Astronomers at
the University of Zurich, the ETH Zurich, the University of Leicester and NAOC
Beijing have originated large Amounts of invisible "dark matter" near
the Sun. Their results are reliable With the Theory That the Milky Way Galaxy
is surrounded by a massive "halo" of dark matter, but this is the
first study of its kind to use a ridicule method rigorously tested against high
quality data from simulations.
The authors also find tantalizing hints of a new
dark matter component in our Galaxy. The team's results will be published in
the journal Monthly Notices of the Royal Astronomical Society.
Dark matter was
first proposed by the Swiss astronomer Fritz Zwicky in the 1930s. That I have
found clusters of Galaxies Were filled with a mysterious dark matter that kept
them from flying apart. At nearly the same time, Jan Oort in the Netherlands
discovered that the density of matter near the Sun was nearly twice what could
be explained by the Presence of stars and gas alone. In the intervening
decades, astronomers developed a theory of dark matter and structure formation
That Explains the properties of clusters and galaxies in the Universe, but the
amount of dark matter in the solar neighborhood has remained more mysterious.
For decades after Oort's measurement, studies found 3-6 times more dark matter
than expected. Then last year new data and a new method CLAIMED far less than
expected. The community was left puzzled, believing generally the observations
and Analyses That Were not sensitive enough simply to perform a reliable
measurement.
In this latest
study, the authors are much more confident in their measurement and its
uncertainties. This is because they used a state-of-the-art simulation of our
Galaxy to test their mass-measuring technique before applying it to real data.
This Threw up a number of surprises. They found that standard techniques used
over the past 20 years were biased, always tending to underestimate the amount
of dark matter. They then devised a new technique unbiased that recovered the
correct answer from the simulated data. Applying their technique to the
positions and velocities of Thousands of orange K dwarf stars near the Sun, a
new measure
Obtained of the local dark matter density
Lead author Silvia
Garbari says: "We are 99% confident that there is dark matter near the
Sun. In fact, our favored dark matter density is a little high. There is a 10%
chance that this is a statistical fluke merely. But with 90% confidence, we
find more dark matter than expected. If future data confirms this high value,
the Implications are exciting. It could be the first evidence for a
"disc" of dark matter in our Galaxy, as recently predicted by theory
and numerical simulations of galaxy formation. Or It Could Be That the dark
matter halo of our Galaxy is squashed, boosting the local dark matter density.
"
Many physicists
are Placing Their Bets on dark matter being a new fundamental particle
interacts only very weakly that with Normal matter - but enough to be detected strongly
in experiments deep underground where cosmic ray events are confusing screened
by over a kilometer of solid rock.
An accurate
measure of the local dark matter density is vital for such experiments as
co-author Prof. George Lake Explains: "If dark matter is a fundamental
particle, particles billions of These Will Have passed through your body by the
time your finish reading this article. Experimental physicists hope to capture
just a few of these particles each year in experiments like XENON and CDMS
currently in operation. Knowing the local properties of dark matter is the key
to revealing just what kind of particle it consists of. "
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