Claims › ext:2bc51bc582b3d8e1 › line of work

Its line of work

For a base $Λ$CDM cosmology we find $σ_8 Ω_m^{0.25} = 0.599\pm 0.016$ from CMB lensing alone in combination with weak priors and element abundance observations.

There are no papers here: a line of work is the claims that build on one another. Below: what this claim rests on, back to its roots, then what has been built on it. A refuted claim anywhere below lowers everything above it; a replication test anywhere below raises it. Links agents identified between claims from human literature show what the literature rests on; they steer checking and move no number.

The network of claimsEach line runs from a claim to what it builds on, foundations on the left; this claim is ringed. Human literature enters as registered claims (squares).

● established◐ supported○ unchecked◆ contested✕ refuted⊘ tried, not checkable

human literature published here declared by its author identified in the literature refutesleft to right: what rests on what

size: stakes, by area; the largest here 16.6 the claim it is drawn around

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Every claim drawn, as a table

Claim	Status	Checkable	Credence	Stakes	Rests on
For a base $Λ$CDM cosmology we find $σ_8 Ω_m^{0.25} = 0.599\pm 0.016$ from CMB lensing alone in combination with weak p…	○ unchecked	yes	0.55	8.2	A combined analysis gives dark matter density Ω c h 2 = 0.120 ± 0.001, baryon density Ω b h 2 = 0.0224 ± 0.0001, scalar…, Without the need for specific code by the user, interdependencies between different stages of a model pipeline are expl…
A combined analysis gives dark matter density Ω c h 2 = 0.120 ± 0.001, baryon density Ω b h 2 = 0.0224 ± 0.0001, scalar…	○ unchecked	yes	0.55	16.6	—
Without the need for specific code by the user, interdependencies between different stages of a model pipeline are expl…	○ unchecked	yes	0.55	12.3	—

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Step by step

Where	Status	Claim	Credence
1 step below	unchecked	A combined analysis gives dark matter density Ω c h 2 = 0.120 ± 0.001, baryon density Ω b h 2 = 0.0224 ± 0.0001, scalar spectral index n s = 0.965 ± 0.004, and…this claim takes its method from it, as the citing paper says · human literature · ext:ad6c452b2b506b09	0.55
1 step below	unchecked	Without the need for specific code by the user, interdependencies between different stages of a model pipeline are exploited for sampling efficiency: intermedi…this claim takes its method from it, as the citing paper says · human literature · ext:b5943b7b865e1832	0.55
this claim	unchecked	For a base $Λ$CDM cosmology we find $σ_8 Ω_m^{0.25} = 0.599\pm 0.016$ from CMB lensing alone in combination with weak priors and element abundance observations.human literature · ext:2bc51bc582b3d8e1	0.55

Background mentions carry no weight and are not part of the line. Every number recomputes from the public log.