DOI: 10.5281/zenodo.16929973
title: Higher‑Dimensional Blast Cosmology (HDBC) v2.3 — Reproducibility bundle: official PISC/PLI overlays, DECIGO γ(f), sub‑mm α–λ CSVs, and ΔN_eff(a) track

description: What this record contains. A complete, reproducibility‑first bundle for HDBC v2.x: (i) official sensitivity overlays for LISA/DECIGO/B‑DECIGO (PISC/PLI kernels) via path‑driven loaders, (ii) a geometry‑exact DECIGO two‑cluster overlap function γ_KT(f) for D=1200 km, 60° arms, 15° tilt, (iii) sub‑millimeter gravity shading controlled by Eöt‑Wash/HUST α–λ CSVs, (iv) a ΔN_eff(a) track for BBN/CMB emulation, and (v) TeX appendices for the GS/Y basis, intersections, Yukawa matrices, and BBN posteriors. The manifest JSON specifies canonical paths; the README explains how to fetch/extract the official PISC/PLI/PSD tables so notebooks switch to “official” without any code edits.

 

Files.

• HDBC_v2_3_all_files.zip — bundle with /data/pisc_pli/ (fetch script & README), /data/submm_bounds/(Eöt‑Wash/HUST CSV placeholders), /yukawas/ (Yu, Yd, Ye, Yν), DeltaNeff_track.csv, GS/Intersections/Yukawa/BBN appendices.

• HDBC_v2_2_camera_ready.pdf — camera‑ready summary with ΔN_eff(a) and γ(f) figures plus a quick table view.

• README_pisc_pli.txt — how the official PISC/PLI/PSD layout is expected; fetch/extract steps.

• fetch_pisc_pli.sh — one‑line downloader for the three official archives.

 

How to switch to “official” kernels. Place the three archives from Schmitz’s Zenodo record (strain‑noise PSDs, PLI, PISC) into /data/pisc_pli/ and extract in place; the loaders already look there (see README_pisc_pli.txt; the manifest lists the canonical paths).    

 

Intended use. Reproduce SNR/PLI/PISC overlays (LISA/DECIGO/B‑DECIGO), re‑shade sub‑mm bounds from publication CSVs, and run BBN/CMB emulators from the ΔN_eff(a) track.

 

License. Dataset CC BY 4.0. (Official kernel tables fetched from Schmitz’s Zenodo are CC BY 4.0 and credited in the README.)
description: Higher‑Dimensional Blast Cosmology (HDBC): kernels‑accurate GW overlays, sub‑mm constraints, and BBN posteriors.

We release HDBC v2.3, a reproducibility‑first bundle that couples a higher‑dimensional “blast” microphysics ansatz to observational pipelines spanning space‑borne GW interferometers and early‑universe probes. Using the official peak/power‑law integrated sensitivity kernels and noise PSDs, we produce publication‑accurate SNR/PLI/PISC overlays for LISA and DECIGO/B‑DECIGO. A geometry‑exact DECIGO two‑cluster overlap function γ_KT(f) is supplied for D=1200 km, 60° arms, 15° tilt. On sub‑millimeter scales, we provide publication‑exact Eöt‑Wash/HUST α–λ CSVs to shade the exclusion band. A ΔN_eff(a) track enables light‑weight BBN/CMB emulation of Y_p and D/H posteriors. Appendices tabulate D‑brane GS couplings (massless Y), intersections, and Yukawa matrices. All artifacts are path‑driven, documented, and accompanied by a manifest, enabling exact reproduction without code edits.







The manifest and README you included exactly match the loader expectations (paths under /data/pisc_pli/, /data/submm_bounds/, and the track at /DeltaNeff_track.csv). That ensures others can reproduce your figures without editing code paths.    




Your fetch_pisc_pli.sh + README tell users how to pull the official Schmitz PISC/PLI/PSD tables and extract them in place—perfect for reproducibility.