R-layer Mode Theory (RLMT) XLI‑L: Multiply-Imaged Type Ia Supernovae as Precision Probes

This volume develops the first full cosmographic application of R-layer Mode Theory (RLMT) to multiply-imaged Type Ia supernovae, focusing on the JWST discovery of SN H0pe. In RLMT, the observed Hubble parameter is a projection of a higher-layer tension field, and different cosmological probes sample different layers. SN H0pe provides three images, two time delays, and three absolute magnifications, enabling the first direct reconstruction of the mid-layer expansion rate, H_mid ≈ 72 km/s/Mpc. This value lies between the TRGB and CMB determinations, offering direct observational evidence for layered cosmic expansion. The volume further presents predictions for future JWST, Roman, and Euclid observations, including the universality of the ordering H_low < H_high < H_mid and the expected appearance of additional multiply-imaged SNe Ia in the G165 field.

Authors

Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-06-24
DOI
https://doi.org/10.5281/zenodo.20821930
Primary Topic
Gamma-ray bursts and supernovae
Type
preprint
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preprint

R-layer Mode Theory (RLMT) XLI‑L: Multiply-Imaged Type Ia Supernovae as Precision Probes

Tsuyoshi Tohi
Zenodo (CERN European Organization for Nuclear Research)
Gamma-ray bursts and supernovae
preprint

R-layer Mode Theory (RLMT) XLI‑L: Multiply-Imaged Type Ia Supernovae as Precision Probes

Tsuyoshi Tohi
preprint en

Abstract

This volume develops the first full cosmographic application of R-layer Mode Theory (RLMT) to multiply-imaged Type Ia supernovae, focusing on the JWST discovery of SN H0pe. In RLMT, the observed Hubble parameter is a projection of a higher-layer tension field, and different cosmological probes sample different layers. SN H0pe provides three images, two time delays, and three absolute magnifications, enabling the first direct reconstruction of the mid-layer expansion rate, H_mid ≈ 72 km/s/Mpc. This value lies between the TRGB and CMB determinations, offering direct observational evidence for layered cosmic expansion. The volume further presents predictions for future JWST, Roman, and Euclid observations, including the universality of the ordering H_low < H_high < H_mid and the expected appearance of additional multiply-imaged SNe Ia in the G165 field.

Zenodo (CERN European Organization for Nuclear Research)
Gamma-ray bursts and supernovae
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