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| author | glisse <glisse@636b058d-ea47-450e-bf9e-a15bfbe3eedb> | 2018-10-10 21:43:35 +0000 |
|---|---|---|
| committer | glisse <glisse@636b058d-ea47-450e-bf9e-a15bfbe3eedb> | 2018-10-10 21:43:35 +0000 |
| commit | d16910a5c74552b3b1feffc3e793ec5b6d52f952 (patch) | |
| tree | 0b6eebf85330035e32b2151885a8eead4030e3e7 /src/cython | |
| parent | c537a466ffdd812d92098bcea04cdf6f0bfc64ec (diff) | |
Use math instead of unicode for epsilon
git-svn-id: svn+ssh://scm.gforge.inria.fr/svnroot/gudhi/branches/sparserips-python@3938 636b058d-ea47-450e-bf9e-a15bfbe3eedb
Former-commit-id: 8cccce774b7406d90a55d0e2827fad6dc3855b39
Diffstat (limited to 'src/cython')
| -rw-r--r-- | src/cython/doc/rips_complex_user.rst | 2 |
1 files changed, 1 insertions, 1 deletions
diff --git a/src/cython/doc/rips_complex_user.rst b/src/cython/doc/rips_complex_user.rst index 95bb40b6..cddf4f16 100644 --- a/src/cython/doc/rips_complex_user.rst +++ b/src/cython/doc/rips_complex_user.rst @@ -45,7 +45,7 @@ A more general technique is to use a sparse approximation of the Rips introduced by Don Sheehy :cite:`sheehy13linear`. We are using the version described in :cite:`buchet16efficient` (except that we multiply all filtration values by 2, to match the usual Rips complex), which proves a -:math:`\frac{1+\epsilon}{1-\epsilon}`-interleaving, although in practice the +:math:`\frac{1+\varepsilon}{1-\varepsilon}`-interleaving, although in practice the error is usually smaller. A more intuitive presentation of the idea is available in :cite:`cavanna15geometric`, and in a video :cite:`cavanna15visualizing`. Passing an extra argument `sparse=0.3` at the |