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THE QUESTION LIBRARY THE UNIVERSE

Why is there any matter left in the universe at all?

The matter in every star and body may be the remnant of a tiny early imbalance whose cause remains unknown.

THE SHORT ANSWER

Nobody knows yet. The young universe had both matter and antimatter. When matching particles met, they turned much of their mass into energy. But matter seems to have had a small lead. CERN puts it at about one extra matter particle for every billion antimatter particles. That small surplus was left after most pairs met. It became the stuff in stars and our bodies. We have found some ways in which matter and antimatter differ, but they cannot yet explain the surplus.

  • Matter and antimatter can meet and turn into light and other particles.
  • CERN says there was about one extra matter particle for each billion antimatter particles.
  • That small surplus became the matter in stars, planets and our bodies.
  • Tests show some ways in which matter and antimatter differ, but they do not yet solve this puzzle.
Exterior of the Antimatter Factory building at CERN.
About this picture

CERN's Antimatter Factory lets researchers study antiparticles. Laboratory antimatter is a clue to a question about the early universe, not a recreation of its conditions.

Mramoeba, via Wikimedia Commons · CC0 1.0 · Image source ↗

WHERE THE EVIDENCE STANDS

How sure are we?

  • A small excess of matter survived the early universe.ESA states that the early universe had slightly more matter than antimatter and that the antimatter disappeared through annihilation; CERN calls a tiny excess of about one per billion “the current best explanation.”
  • Some particle processes treat matter and antimatter differently.CERN reports measured charge–parity violation, including LHCb's observed baryon decay asymmetry published in Nature in 2025.
  • Known particle physics fully explains the cosmic surplus.CERN says the CP violation predicted by the Standard Model is many orders of magnitude too small to account for the observed cosmic imbalance.
  • What produced the early matter surplus remains unknown.CERN calls understanding the source of the matter–antimatter asymmetry one of the greatest challenges in physics today.
What the labels mean

WHAT WE DON’T KNOW YET

We do not know what made matter get ahead. We also cannot watch the first moments of the universe as they happened.

WHAT WOULD CHANGE THIS ANSWER

A new idea must predict the size of the surplus and pass tests in labs and in space. Then it could explain why matter was left.

Nobody knows yet why any matter was left. This is a question about the young universe. It asks why matter did not cancel out with antimatter. Each matter particle has an antimatter partner. When the two meet, they can turn much of their mass into energy. CERN says the young universe had huge numbers of both kinds.

Here is an analogy. Picture two groups of people. Each person in one group leaves with a partner from the other group. If the groups match in size, no one stays. If one group has a few extra people, they stay after the rest leave. Real particles do not line up like people. Their meetings also make light and other particles. But the image shows how a tiny lead can leave a trace.

CERN says matter had about one extra particle for each billion antimatter particles. Most pairs met and were lost from the matter count. The small surplus became the matter in stars, planets and living things. This number helps us see the scale. It is not a head count made at the Big Bang.

Tests show that matter and antimatter do not always act alike. One form of this is called CP violation. It means a process can change when we swap particles for their antimatter partners and reverse left and right. In 2025, CERN's LHCb team found this kind of difference in a type of particle decay. But CERN says the effects in today's main particle theory are far too small to make the surplus we see. We know the matter is here. We do not yet know what gave it the lead.

THE LONG ANSWER

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Words worth knowing (4)
Antimatter
Particles paired with matter particles, with the same mass and opposite charge when charged.
Annihilation
A process in which a particle and its antiparticle meet and their energy becomes other particles and radiation.
CP violation
A difference that remains when a process is compared with one in which particles and antiparticles are exchanged and spatial directions reversed.
Standard Model
The leading tested theory of known elementary particles and their non-gravitational interactions.

Sources & further reading

(4) · Checked Sep 28, 2026
  1. Antimatter ↗CERNPairs produced and annihilated, leaving mostly photons and pions; “current best explanation” of a tiny excess, about one extra particle per billion antiparticles; source of the asymmetry one of the greatest challenges in physics today.
  2. A new piece in the matter–antimatter puzzle ↗CERN2025 LHCb observation of CP violation in baryon decays; 2.45% ± 0.47% is decay asymmetry, not cosmic surplus; known Standard Model CP violation is insufficient.
  3. CMS explores subtle matter–antimatter difference using beauty mesons ↗CERN17 July 2026: calls the matter excess one of the greatest mysteries in physics and CP violation one ingredient that could help explain it; CMS results agree with the Standard Model.
  4. History of cosmic structure formation ↗European Space AgencyWithin the first second, slightly more matter than antimatter; annihilation left particles dominant and antimatter disappeared; dark matter an unknown type of massive particle.

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