pyslha 3.3.2

Parsing, manipulating, and visualising SUSY Les Houches Accord data

A simple but flexible handler of the SUSY Les Houches Accord (SLHA) data format.

pyslha is a parser/writer module for particle physics SUSY Les Houches Accord (SLHA) supersymmetric spectrum/decay files, and a collection of scripts which use the interface, e.g. for conversion to and from the legacy ISAWIG format, or to plot the mass spectrum and decay chains.

The current release supports SLHA version 1, and as far as I'm aware is also fully compatible with SLHA2: the block structures are read and accessed generically. If you have any problems, please provide an example input file and I'll happily investigate. SLHA3 is not yet supported (or standardised) but in recent releases the new structures will not crash the parser. Support will be added once the format is standardised (and in response to demand!)

The plotting script provides output in PDF, EPS and PNG via LaTeX and the TikZ graphics package, and as LaTeX/TikZ source for direct embedding into documents or user-tweaking of the generated output.

Users of version 2.x should note that the interface has changed a little in version 3.0.0 and onward: there are now generic read()/write() functions which can operate on filenames or file objects, and all I/O functions now return/accept a single Doc object rather than a tuple of blocks, decays, etc. dicts. This single-object interface to the SLHA document allows for more coherent handling of the data, as well as better robustness against future changes in the format and planned support for documentation comments.

API example

>>> import pyslha
>>> # generic read from file:
>>> d = pyslha.read('spcfiles/sps1a.spc')
>>> d
<PySLHA Doc: 22 blocks, 35 decays, 0 xsections>
>>> # or, to ignore blocks known to be e.g. badly formatted:
>>> d = pyslha.read('spcfiles/sps1a.spc', ignoreblocks=['DCINFO'])
>>> d
<PySLHA Doc: 21 blocks, 35 decays, 0 xsections>
>>> d.blocks
Blocks
  SPINFO { 1 : SOFTSUSY; 2 : 2.0.5 }
  MODSEL { 1,1 : sugra }
  SMINPUTS { 1 :  1.27934000e+02; 2 :  1.16637000e-05; ...
  ...
>>> d.blocks.has_key('MODSEL')
True
>>> d.blocks['MODSEL']
MODSEL { 1,1 : sugra }
>>> d.blocks['MODSEL'][1,1]
'sugra'
>>> d.blocks['MODSEL'][1,2] = 'foo'
>>> d.blocks['MODSEL']
MODSEL { 1,1 : sugra; 1,2 : foo }

The Block interface also supplies dict-like has_key(), keys(), and items() methods, as well as more specialist value(), set_value() and is_single_valued() methods for improved access to ALPHA and any other unindexed blocks.

The decay system has a similar interface to that of the generic Block for accessing particle decay-channel information:

>>> d.decays.keys()
[23, 24, 6, 25, 35, 36, 37, 1000021, 1000006, 2000006, 1000005, 2000005, ...
>>> d.decays[1000021]
1000021 : mass = 6.07713704e+02 GeV : total width = 5.50675438e+00 GeV
   1.05840237e-01 [1000005, -5]
   1.05840237e-01 [-1000005, 5]
   ...

The DECAY blocks in SLHA files are in fact mapped into Particle objects, each of which contains multiple Decay objects. Check the Python documentation for Doc, Block, Particle and Decay, plus the pyslha module free functions for I/O.

Citation

If you use PySLHA, for either model data handling or spectrum visualisation, please cite the paper: http://arxiv.org/abs/1305.4194