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GAMBIT  v1.5.0-2191-ga4742ac
a Global And Modular Bsm Inference Tool
spectrum.cpp File Reference

This class is used to deliver both information defined in the Standard Model (or potentially just QED X QCD) as a low-energy effective theory (as opposed to correspending information defined in a high-energy model) as well as a corresponding high energy theory. More...

Include dependency graph for spectrum.cpp:

Go to the source code of this file.

Namespaces

 Gambit
 TODO: see if we can use this one:
 

Functions

bool Gambit::is_abs (str &s)
 Helper function for checking if a particle or ratio has been requested as an absolute value. More...
 
void Gambit::swap (Spectrum &first, Spectrum &second)
 Swap resources of two Spectrum objects Note: Not a member function! This is an external function which is a friend of the Spectrum class. More...
 

Detailed Description

This class is used to deliver both information defined in the Standard Model (or potentially just QED X QCD) as a low-energy effective theory (as opposed to correspending information defined in a high-energy model) as well as a corresponding high energy theory.

Parameters defined in the low-energy model are often used as input to a physics calculators. In addition, parameters used to define the Standard Model, in SLHA2 format, are provided in the SMINPUTS data member.

Access to the pole masses of either SubSpectrum is provided by the "get_Pole_Mass" function, which will search both subspectra for a match. For running parameters, one should access them via the getters of "LE" or "HE" subspectra.


Authors:

Author
Ben Farmer (benja.nosp@m.min..nosp@m.farme.nosp@m.r@fy.nosp@m.sik.s.nosp@m.u.se)
Date
2015 Mar
Author
Pat Scott (p.sco.nosp@m.tt@i.nosp@m.mperi.nosp@m.al.a.nosp@m.c.uk)
Date
2015 May, 2016 Nov
Author
Abram Krislock (a.m.b.nosp@m..kri.nosp@m.slock.nosp@m.@fys.nosp@m..uio..nosp@m.no)
Date
2016 Feb

Definition in file spectrum.cpp.