learn/steps in the work
Simulation
A simulation is a computer model that works out what something would do, step by step, from the rules it is thought to obey, so scientists can watch it happen without doing it.
What it is
A simulation starts with a description of a system and a set of rules about how it changes: atoms pulled about by the forces between them, light bent by the mass it passes, a star swelling as it burns through its fuel. The computer applies those rules over and over, in small steps of time or space, and records what comes out. Scientists can then look at the result as if it were an observation, except that they chose every condition themselves. Some simulations are built to reproduce reality closely; others are built to produce fake data that resembles what an instrument would collect, so methods can be tested on examples whose true answer is known.
Because the rules are often expensive to apply exactly, a second approach has grown up alongside. A model is trained on the results of the slow, careful calculation and learns to guess its answers directly. This learned stand-in, sometimes called a surrogate, does the same job far more cheaply, which lets scientists simulate things far bigger or for far longer than they could before. It is still a simulation: it is still working out what the system would do, just with a shortcut in place of the arithmetic.
Why scientists use it
Scientists simulate when the real thing is too slow, too small, too large, too dangerous or simply unavailable. You cannot watch glass form atom by atom, or wait for a star system to evolve, or build a telescope to see whether your analysis would have worked. The simulation stands in for the experiment or the observation. It also stands in for truth: when fake data is generated from known starting conditions, every answer is already known, so a method can be scored on how close it comes. That is how many machine-learning tools in the sciences are trained and checked at all.
A simulation is also a way of asking what if. Conditions can be changed one at a time, repeated exactly, and pushed to extremes that nature does not conveniently supply. And because a simulation can be run many times, it can be put inside a loop: run it, see where its answers are least trustworthy, go back to the slower and more reliable method for just those cases, and improve the fast model with what you learn.
In the record
Limits
A simulation can only contain the rules it was given. Leave out a force, a source of noise or a piece of physics, and the output will be confidently wrong in exactly that respect, which matters most when simulated data is used to train or test a method that will later meet the real world. Learned stand-ins add a second gap: they are reliable only for the kinds of cases they were trained on, and may fail quietly on anything unfamiliar. Agreement with a simulation is never, on its own, agreement with nature.
Written by AIxSci: the background from general knowledge, the examples from checked records.
Every article
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Machine learning sorts a simulated polymer into ordered and disordered beads
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Reconstructing the early universe's density field with a smoothed map of cosmic structure
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Sparse regression fits crystal force constants to model heat flow and vibrations
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Neural network supplies the sideways flows needed to measure the quiet Sun's magnetic energy
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Neural network predicts how titanium alloy grains round off during annealing
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Neural networks trained on molecule pairs predict light absorption in stacks of fifty
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Neural networks weigh cluster X-ray maps to estimate galaxy cluster masses
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Neural network models simulate how lead titanate loses its electrical polarisation on heating
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Image classifiers flag a gas kink in a young star's disc, pointing to a planet
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Neural networks read a fast radio burst's dispersion straight from its spectrum
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Neural network predicts atomic charges from bond lists, without atomic coordinates
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Neural network designs five hard metallic glasses, all confirmed by experiment
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Machine learning fitted to flexible molecules predicts oxidation potentials and hydration energies
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Neural networks stand in for a slow model of interstellar gas clouds
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Machine learning assigns atomic charges to size up polarisation in bismuth vanadate conductors
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AlphaFold models used to map membrane-crossing segments in human proteins
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Neural networks pick amino acid sequences for short peptides in protein binding sites
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AlphaFold2 used to predict the shapes of hepatitis E virus copying proteins
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Testing whether symmetry-aware neural networks can tell apart atomic arrangements in perovskites
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Neural networks predict how zeolites take up carbon dioxide from structure alone
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Peptides designed by simulation and machine learning sit at condensate surfaces
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Thin molybdenum disulfide memory cells tested, with reinforcement learning fitting their circuit model
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Machine-learned potentials trained to simulate copper ion conductor Cu7PS6 faster
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Seven machine-learned water models test how density functional choice shapes water's behaviour
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Machine learning predicts nanofibre thickness from electrospinning settings, tested against new scaffolds
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Simulations probe shape-shifting of opium poppy's reticuline-flipping enzyme using a predicted structure
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Neural network potentials trained by repeatedly checking where models disagree on hydrogen sticking to copper
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Clustering algorithm sorts cluster stars from background stars in thirteen open clusters
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Meta-learning lets a cosmology emulator adapt to new galaxy depth maps quickly
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Five codes measured galaxy shapes in simulated Euclid images, one using neural networks
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Machine-learned potential predicts how chromium sulfide layers rearrange during exfoliation
