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GAMBIT  v1.5.0-2191-ga4742ac
a Global And Modular Bsm Inference Tool
spectrum.hpp 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...

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Classes

struct  YAML::convert< sdd >
 
struct  YAML::convert< ssdd >
 
class  Gambit::Spectrum
 "Standard Model" (low-energy) plus high-energy model container class More...
 

Namespaces

 YAML
 YAML overloads for mass cut and mass cut ratio constituents.
 
 Gambit
 TODO: see if we can use this one:
 

Typedefs

typedef std::pair< std::string, std::pair< double, double > > YAML::sdd
 
typedef std::pair< std::pair< std::string, std::string >, std::pair< double, double > > YAML::ssdd
 

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
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.hpp.