Spin–Spin Coupling Constant: Overview
¹H NMR: Long-Range Coupling
Spin–Spin Coupling: One-Bond Coupling
¹³C NMR: ¹H–¹³C Decoupling
Spin–Spin Coupling: Two-Bond Coupling (Geminal Coupling)
Spin–Spin Coupling: Three-Bond Coupling (Vicinal Coupling)
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Updated: May 28, 2026

Setting Limits on Supersymmetry Using Simplified Models
Published on: November 15, 2013
A Avgoustidis1, E J Copeland, A Moss
1Centre for Theoretical Cosmology, DAMTP, CMS, Wilberforce Road, Cambridge CB3 0WA, United Kingdom.
Cosmic superstrings with multiple tensions and Y junctions leave imprints on the cosmic microwave background (CMB). The string coupling constant g(s) influences network density, potentially shifting the B-mode peak for direct constraint.
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