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CosmoBuilder

Struct CosmoBuilder 

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pub struct CosmoBuilder { /* private fields */ }

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impl CosmoBuilder

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pub fn new() -> Self

Create a new builder with default accuracy settings.

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pub fn flat(self) -> Self

Enforce spatial flatness (Ω_k = 0) and solve for ω_Λ by closure.

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pub fn h(self, val: f64) -> Self

Set the dimensionless Hubble parameter h (H0 = 100 h).

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pub fn H0(self, val: f64) -> Self

Set H0 in (km/s)/Mpc (converted internally to h).

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pub fn Omega_m(self, val: f64) -> Self

Set total matter density Ω_m.

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pub fn Omega_b(self, val: f64) -> Self

Set baryon density Ω_b.

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pub fn Omega_cdm(self, val: f64) -> Self

Set CDM density Ω_cdm.

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pub fn Omega_k(self, val: f64) -> Self

Set curvature density Ω_k.

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pub fn Omega_L(self, val: f64) -> Self

Set dark energy density Ω_Λ.

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pub fn omega_b_phys(self, val: f64) -> Self

Set physical baryon density ω_b.

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pub fn omega_cdm_phys(self, val: f64) -> Self

Set physical CDM density ω_cdm.

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pub fn T_cmb0(self, val: f64) -> Self

Set the present-day CMB temperature T_cmb0 in Kelvin.

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pub fn accuracy(self, val: AccuracyPreset) -> Self

Set the global accuracy preset controlling numerical settings.

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pub fn neutrino_effective(self, n_eff: f64, masses_ev: Vec<f64>) -> Self

Use an “effective” neutrino model with total n_eff and a mass list.

For massless neutrinos, pass [0.0] (or multiple zeros if you want explicit states).

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pub fn neutrino_split( self, n_ur: f64, masses_ev: Vec<f64>, temp_factors: Vec<f64>, ) -> Self

Use a “split” neutrino model with explicit ultra-relativistic contribution n_ur plus a list of massive eigenstates and per-species temperature factors.

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pub fn build(self) -> Result<ScientificParams, String>

Build ScientificParams by resolving inputs, enforcing consistency, and computing all derived quantities.

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impl Clone for CosmoBuilder

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fn clone(&self) -> CosmoBuilder

Returns a duplicate of the value. Read more
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fn clone_from(&mut self, source: &Self)

Performs copy-assignment from source. Read more
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impl Debug for CosmoBuilder

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fn fmt(&self, f: &mut Formatter<'_>) -> Result

Formats the value using the given formatter. Read more
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impl Default for CosmoBuilder

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fn default() -> CosmoBuilder

Returns the “default value” for a type. Read more

Auto Trait Implementations§

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impl<T> Any for T
where T: 'static + ?Sized,

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fn type_id(&self) -> TypeId

Gets the TypeId of self. Read more
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impl<T> Borrow<T> for T
where T: ?Sized,

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fn borrow(&self) -> &T

Immutably borrows from an owned value. Read more
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impl<T> BorrowMut<T> for T
where T: ?Sized,

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fn borrow_mut(&mut self) -> &mut T

Mutably borrows from an owned value. Read more
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impl<T> CloneToUninit for T
where T: Clone,

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unsafe fn clone_to_uninit(&self, dest: *mut u8)

🔬This is a nightly-only experimental API. (clone_to_uninit)
Performs copy-assignment from self to dest. Read more
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impl<T> From<T> for T

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fn from(t: T) -> T

Returns the argument unchanged.

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impl<T, U> Into<U> for T
where U: From<T>,

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fn into(self) -> U

Calls U::from(self).

That is, this conversion is whatever the implementation of From<T> for U chooses to do.

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impl<T> ToOwned for T
where T: Clone,

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type Owned = T

The resulting type after obtaining ownership.
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fn to_owned(&self) -> T

Creates owned data from borrowed data, usually by cloning. Read more
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fn clone_into(&self, target: &mut T)

Uses borrowed data to replace owned data, usually by cloning. Read more
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impl<T, U> TryFrom<U> for T
where U: Into<T>,

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type Error = Infallible

The type returned in the event of a conversion error.
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fn try_from(value: U) -> Result<T, <T as TryFrom<U>>::Error>

Performs the conversion.
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impl<T, U> TryInto<U> for T
where U: TryFrom<T>,

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type Error = <U as TryFrom<T>>::Error

The type returned in the event of a conversion error.
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fn try_into(self) -> Result<U, <U as TryFrom<T>>::Error>

Performs the conversion.