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Amber26 is now available!

We are pleased to announce the release (on April 30, 2026) of version 26 of the Amber software suite. (How to order.) This represents a significant update from version 24, which was released in April, 2024.

The Amber26 package adds the pmemd program, which resembles the sander (molecular dynamics) code in AmberTools, but provides (much) better performance on multiple CPUs, and dramatic speed improvements on GPUs.

Major new features include:

Improvements to Advanced Methods

  • Enhancements to alchemical transformation pathways/softcore potentials and alchemical enhanced sampling (ACES) method:
    • advanced lambda scheduling options including new tools for optimized phase space overlap lambda-spacing
    • scaffold-hopping and absolute binding free energy capability through lambda-dependent "Boresch" bond, angle, and torsion restraints
    • lambda-dependent RMSD-fitting restraints to floating reference molecular scaffolds
    • non-equilibrium work framework (Jarzynski and Crooks equations) for alchemical free energy transformations and end-state (e.g., MM->QM or MM->ML) book-ending simulations
    • advanced methods for network-wide alchemical free energy analysis of protein-ligand binding thermodynamic graphs with cycle closure and experimental constraints.
  • Improved REMD structure reservoir options, including reservoirs for H-REMD and flexible reservoir temperature with T-REMD
  • Gaussian accelerated MD (LIG-GaMD).

Improved Implicit Solvent Methods

  • New tensor-based Poisson-Boltzmann solver backend in PBSA, with GPU acceleration, preconditioning, and matrix-free operation.
  • Bundled LibTorch now ships in two versions (2.5.1 and 2.10.0), expanding CUDA support from 11.8 through 13.0.
  • Implicit solvent/explicit ion solvent model (GBION). The parameters have been refined to handle DNA and protein-DNA complexes, most importantly the nucleosome.
  • Added highly-accurate dSASA method for calculating the solvent accessible surface area in nonpolar solvation free energy calculations, as well as forces required for MD simulations.
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