# SCRIPT: BH-COVER-V10 # Full-bleed cover: the black-hole art fills the screen behind the title (desktop), with the paper's two walls # drawn on it; on phones a cropped panel of the art sits above the text. Output: cover_v2_block.html + CSS. import base64 full='data:image/jpeg;base64,'+base64.b64encode(open('bh_art_full.jpg','rb').read()).decode() crop='data:image/jpeg;base64,'+base64.b64encode(open('bh_art.jpg','rb').read()).decode() def overlay(dx): cx=682+dx return f''' the horizon a geometric fold · §8.2 r = 6M a spectral wall · §8.1 ''' glow=lambda dx: f'' html=f'''
{glow(760)} {overlay(760)}

Jeromie Beasley

Beyond the
Event Horizon

What survives at a rigidity wall

A black hole carries one wall of each kind. The static base of its horizon is a fold: read in the right coordinate it is smooth, and nothing breaks there. Its innermost stable orbit is a Jordan block, where steady circling turns into a plunge. At both, what a single eigenvector reports can fail; the pair and its ledger come through exact.

Read the paper

Research edition 10 · October 2026 · every number checked by a script in the archive

p = 2 + 6M/r

Read from the epicyclic ratio, gravity's effective power reaches the inverse cube exactly at the innermost stable orbit.

376.73 Ω

The horizon's effective surface resistance is the impedance of empty space: a matched load that returns nothing.

2√(1 + tanh²2r) > 2

In the ideal squeezed state one Hawking pair beats Bell's bound at every frequency, while its outside half stays thermal.

10597 → 4

Ramanujan's two functions each blow up near −1; their signed combination lands on 4.

''' css=''' ''' paper=open('bh_paper_v10_nocover.html').read() assert paper.count('')==1 and paper.count('')==1 out=paper.replace('',css+'').replace('',''+html,1) open('bh_paper_v10.html','w').write(out) open('cover_v2_block.html','w').write(css+html) print('ok',len(out)//1024,'KB')