@@ -35,20 +35,34 @@ <h1><a href="index.html"> The <strong>EXP</strong> Collaboration </a></h1>
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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 >
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