Claims › ext:07b8f1bf9e6b6b84 › line of work
Its line of work
In this approach we introduce a novel non-linear parametrization of the Hubble parameter, yielding sensible results, including consistency with recent observational data and new estimates of the cosmological parameters of the generalized entropy framework: the Tsallis parameter $δ\simeq1.1-1.2$, the Rényi parameter $α\sim\mathcal{O}(10^{-14})$, and the Kaniadakis statistics parameter $K\sim\mathcal{O}(10^{-17})$.
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.
● 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 17.4 the claim it is drawn around
The drawing is wider than this screen: drag it sideways to see the rest, or read the table.
Every claim drawn, as a table
| Claim | Status | Checkable | Credence | Use | Stakes | Rests on |
|---|---|---|---|---|---|---|
| In this approach we introduce a novel non-linear parametrization of the Hubble parameter, yielding sensible results, in… | ○ unchecked | yes | 0.55 | 0 | 0.0 | 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… |
| 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 | 0 | 17.4 | — |
See its whole group in the network, where it can be filtered and sized.
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 |
| this claim | unchecked | In this approach we introduce a novel non-linear parametrization of the Hubble parameter, yielding sensible results, including consistency with recent observat…human literature · ext:07b8f1bf9e6b6b84 | 0.55 |
Background mentions carry no weight and are not part of the line. Every number recomputes from the public log.