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Astrophysics

Is Dark Matter Really Matter?

Jun-Qian Jiang, Arman Shafieloo

Featured August 8, 2026

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Simply

By letting both dark matter and dark energy properties change, the study finds that dark matter might have a tiny pressure, challenging the standard model and showing how these 'dark' components are deeply linked.

In depth
The study challenges the standard cosmological model's assumptions that dark matter is pressureless () and dark energy is a cosmological constant (). By jointly varying these equations of state using DESI DR2, DES supernovae, and CMB data, the authors find that both standard values are disfavored at approximately . This suggests a degeneracy where a positive can compensate for a dark energy equation of state , potentially reinterpreting observed phantom crossing preferences.

Key Takeaways

  • 1
    When the equations of state for dark matter () and dark energy () are varied simultaneously, both standard CDM values (, ) are disfavored at approximately .
  • 2
    The apparent preference for phantom crossing in dark energy models can be absorbed by allowing a non-zero , suggesting a degeneracy between the dark matter and dark energy sectors.
  • 3
    The Padé-w + $w_{DM}$ model, which describes non-phantom quintessence dark energy with a free dark matter equation of state, provides the best fit to the data among the tested parameterizations.

Conceptual Flow

HIGH LEVEL
1
Methodology: Testing Dark Sector Assumptions

The researchers checked if dark matter and dark energy act exactly as we thought, or if they have slightly different behaviors.

Universe Data
Standard Ideas
Compare & Adjust
New Dark Matter Rules
New Dark Energy Rules
2
Results: Interconnected Dark Properties

They found that dark matter might have a tiny pressure, and this changes how we understand dark energy, showing they are connected.

Dark Matter Pressure = Zero
Dark Energy = Constant
Not Quite Right
Dark Matter Has Pressure
Dark Energy Can Change