New Study Sets Stronger Mass Limit on Ultralight Bosonic Dark Matter 6573w

Researchers set a new lower mass limit of 2.2 × 10⁻²¹ eV for ultralight bosonic dark matter using stellar motion data from Leo II. 4i5j53

New Study Sets Stronger Mass Limit on Ultralight Bosonic Dark Matter

Photo Credit: Physical Review Letters 693q4j

New Study Sets Stronger Mass Limit on Ultralight Bosonic Dark Matter

Highlights
  • New dark matter lower mass bound is 2.2 × 10⁻²¹ electron volts
  • Study challenges fuzzy dark matter model assumptions directly
  • Uses stellar data from Leo II and quantum physics tools
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Over 80 years, dark matter has been a great mystery for the researchers. Elusive of direct observation, it has made its existence known only by the gravitational impacts it makes on dark matter particles.

About the study j662z

According to the study published in Physical Review Letters, the mass of ultralight bosonic dark matter must be more than 2 × 10-21 electron volts (eV), 100 times more than previous estimates using Heisenberg's uncertainty principle.

The team of researchers, led by the first author of the study, Tim Zimmermann, a Ph.D. candidate at the Institute of Theoretical Astrophysics, University of Oslo, focused their method on the data of Leo II, the Milky Way's satellite galaxy. It is a Milky Way. By analyzing the internal motions of stars within Leo II—heavily influenced by dark matter—the team derived 5,000 possible dark matter density profiles using a tool called GRAVSPHERE.

They compared these with profiles generated by quantum wave functions of various dark matter particle masses. If the particle is too light, quantum fuzziness spreads it too thinly, preventing it from forming the observed structures. The study concluded that the dark matter particle must have a mass greater than 2.2 × 10⁻²¹ electron volts (eV)—over 100 times more than previous lower estimates.

Impact on dark matter studies 2u5g4j

The findings have significant implications for popular ultralight dark matter models, particularly fuzzy dark matter, which typically proposes particles with masses around 10-22 ev.

Looking ahead, the team plans to extend their methodology to mixed dark matter scenarios, where dark matter is composed of particles with different masses.

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Further reading: Astronomy News
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