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"Detectable"? Purely in theory. In reality, it took 12 years to even develop a concept for detection, and a total 26 years to get the result. If you expect the exact method of detection with your next morning coffee, look who's been infantile.
You would do well to at least read the Wikipedia article, otherwise you look quite silly.
However, all you are saying is that scientists can't envision a way to detect their current model of dark matter.
Or, perhaps, through the use of gravitation, as I indicated in the above post, because hypothetical dark matter DOES interact gravitationally with normal matter.
Nor does it mean that something like dark matter DOES exist, but in a different model than what they are currently proposing. Perhaps a future model for dark matter will allow for some highly limited manner of detection.
Originally posted by Maddogkull
reply to post by Ionized
The thing I do not understand is the CMB. Doesn't that show that the earth is 14 billion years old?
Originally posted by Maddogkull
reply to post by sirnex
Sorry I did not mean earth, I meant universe
Originally posted by Maddogkull
could you elaborate on, a vaster structure of the universe? Why would the CMB only show a certain section of the universe? Isn't it probable it would show the whole.
could you elaborate on, a vaster structure of the universe? Why would the CMB only show a certain section of the universe? Isen't it probable it would show the whole.
Originally posted by sirnex
You would do well to at least read the Wikipedia article, otherwise you look quite silly.
Yea, it says it can only be detected gravitationally.
Direct detection experiments
Direct detection experiments operate in deep underground laboratories to reduce the background from cosmic rays. These include: the Soudan mine; the SNOLAB underground laboratory at Sudbury, Ontario (Canada); the Gran Sasso National Laboratory (Italy); the Boulby Underground Laboratory (UK); and the Deep Underground Science and Engineering Laboratory, South Dakota.
The majority of present experiments use one of two detector technologies: cryogenic detectors, operating at temperatures below 100mK, detect the heat produced when a particle hits an atom in a crystal absorber such as germanium. Noble liquid detectors detect the flash of scintillation light produced by a particle collision in liquid xenon or argon. Cryogenic detector experiments include: the Cryogenic Dark Matter Search (CDMS), CRESST, EDELWEISS, and EURECA. Noble liquid experiments include ZEPLIN, XENON, DEAP, ArDM, WARP and LUX. Both of these detectors are capable of distinguishing background particles which scatter off electrons, from dark matter particles which scatter off nuclei.
The DAMA/NaI, DAMA/LIBRA experiments have detected an annual modulation in the event rate, which they claim is due to dark matter particles. (As the Earth orbits the Sun, the velocity of the detector relative to the dark matter halo will vary by a small amount depending on the time of year). This claim is so far unconfirmed and difficult to reconcile with the negative results of other experiments assuming that the WIMP scenario is correct.[52]
Other direct dark matter experiments include DRIFT, MIMAC, PICASSO, and the '___'PC.
On 17 December 2009 CDMS researchers reported two possible WIMP candidate events. They estimate that the probability that these events are due to a known background (neutrons or misidentified beta or gamma events) is 23%, and conclude "this analysis cannot be interpreted as significant evidence for WIMP interactions, but we cannot reject either event as signal."[53]
False. You didn't bother to read and yes, you do look silly
The vast majority of the dark matter in the universe is believed to be nonbaryonic, which means that it contains no atoms and does not interact with ordinary matter via electromagnetic forces. The nonbaryonic dark matter includes neutrinos, and possibly hypothetical entities such as axions, or supersymmetric particles. Unlike baryonic dark matter, nonbaryonic dark matter does not contribute to the formation of the elements in the early universe ("big bang nucleosynthesis") and so its presence is revealed only via its gravitational attraction. In addition, if the particles of which it is composed are supersymmetric, they can undergo annihilation interactions with themselves resulting in observable by-products such as photons and neutrinos ("indirect detection").
Originally posted by Paschar0
Theories are are a wonderful demonstration of creative thinking. Every so often they're supported by tangible evidence. Even when they're proven wrong they've served a purpose in challenging others to think in new ways.
Originally posted by sirnex
The vast majority of the dark matter in the universe is believed to be nonbaryonic, which means that it contains no atoms and does not interact with ordinary matter via electromagnetic forces. The nonbaryonic dark matter includes neutrinos, and possibly hypothetical entities such as axions, or supersymmetric particles. Unlike baryonic dark matter, nonbaryonic dark matter does not contribute to the formation of the elements in the early universe ("big bang nucleosynthesis") and so its presence is revealed only via its gravitational attraction. In addition, if the particles of which it is composed are supersymmetric, they can undergo annihilation interactions with themselves resulting in observable by-products such as photons and neutrinos ("indirect detection").