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Neutrinos Are Likely Half as Massive as Previous Estimates Suggested

July 12, 2010 — Physicists have long known that neutrinos are among the lightest and most evasive fundamental particles. Now a survey of the galaxies is helping to narrow down the neutrino mass even further. It seems that neutrinos are at best half as massive as previously estimated, according to an analysis appearing July 12 in the journal Physical Review Letters.


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The lower neutrino mass estimate is the result of a 3-dimensional survey of more than 700,000 galaxies called MegaZ DR7. Although neutrinos are very light and interact with matter very rarely, they are so numerous that they can have a significant effect on the evolution of the material distribution in the universe. The galactic distributions revealed in the MegaZ map appear consistent with a reduced upper limit of neutrino mass estimates.

There are restrictions on the information the map can provide, in part because there are three varieties of neutrinos (electron, muon, and tau neutrinos), each of which likely have different masses. As a result, MegaZ can only estimate the sum of the three neutrino masses. The galactic distribution suggests that the combined mass the three neutrino varieties is less than 0.28 electron volts. Although the survey doesn't offer a lower limit of neutrino masses, it's clear from the detection of neutrinos coming from our sun, as well as from laboratory experiments, that neutrinos have at least some mass.

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The above story is reprinted from materials provided by American Physical Society, via EurekAlert!, a service of AAAS.

Note: Materials may be edited for content and length. For further information, please contact the source cited above.


Journal References:

  1. Shaun A. Thomas, Filipe B. Abdalla, and Ofer Lahav. Upper Bound of 0.28 eV on Neutrino Masses from the Largest Photometric Redshift Survey. Physical Review Letters, 105, 031301 DOI: 10.1103/PhysRevLett.105.031301
  2. Julien Lesgourgues. Galaxies weigh in on neutrinos. Physics, 3, 57 (2010) DOI: 10.1103/Physics.3.57
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