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Machine-learned potential makes long simulations of CO hydrogenation on rhodium affordable
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Neural network predicts nanostructure optics to design a two-colour laser collimator
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Language model trained on protein sequences predicts shape and stability of disordered proteins
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Machine-learned force field used to model two crystal forms of formamide
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Neural network stands in for slow spectral modelling to read 64 stars' chemistry
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Researchers train a machine-learned force model to simulate carbon nanotubes' strength and heat limits
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Diffusion model generates glass and silicon structures to order from target properties
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Neural networks sort supernovae and estimate their distances from brightness alone
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Pretrained potentials give a structure search a head start in finding atomic arrangements
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Classifying stars by type from a single wide-band telescope image
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Neural networks swap places with black hole image simulations, both directions
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Neural network potential used to simulate how calcium oxide melts under pressure
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Zero-padding lets one neural network encode crystals with differing element counts
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Oxidation potentials for 15,238 molecules assembled from quantum calculations and lab measurements
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Simulations map three sodium–bismuth compounds, then models predict their heat-to-electricity performance
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Neural networks speed up forecasts of what gravitational wave detections LISA will catch
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Two protein design models redesigned T cell receptor contact points on solved structures
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Neural network potential used to simulate carbon dioxide moving inside porous frameworks
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Neural network force field simulates how a ferroelectric crystal's molecules begin to spin
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Machine learning reads planet-forming disk masses from archival ALMA observations
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Neural networks trained on atomic surroundings score how mutations change proteins
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Neural network retrained to predict how crystals absorb light, from few examples
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Neural networks recover a simulated barred galaxy's gravity from one snapshot
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Neural networks trained on simulated radio bursts sort real bursts by shape
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Neural networks read simulated galaxy cluster catalogues to estimate cosmological parameters
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A compact neural network learns to generate shape-shifting protein structures
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Machine learning sifts three-colour infrared survey data for cold brown dwarfs
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Simulated water in graphene gaps shows acid's charge hugging the surface
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Software predictions map floppy stretches of touch-sensing PIEZO channels
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Simulations map how surface atoms rearrange in alloys when molecules attach
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Neural network scores candidate composite microstructures in a strength–toughness design loop
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A single neural network stands in for quantum calculations across 45 elements
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Neural networks stand in for slow cosmology code in parameter fitting
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Machine-learnt stand-in for a planet model cuts interior inference from 42 hours to 8 minutes
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Genetic algorithm trims chemical reaction lists for hot Jupiter atmosphere models
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Neural networks sift 315,000 galaxy images for rare polar ring systems
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Eight machine learning methods sorted supernova gravitational wave signals by nuclear physics model
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Neural networks stand in for slow galaxy clustering calculations in cosmology analyses
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Two neural networks predict how heat shrinks the band gap of silver-based crystals
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Neural network reads simulated quasar light curves to estimate black hole properties
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Machine-learnt electron densities drive molecular dynamics of a gold–saltwater interface
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Two unsupervised methods compress fast radio burst spectra into a handful of numbers
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Machine learning predicts whether a dying massive star explodes, from its density profile
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Hubble and Webb images reveal a candidate massive touching binary star in WLM
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Four million simulated X-ray patterns used to test 21 crystal-symmetry classifiers
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Neural network built from physics equations extracts solder deformation coefficients
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Neural network turns galaxy shape distortions into maps of invisible cluster mass
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Neural network trained on quantum calculations maps how gallium melts and freezes
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Neural networks read infrared spectra to work out how CO sits on platinum
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Machine learning picked which engineered enzymes to build for fatty alcohol production
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Machine learning picked which shape-memory alloys to make next, round by round
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Transformer model predicts how gas-storing crystals take up gases, replacing slow simulations
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Neural network segments 650 battery particles to measure their detachment after cycling
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Machine-learned force model simulates silicon-oxygen structures from glass surfaces to monoxide grains
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