Skip to content

Commit 03167d2

Browse files
committed
edits
1 parent e4fc8e5 commit 03167d2

File tree

2 files changed

+29
-15
lines changed

2 files changed

+29
-15
lines changed

assets/css/main.css

Lines changed: 1 addition & 1 deletion
Original file line numberDiff line numberDiff line change
@@ -1488,7 +1488,7 @@ input, select, textarea {
14881488

14891489
#header h1 a {
14901490
border: 0;
1491-
color: inherit;
1491+
color: #030304;
14921492
}
14931493

14941494
#header h1 a:hover {

index.html

Lines changed: 28 additions & 14 deletions
Original file line numberDiff line numberDiff line change
@@ -35,20 +35,34 @@ <h1><a href="index.html"> The <strong>EXP</strong> Collaboration </a></h1>
3535
<article class="thumb">
3636
<a href="images/fulls/plain.png" class="image"><img src="images/thumbs/1.png" alt="" /></a>
3737
<h2> What is a basis function expansion? </h2>
38-
<p> A basis function expansion (BFE) uses relatively simple equations to represent a more complex
39-
distribution. Each term in the expansion is given a weight such that the sum of the functions
40-
optimally represents the given distribution. In our case, we use BFEs to represent the
41-
gravitational potential and mass distribution of the dark matter (and/or baryons) in a galaxy.
42-
We tailor the expansion such that the zeroth order term represents the equilibrium state of the galaxy.
43-
The BFE framework is a powerful tool for analyses of galactic dynamics and disequilibrium dynamics, in
44-
particular. The EXP collaboration is built around the shared vision of developing these tools for galactic
45-
dynamics, combining the varied expertise of its members to learn about disequilibrium dynamics in galaxies.
46-
The publicly-available <a href="https://github.com/EXP-code">EXP code</a> was developed to help achieve
47-
this task. As evidenced in the following pages, there are a number of use cases for BFE analysis framework,
48-
and members of our collaboration have used BFEs to provide profound insight into a variety of problems. </p>
49-
<p> Interested in learning more? Check out the other tabs of this website,
50-
the <a href="https://github.com/EXP-code">Github</a>, and the theory page of the
51-
<a href="https://exp-docs.readthedocs.io/en/latest/index.html">readthedocs</a></p>
38+
<p> In the Milky Way, the density, potential, velocity, energy, angular momentum and chemical abundance
39+
patterns fluctuate across the disk. More generally, fields in galaxies – and other physical systems –
40+
often vary in complex manners that cannot be captured with simple, analytic formulae. In simulations,
41+
these fluctuations are described in simulations by particles representing random draws from the full
42+
field. In the Milky Way, the fluctuations are captured in the spatial density of stars. In
43+
observations of other galaxies, the fluctuations are reflected in the properties of light captured in
44+
a pixel. A full description often requires millions or even hundreds of millions of numbers. </p>
45+
<p> A well-designed Basis Function Expansion can typically capture the salient features of a complex
46+
field in 1000’s of numbers, providing a succinct description. It does so by representing the full
47+
field in a series of basis functions that span function space. The information in the field is
48+
captured in the coefficients of each basis function in the expansion. For large enough numbers of
49+
basis functions, any field can be represented. However, BFE’s become truly powerful if they can be
50+
tailored to the application, so the information can be captured in as few terms as possible. </p>
51+
<p> The best-known examples of a BFE are Fourier series of sines and cosines, which are very good at
52+
capturing variations in time or space that repeat with a small set of regular periods. In a galactic
53+
dynamics context, the optimal basis will resemble the galaxy, with additional functions to capture
54+
variance or deviations from the simplest axisymmetric model. In N-body simulations of galaxies, BFEs
55+
have been used to derive potential fields at each timestep from particle data at computational effort
56+
proportional to the number of particles – drastically less computationally intense than other
57+
techniques to determine potentials
58+
<a href="https://ui.adsabs.harvard.edu/abs/1992ApJ...386..375H/abstract">Hernquist (1992)</a>. </p>
59+
<p> More generally: in theoretical analyses, BFE have been partnered with mathematical tools of
60+
perturbation theory and linear algebra to solve equations, to describe interactions and identify
61+
physical mechanisms such as in the interaction of the Milky Way and Large Magellanic Cloud
62+
(<a href="https://ui.adsabs.harvard.edu/abs/2006ApJ...641L..33W/abstract">Weinberg & Blitz 2006</a>).
63+
Additionally, BFE have been used in observations to compress vast data sets and allow interpretation,
64+
such as in the power spectrum of fluctuations in the temperature of the Cosmic Microwave Background
65+
(<a href=”https://ui.adsabs.harvard.edu/abs/2007ApJS..170..377S/abstract”>Spergel et al. 2007</a>). </p>
5266
</article>
5367
<article class="thumb">
5468
<a href="images/fulls/plain.png" class="image"><img src="images/thumbs/2.png" alt="" /></a>

0 commit comments

Comments
 (0)