2013年4月8日星期一

Dark Matter Mystery Explained: A Reader's Guide (Infographic)

Find out about what is known about the mysterious dark matter that fills the universe in this SPACE.com Infographic.
Source SPACE.com: All about our solar system, outer space and exploration


Most of the universe is made up of dark energy, a mysterious force that drives the accelerating expansion of the universe. The next largest ingredient is dark matter, which only interacts with the rest of the universe through its gravity. Normal matter, including all the visible stars, planets and galaxies, makes up less than 5 percent of the total mass of the universe.

Astronomers cannot see dark matter directly, but can study its effects. They can see light bent from the gravity of invisible objects (called gravitational lensing). They can also measure that stars are orbiting around in their galaxies faster than they should be.

This can all be accounted for if there were a large amount of invisible matter tied up in each galaxy, contributing to its overall mass and rotation rate.

Astronomers know more about what dark matter is not than what it is.

Dark matter is dark: It emits no light and cannot be seen directly, so it cannot be stars or planets.

Dark matter is not clouds of normal matter: Normal matter particles are called baryons. If dark matter were composed of baryons it would be detectable through reflected light. [Gallery: Dark Matter Throughout the Universe]

Dark matter is not antimatter: Antimatter annihilates matter on contact, producing gamma rays. Astronomers do not detect them.

Dark matter is not black holes: Black holes are gravity lenses that bend light. Astronomers do not see enough lensing events to account for the amount of dark matter that must exist.

Structure in the universe formed on the smallest scales first. It is believed that dark matter condensed first to form a “scaffolding,” with normal matter in the form of galaxies and clusters following the dark matter concentrations.

Scientists are using a variety of techniques across the disciplines of astronomy and physics to hunt for dark matter:
  • Particle colliders such as the Large Hadron Collider.
  • Cosmology instruments such as WMAP and Planck.
  • Direct detection experiments including CDMS, XENON, Zeplin, WARP, ArDM and others.
  • Indirect detection experiments including: Gamma ray detectors (Fermi from space and Cherenkov Telescopes from the ground); neutrino telescopes (IceCube, Antares); antimatter detectors (Pamela, AMS-02) and X-ray and radio facilities.
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暗物质

维基百科,自由的百科全书
宇宙学中,暗物质(dark matter)又稱為暗质,是指無法通過电磁波的觀測
進行研究,也就是不與电磁力產生作用的物质。人们目前只能通过重力产生的
效应得知,而且已經發现宇宙中有大量暗物质的存在。
现代天文学通过重力透镜、宇宙中大尺度结构的形成、微波背景辐射等研究表明:
我们目前所认知的部分,即重子(加上電子),大致占宇宙的4%,而暗物质則占了
宇宙的23%,还有73%是一种导致宇宙加速膨胀的暗能量。暗物质的存在可以解决
大爆炸理论中的不自洽性,对结构形成也非常关键。暗物质很有可能是一种
(或几种)粒子物理标准模型以外的新粒子所構成。
对暗物质(和暗能量)的研究是现代宇宙学粒子物理的重要课题。

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