @@ That does look pretty good eh? So lets save it along with the sample size.
#+end_src
#+RESULTS:
: \(\mathfrak{e}=\SI{30}{\percent}\)
: \(\mathfrak{e}=\SI{36}{\percent}\)
** Observables
Let's look at a histogramm of eta samples.
@ -757,7 +757,7 @@ Let's look at a histogramm of eta samples.
#+RESULTS:
:RESULTS:
: 10000000
[[file:./.ob-jupyter/0b1b4f39201dac86ebfbfb8953561cfe81a6c70f.png]]
[[file:./.ob-jupyter/764bd95aedbef68e7709a84780df593399e347a4.png]]
:END:
Let's use a uniform histogram image size.
@ -786,7 +786,7 @@ And now we compare all the observables with sherpa.
#+end_src
#+RESULTS:
[[file:./.ob-jupyter/a32ee488f4357426e3acecb1a5baaeddc367ee9b.png]]
[[file:./.ob-jupyter/800bffd38987eae852b74eb2483698169c08c4de.png]]
Hah! there we have it!
@ -817,11 +817,10 @@ both equal.
#+end_src
#+RESULTS:
[[file:./.ob-jupyter/deeb122e09b948ea416db671bfe1838aedeae84a.png]]
[[file:./.ob-jupyter/45cc8fbfa523c8faf704505d716ebc299a1a44fd.png]]
The invariant mass is not constant anymore.
#+begin_src jupyter-python :exports both :results raw drawer
bins = np.logspace(*np.log10([2 * min_pT, 2 * e_proton]), 51)
yoda_hist_inv_m = yoda_to_numpy(yoda_file["/MC_DIPHOTON_PROTON/inv_m"])
fig, (ax, ax_ratio) = draw_ratio_plot(
@ -842,7 +841,7 @@ The invariant mass is not constant anymore.
#+end_src
#+RESULTS:
[[file:./.ob-jupyter/a7708226adeb9782b68ffb10003c280d8dd19ef2.png]]
[[file:./.ob-jupyter/9ad48ff715bb6445bf5a0c515e4a4f41593146fe.png]]
The cosθ distribution looks more like the paronic one.
#+begin_src jupyter-python :exports both :results raw drawer
@ -861,7 +860,7 @@ The cosθ distribution looks more like the paronic one.
#+end_src
#+RESULTS:
[[file:./.ob-jupyter/5bf3849e8196878ba4585a09e496e852b9969866.png]]
[[file:./.ob-jupyter/d834978baba81dba0e2f052f1965b62ae736c151.png]]
#+begin_src jupyter-python :exports both :results raw drawer
@ -883,7 +882,7 @@ The cosθ distribution looks more like the paronic one.
#+end_src
#+RESULTS:
[[file:./.ob-jupyter/cd50dc4eb341d959871bf4288ff3620556a53970.png]]
[[file:./.ob-jupyter/22100d74fc1e07aa9ac75e22dd38ce49eaad89d4.png]]
In this case the opening angles are the same because the CS frame is
the same as the ordinary rest frame. The z-axis is the beam axis
@ -907,4 +906,4 @@ because pT=0!
#+end_src
#+RESULTS:
[[file:./.ob-jupyter/9ae6d76460a0d99d6e64cd85c8d0b712984b93d6.png]]
[[file:./.ob-jupyter/28abf9fcf1840bc31a5819d380a8eff0c2ef3e43.png]]

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@ -1 +1 @@
\(\sigma = \SI{38.691\pm 0.020}{\pico\barn}\)
\(\sigma = \SI{38.689\pm 0.009}{\pico\barn}\)

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@ -1 +1 @@
\(K=30000\)
\(K=40000\)

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@ -1 +1 @@
\(\SI{10}{\percent}\)
\(\SI{0}{\percent}\)

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@ -1 +1 @@
\(\mathfrak{e}=\SI{30}{\percent}\)
\(\mathfrak{e}=\SI{36}{\percent}\)