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CDN-323: The High-z HMF Amplification Ledger | Synapse

June 22, 20260 citationsOpen Access

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CDN-323: The High-z HMF Amplification Ledger

NHNicky Joseph Hubertus Catharina Hacquier

Key Points

The aim is to create a standalone ledger from GCFT-CLASS halo-mass-function outputs for high-redshift data.
Converts imported GCFT-CLASS high-redshift data into a ledger.
Reintegrates archived differential HMF tables for cumulative abundance analysis.
Records z=25 parameters against maximum relative P(k) distances.
Reproduced cumulative GCFT/LCDM abundance amplification at redshifts z=5 to z=30.
Established a new parameter envelope for observations at z=25.
Documented successful integration of archived HMF tables.

Abstract

CDN-323 converts the imported GCFT-CLASS high-redshift halo-mass-function outputs into a standalone evidence ledger. It independently reintegrates the archived differential HMF tables to reproduce the imported cumulative GCFT/LCDM abundance amplification at z=5 through z=30 and records the z=25 parameter envelope against the imported maximum relative P(k) distances.

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Nicky Joseph Hubertus Catharina Hacquier (Sat,) studied this question.

synapsesocial.com/papers/6a38d152da1bad9caca30f59 https://doi.org/https://doi.org/10.5281/zenodo.20768861

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