Open Access

Table 1

Symbols and abbreviations used repeatedly.

Abbreviation Description Example unit

Physical parameters in the gas parcel

t Simulation integration time yr, s
Tgas Gas temperature K
NH Hydrogen atom column density cm−2
NH Hydrogen atom number density cm−3
n(H2) Hydrogen molecule number density cm−3
ζ Cosmic-ray ionisation rate s−1

Granular parameters

ng Number density of interstellar grains cm−3
Td Dust grain temperature K
a Dust grain radius μm
b Ice mantle thickness on grains μm, MLs
X:H2O Icy species’ X abundance relative to that of water ice %
ML Monolayer –ice layer with the thickness of a single molecule

Desorption energy parameters

ED Surface molecule desorption (binding) energy K
Ediff Surface molecule diffusion energy; 0.5ED K
ED,pol Default base ED value, on H2O ice surface K
ED,np ED on hyper-volatile (CO) ice surface K
ED,bare ED for molecules on completely bare grains K
ED,np/ED,pol Factor for ED,pol change in CO ices
ED,pol-ED,bare Energy value of a H-bond. K
EA Reaction activation energy K
Xdes Fitting parameter for ED on mixed ice, Eq. (3)
H-bond rule Bare grain surface does not form hydrogen bonds.
Hyper-volatiles Icy species with ED lower than ≈1300 K

Efficiency parameters for desorption mechanisms

fCRD Frequency of cosmic-ray induced heating of whole grains s−1
Ypd UV photodesorption yield. molecule photon−1
fCD Probability for surface reaction product desorption

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