func initCorrectedHalo(h *Halo, cFunc num.Func1D, m500cCorrect float64) {
rho500c := cosmo.RhoCritical(h.Z) * 500
h.C500.M = m500cCorrect
h.C500.R = haloRadius(h.C500.M, rho500c)
initSearching(h, cFunc, h.C500.M, h.C500.R)
// initDensityInfo may require that r500cBias and m500cBias be initialized.
if h.ppt.RequiresBiasedMass() {
// initial guess
h.M500cBias = h.C500.M
h.R500cBias = h.C500.R
r500cBiasLhs := func(r500cBias float64) float64 { return r500cBias }
r500cBiasRhs := func(r500cBias float64) float64 {
h.R500cBias = r500cBias
h.M500cBias = haloMass(r500cBias, rho500c)
return h.OverdensityRadius(Biased, rho500c)
}
h.R500cBias = num.FindEqual(r500cBiasLhs, r500cBiasRhs,
h.C500.R/2, h.C500.R)
h.M500cBias = haloRadius(h.R500cBias, rho500c)
}
initDensityInfo(h, cFunc, h.C500.M, h.C500.R)
h.R500cBias = h.OverdensityRadius(Biased, rho500c)
h.M500cBias = haloMass(h.R500cBias, rho500c)
}
// initDensityInfo modifies h so that its various DensityInfo fields
// correspond to a halo with the given m500c. Also updates h.Rs and h.rhoS
func initDensityInfo(h *Halo, cFunc num.Func1D, m, r float64) {
rho500c := cosmo.RhoCritical(h.Z) * 500
rho200a := cosmo.RhoAverage(h.Z) * 200
// This sets c200 for us.
initSearching(h, cFunc, m, r)
h.A200.R = h.OverdensityRadius(Corrected, rho200a)
h.A200.C = h.A200.R / h.Rs
h.A200.M = haloMass(h.A200.R, rho200a)
h.C500.R = h.OverdensityRadius(Corrected, rho500c)
h.C500.C = h.C500.R / h.Rs
h.C500.M = haloMass(h.C500.R, rho500c)
// This will already be set if the biased mass is required.
if !h.ppt.RequiresBiasedMass() {
h.R500cBias = h.OverdensityRadius(Biased, rho500c)
h.M500cBias = haloMass(h.R500cBias, rho500c)
}
}
func initBiasedHalo(h *Halo, cFunc num.Func1D, m500cBias float64) {
rho500c := 500 * cosmo.RhoCritical(h.Z)
h.R500cBias = haloRadius(m500cBias, rho500c)
h.M500cBias = m500cBias
bFracLhs := func(b float64) float64 { return b }
bFracRhs := func(b float64) float64 {
initSearching(h, cFunc, b*h.M500cBias, h.R500cBias)
h.C500.R = h.OverdensityRadius(Corrected, rho500c)
h.C500.M = haloMass(h.C500.R, rho500c)
return h.BFrac(h.R500cBias)
}
// h.BFrac evaluated at r500cBias
b := num.FindEqual(bFracLhs, bFracRhs, 1.0, 2.0)
mR500cBias := m500cBias * b
initDensityInfo(h, cFunc, mR500cBias, h.R500cBias)
}
func initSearching(h *Halo, cFunc num.Func1D, m, r float64) {
rho200c := cosmo.RhoCritical(h.Z) * 200
m200cToR := func(m200c float64) float64 {
h.C200.R = haloRadius(m200c, rho200c)
h.C200.C = cFunc(m200c)
h.C200.M = m200c
h.Rs = h.C200.R / h.C200.C
return h.MassEnclosed(Corrected, r)
}
m200c := num.FindEqualConst(m200cToR, m, m, m)
h.C200.R = haloRadius(m200c, rho200c)
h.C200.C = cFunc(m200c)
h.C200.M = m200c
h.Rs = h.C200.R / h.C200.C
}
func pThermal(h *Halo, ppt PressureProfileType, pt PressurePopulationType, r float64) float64 {
type battagliaParam func(m500c, z float64) float64
makeBattagliaParam := func(a0, am, az float64) battagliaParam {
return func(m500c, z float64) float64 {
return a0 * math.Pow(1+z, az) *
math.Pow(m500c/battagliaPMassPivot, am)
}
}
pDeltaBattaglia := pDeltaBattagliaPre * cosmo.RhoCritical(h.Z) *
h.C500.M / h.C500.R
switch pt {
case AllPressure:
muFrac := cosmo.Mu / cosmo.ElectronMu
return pThermal(h, ppt, ElectronPressure, r) * muFrac
case ElectronPressure:
switch ppt {
case Planck2012:
// This is a measured fit, so we need to use the biased mass.
