Table 1.

Relevant parameters of the ETHOS (Effective Theory of Structure Formation) models considered in this work. Here, αχ is the coupling between the mediator and dark matter, αν is the coupling between the mediator and a massless neutrinos-like fermion, mϕ is the mass of the mediator, and mχ is the mass of the DM particle. The parameter a4 is the coefficient of the power-law expansion in redshift of the DM drag opacity caused by the DM–DR interaction, which determines the linear initial matter power spectrum (see Cyr-Racine et al. 2016a). The parameters 〈σ〉30, 〈σ〉200, and 〈σ〉1000 are the DM self-interaction cross-sections at different velocities: 30, 200, and 1000 km s−1 and describe the velocity-dependent cross sections. We refer the reader to Vogelsberger et al. (2016) for more details on these models.

Nameαχανmϕ [Gev c−2]mχ [Gev c−2]a4 [h Mpc−1]〈σ〉30/mχ [cm2 g−1]〈σ〉200/mχ [cm2 g−1]〈σ〉1000/mχ [cm2 g−1]
ETHOS10.0710.1230.723200014095.654.980.0720.0030
ETHOS20.0160.030.835001784.059.00.1970.00097
ETHOS30.0060.0181.15178305.9416.90.480.0028
ETHOS40.51.55.03700286.090.160.0220.00075
Nameαχανmϕ [Gev c−2]mχ [Gev c−2]a4 [h Mpc−1]〈σ〉30/mχ [cm2 g−1]〈σ〉200/mχ [cm2 g−1]〈σ〉1000/mχ [cm2 g−1]
ETHOS10.0710.1230.723200014095.654.980.0720.0030
ETHOS20.0160.030.835001784.059.00.1970.00097
ETHOS30.0060.0181.15178305.9416.90.480.0028
ETHOS40.51.55.03700286.090.160.0220.00075
Table 1.

Relevant parameters of the ETHOS (Effective Theory of Structure Formation) models considered in this work. Here, αχ is the coupling between the mediator and dark matter, αν is the coupling between the mediator and a massless neutrinos-like fermion, mϕ is the mass of the mediator, and mχ is the mass of the DM particle. The parameter a4 is the coefficient of the power-law expansion in redshift of the DM drag opacity caused by the DM–DR interaction, which determines the linear initial matter power spectrum (see Cyr-Racine et al. 2016a). The parameters 〈σ〉30, 〈σ〉200, and 〈σ〉1000 are the DM self-interaction cross-sections at different velocities: 30, 200, and 1000 km s−1 and describe the velocity-dependent cross sections. We refer the reader to Vogelsberger et al. (2016) for more details on these models.

Nameαχανmϕ [Gev c−2]mχ [Gev c−2]a4 [h Mpc−1]〈σ〉30/mχ [cm2 g−1]〈σ〉200/mχ [cm2 g−1]〈σ〉1000/mχ [cm2 g−1]
ETHOS10.0710.1230.723200014095.654.980.0720.0030
ETHOS20.0160.030.835001784.059.00.1970.00097
ETHOS30.0060.0181.15178305.9416.90.480.0028
ETHOS40.51.55.03700286.090.160.0220.00075
Nameαχανmϕ [Gev c−2]mχ [Gev c−2]a4 [h Mpc−1]〈σ〉30/mχ [cm2 g−1]〈σ〉200/mχ [cm2 g−1]〈σ〉1000/mχ [cm2 g−1]
ETHOS10.0710.1230.723200014095.654.980.0720.0030
ETHOS20.0160.030.835001784.059.00.1970.00097
ETHOS30.0060.0181.15178305.9416.90.480.0028
ETHOS40.51.55.03700286.090.160.0220.00075
Close
This Feature Is Available To Subscribers Only

Sign In or Create an Account

Close

This PDF is available to Subscribers Only

View Article Abstract & Purchase Options

For full access to this pdf, sign in to an existing account, or purchase an annual subscription.

Close