concept

new physics

Phenomena or particles beyond the Standard Model of particle physics, potentially revealing extra dimensions or new fields.
17 related articles

Description

New physics refers to any phenomenon or particle that cannot be explained by the Standard Model of particle physics, the remarkably successful but incomplete theory describing known fundamental particles and forces. The Standard Model leaves several mysteries unresolved: the nature of dark matter, the tiny mass of neutrinos, the hierarchy problem (why gravity is so weak), and the matter-antimatter asymmetry of the universe. New physics would encompass the particles or forces that fill these gaps, such as supersymmetric partners, axions, sterile neutrinos, or extra spatial dimensions.

History

The term 'new physics' gained prominence in the 1980s as the Standard Model became established and its limitations became clear. The concept of physics beyond the Standard Model has been a major driver of theoretical and experimental work since then.

How it works

The search for new physics typically involves looking for deviations from Standard Model predictions. This can be done at high-energy colliders (like the LHC) by searching for new particles produced in collisions, or in precision experiments that measure known quantities with extreme accuracy, looking for tiny discrepancies. Cosmological observations, such as the expansion rate of the universe or the distribution of galaxies, also provide indirect probes of new physics that might have influenced the early universe.

In practice

While new physics has not yet been discovered, the search drives the development of advanced detector technologies, superconducting magnets, and data analysis techniques that find applications in medical imaging and computing.

Fun fact

The muon's anomalous magnetic moment shows a 4.2-sigma discrepancy between experiment and Standard Model prediction, one of the most significant hints of new physics that has not yet reached the gold-standard 5-sigma threshold for discovery.

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Related articles · 17

HEP Phenomenology2026-06-181 minarXiv:2606.20393express
Neutrino Wind from Neutron Stars
In the depths of a neutron star, the remnant of an exploded star, matter is compressed so tightly that a teaspoon would weigh billions of tons. Within this superdense material, a special kind of force might be at work, one that affects only muon and tau neutrinos.
Cosmology2026-06-041 minarXiv:2606.05723express
Dark Energy That Will Disappear
Since the late 20th century, astronomers have known that the recession of galaxies is accelerating, as if pushed by an invisible tailwind.
HEP Phenomenology2026-05-272 minarXiv:2605.28248express
Dark matter tugs at satellites like invisible strings
A stone thrown into water leaves ripples. A satellite orbiting Earth also leaves a trace — not on water, but in the laws of physics. Its orbit is not a frozen line: it slowly rotates, like the hand of a giant clock.
General Relativity2026-05-242 minarXiv:2605.25071express
Black Holes in Dark Matter Halos
A fluffy ball of invisible web envelops a black hole. This web is dark matter, which doesn't shine but, through its weight, governs the motion of stars on the outskirts of galaxies. Astrophysicists have long seen such 'fluffy' clouds around cosmic objects and have mapped their profiles — how density falls from the center to the edge.
HEP Theory2026-05-131 minarXiv:2605.13490express
The Universe as a Finite Book: Why a Unified Plot Is Unattainable
Picture the Universe as a book with a finite number of pages. Its accelerated expansion, driven by dark energy, a mysterious substance pushing space apart, acts like an invisible binding: distant pages are forever glued together, becoming inaccessible chapters.
The Angular Momentum Symphony: When Weak Gravity Is Strong
Back in the 1930s, Fritz Zwicky noticed that the speeds of galaxies in clusters were too high for the visible mass. Later, Vera Rubin confirmed this for individual galaxies.
Physics and Society2026-05-111 minarXiv:2605.11058express
Big Mysteries: Survey Reveals Physicists' Disagreements
Physics often resembles the construction of a giant ship — the Universe. The physicist-engineers have yet to agree on the basic blueprints.
Cosmology2026-04-211 minarXiv:2604.19922express
Weighing neutrinos by watching galaxies dance
Neutrinos are the most abundant massive particles in the universe. Trillions of them pass through us every second, yet they leave barely a trace. Their collective gravity, though tiny, can influence the motion of entire galaxies. Think of two people approaching each other on a busy street; invisible passersby alter their speed.
HEP Theory2026-03-051 minarXiv:2603.05683express
Why the New Dark Energy Theory Collapsed
An attempt to suppress room background noise by adding anti-sound turns into speaker howl if the circuit has an error. A similar glitch occurred with a theory that set out to remove the main cosmic hum — the inexplicably weak dark energy.
HEP Phenomenology2026-02-192 minarXiv:2602.17620express
A 17 MeV Ghost Particle
In nuclear transitions of beryllium-8, helium-4, and carbon-12, physicists from the ATOMKI collaboration have been seeing extra events since 2020—as if, when an excited nucleus decays, something else is sometimes born besides the usual photons. The energy of this "something" is always the same: about 17 million electron-volts.
General Relativity2026-02-021 minarXiv:2602.02646express
A Universe Without the Big Bang: A Smooth Beginning
Traditional cosmology begins with the Big Bang — the idea of Georges Lemaître. However, a new approach, inspired by the work of Stephen Hawking, bypasses the mystery of the initial moment.
Cosmology2026-01-071 minarXiv:2601.04312express
Neutrino Decay Reconciles Two Worlds
In the thirties, Pauli realized: without tiny ghost-like particles, the energy of stars doesn't add up. Thus neutrinos were born — intangible wanderers that permeate everything.
Cosmology2026-01-041 minarXiv:2601.01525express
Why Has Cosmology Cracked?
The universe is a pie baked from a single recipe, but the teaspoon and the kitchen scale stubbornly show different amounts of sugar. That’s how it is with the expansion of the universe: measurements from nearby stars (the spoon) give one number, while those from the ancient light of the Big Bang (the scale) give a completely different one.
Quantum Physics2025-12-201 minarXiv:2512.18400express
The Quantum Coin: Bohr & von Neumann's Solution
A quantum particle, an inhabitant of the elementary particle world, resembles a coin spinning in the air: neither heads nor tails, but a blend of possibilities. Yet when it lands on the table, the outcome becomes definite. What serves as the table in a measurement?
Quantum Physics2025-10-091 minarXiv:2510.07844express
Listening to the Shudder of Space: The Nano-Mirror Experiment
Two great theories describe reality: one — how massive bodies cause curvature of space, the other — the Standard Model — governs elementary particles. Reconciling them remains elusive, like trying to describe an ocean storm in the language of a diamond lattice.
A Ghost in the Atom: How Vacuum Hides a Pseudoscalar
In 1976, Gerard 't Hooft noticed that the vacuum of a gauge theory is not as simple as it seems: it possesses a topological structure that manifests itself in a nonzero topological susceptibility.
Five Questions Physics Asks Philosophy
At night, an astronomer points a telescope at the edge of the visible universe and sees not stars but ripples — the imprint of the first moments. He knows these ripples should obey statistics, like the heights of people in a crowd. But he has only one crowd, and nothing to compare it with. This is cosmic variance.