mFrac := h.M500cBias / (planckPivotM500H / cosmo.H70)
x := r / h.R500cBias
y := planckC500 * x
scaledPressure := planckP0 / (math.Pow(y, planckGamma) *
math.Pow(1.0+math.Pow(y, planckAlpha),
(planckBeta-planckGamma)/planckAlpha))
P500 := (planckA0kev * math.Pow(mFrac, 2.0/3.0+0.12) *
math.Pow(cosmo.HubbleFrac(h.Z), 8.0/3.0) *
(cosmo.H70 * cosmo.H70))
PkeV := P500 * scaledPressure
return PkeV * kevToPascal
case Arnaud2009:
mFrac := h.M500cBias / (arnaudPivotM500H / cosmo.H70)
x := r / h.R500cBias
y := arnaudC500 * x
app := 0.1 - (arnaudAP+0.1)*math.Pow(x/2, 3.0)/
(1+math.Pow(x/2, 3.0))
scaledPressure := +math.Pow(mFrac, arnaudAP+app) *
math.Pow(cosmo.H70, -1.5) *
arnaudP0 / (math.Pow(y, arnaudGamma) *
math.Pow(1+math.Pow(y, arnaudAlpha),
(arnaudBeta-arnaudGamma)/arnaudAlpha))
P500 := (arnaudA0kev * math.Pow(mFrac, 2.0/3.0) *
math.Pow(cosmo.HubbleFrac(h.Z), 8.0/3.0) *
(cosmo.H70 * cosmo.H70))
PkeV := P500 * scaledPressure
return PkeV * kevToPascal
case BattagliaAGN2012:
x := r / h.C500.R
p0 := makeBattagliaParam(battagliaP0AGN,
battagliaPmAGN,
battagliaPzAGN)
xc := makeBattagliaParam(battagliaX0AGN,
battagliaXmAGN,
battagliaXzAGN)
beta := makeBattagliaParam(battagliaB0AGN,
battagliaBmAGN,
battagliaBzAGN)
xFrac := x / xc(h.C500.M, h.Z)
muFrac := cosmo.Mu / cosmo.ElectronMu
return p0(h.C500.M, h.Z) * math.Pow(xFrac, battagliaPGamma) *
math.Pow(1.0+math.Pow(xFrac, battagliaPAlpha),
-beta(h.C500.M, h.Z)) * pDeltaBattaglia / muFrac
case BattagliaShockHeating2012:
x := r / h.C500.R
p0 := makeBattagliaParam(battagliaP0ShockHeating,
battagliaPmShockHeating,
battagliaPzShockHeating)
xc := makeBattagliaParam(battagliaX0ShockHeating,
battagliaXmShockHeating,
battagliaXzShockHeating)
beta := makeBattagliaParam(battagliaB0ShockHeating,
battagliaBmShockHeating,
battagliaBzShockHeating)
xFrac := x / xc(h.C500.M, h.Z)
muFrac := cosmo.Mu / cosmo.ElectronMu
return p0(h.C500.M, h.Z) * math.Pow(xFrac, battagliaPGamma) *
math.Pow(1.0+math.Pow(xFrac, battagliaPAlpha),
-beta(h.C500.M, h.Z)) * pDeltaBattaglia / muFrac
}
panic("Given unrecognized PressureProfileType.")
}
panic("Given unrecognized PressureType.")
}