Published August 9, 2024 | Version 1.1.1

The NANOGrav 15-year Search for New Physics Signals - model files

Authors/Creators

Description

 

PTArcade model files used in the paper "The NANOGrav 15 yr Data Set: Search for Signals from New Physics".

The tabulated data used to define some of the signals is provided in the 'models_data' folder.

Refer to the PTArcade documentation page for details on how PTArcade model files are defined and used.

The naming convention for the files is the following:

  • igw: inflationary Gravitational Waves (GWs)
  • sigw: scalar-induced GWs
    • sigw_box: assumes a box-like feature in the primordial power spectrum.
    • sigw_delta: assumes a delta-like feature in the primordial power spectrum.
    • sigw_gauss: assumes a gaussian peak feature in the primordial power spectrum.
  • pt: cosmological phase transitions
    • pt_bubble: assumes that the dominant contribution to the GW productions comes from bubble collisions.
    • pt_sound: assumes that the dominant contribution to the GW productions comes from sound waves.
  • stable: stable cosmic strings
    • stable-c: stable strings emitting GWs only in the form of GW bursts from cusps on closed loops.
    • stable-k: stable strings emitting GWs only in the form of GW bursts from kinks on closed loops.
    • stable-m: stable strings emitting monochromatic GW at the fundamental frequency.
    • stable-n: stable strings described by numerical simulations including GWs from cusps and kinks.
  • meta: metastable cosmic strings
    • meta-l: metastable strings with GW emission from loops only.
    • meta-ls metastable strings with GW emission from loops and segments.
  • super: cosmic superstrings.
  • dw: domain walls
    • dw-sm: domain walls decaying into Standard Model particles.
    • dw-dr: domain walls decaying into dark radiation.
  • uldm_e: ULDM Earth signal.
  • uldm_c: ULDM combined Earth + pulsar signal for direct coupling
    • uldm_c_cor: correlated limit
    • uldm_c_unc: uncorrelated limit
  • uldm_vecB: vector ULDM coupled to the baryon number
    • uldm_vecB_cor: correlated limit
    • uldm_vecB_unc: uncorrelated limit
  • uldm_vecBL: vector ULDM coupled to B-L
    • uldm_vecBL_cor: correlated limit
    • uldm_vecBL_unc: uncorrelated limit
  • uldm_p: ULDM pulsar signal
    • uldm_p_cor: ULDM pulsar signal in the correlated limit.
    • uldm_p_unc: ULDM pulsar signal in the uncorrelated limit.
  • uldm_c_grav: ULDM combined Earth + pulsar signal for gravitational only coupling
    • uldm_c_grav_cor: correlated limit
      • uldm_c_cor_grav_low: low mass region  
      • uldm_c_cor_grav_mon: monopole region
      • uldm_c_cor_grav_high: high mass region
    • uldm_c_unc: uncorrelated limit
      • uldm_c_unc_grav_low: low mass region  
      • uldm_c_unc_grav_mon: monopole region
      • uldm_c_unc_grav_high: high mass region
  • pbh_dynamic: substructure signal in the dynamic limit.
  • pbh_static: substructure signal in the static limit.

Notes

Fixed typo in the normalization of the phase transition spectra.

Files

models_1.1.1.zip

Files (7.7 MB)

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Additional details

Related works

Is supplement to
Journal article: 10.3847/2041-8213/acdc91 (DOI)
Journal article: 10.3847/2041-8213/ad68fc (DOI)