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参考消息

【媒库文选】最精妙理论也难解释“暗物质”

2018-10-24 14:10:02 来源:参考消息网 责任编辑:王露露

核心提示:或许我们对界定宇宙最微小粒子如何起作用和相互作用的标准模型中某些东西的理解是错误的,暗物质的确存在,不过是以截然不同于我们预期的方式存在。

What Is Dark Matter?

Even the Best Theories Are Crumbling

最精妙理论也难解释“暗物质”

Korey Haynes 科丽·海恩斯

Dark matter research is unsettling. Scientists were unnerved when they first noticed that galaxies don't rotate by the same physics as a spinning plate. The stars at a galaxy's edge rotate faster than expected. And their motion can only be explained by a lot of invisible matter that we can't see.

That was exciting more than unsettling when the field was new and ideas were plentiful and had yet to be proven wrong. Researchers consolidated the possibilities into two main camps, complete with clever acronyms: MACHOs (Massive Compact Halo Objects) and WIMPs (Weakly Interacting Massive Particles).

MACHOs are the less exotic possibility. You and I don't glow or reflect light terribly well, so it's perfectly reasonable to suggest that space and galaxies contain lots of stuff that we simply can't see because they are literally dark and we don't have a big enough flashlight.

Except we can detect some of those objects out there because they're so massive that they bend light around them. They do exist, and we know they're there despite their darkness. And yet there's just not enough of them to make the galaxy-rotation math work.

So the astrophysics community mostly moved on to WIMPs. Rather than big objects, maybe the universe is full of little things we can't see. These would be swarms of objects like atoms that just don't reflect or absorb light or any other kind of electromagnetic energy, unlike all the matter we can touch and measure and see around us on Earth. We do know that neutrinos exist: tiny, mostly mass-less particles that barely interact with the universe around them. The problem there is that they're mostly mass-less. We can't figure out how there are enough of them to make up the 84 percent of the universe's matter that we can't see.

So maybe dark matter is a different object we haven't observed at all yet, something called a neutralino.

But we've been looking for them for a while. We've built incredibly sensitive, bizarre instruments to look for them. It includes the Large Hadron Collider, one of the most expensive science experiments ever built. And we haven't found them. We haven't found the WIMPs themselves, and we haven't found convincing evidence that they exist.

For decades, a few rogue scientists have stood hopefully at the edge of respectability, offering their theory called Modified Newtonian Dynamics, or MOND. Essentially, it says that physics doesn't work as we know it at the largest scales. It says we've been drawing the wrong conclusions, and dark matter isn't required to explain the universe. No one has managed to develop a theory of MOND that adequately explains the universe around us, but it occasionally gains converts simply because the competing theory of dark matter has a glaring flaw: we can't find it.

Perhaps we're wrong about something in the standard model that defines how the tiniest particles in the universe behave and interact, and dark matter exists, but in a very different form than we're expecting. Or perhaps we are wrong about the laws of gravity.

Or perhaps, maybe even tomorrow, an experiment will turn up a neutralino exactly where researchers say it should be. The LHC team will discover a new particle. Science is hard, and seen against the long story of scientific progress, we only started looking for dark matter yesterday. Until something changes, well have to rest uneasy with the unsettling possibility that physics as we know it might be very wrong.

暗物质研究让人不安。科学家首次发现星系不是按照与转盘相同的物理特性转动时,他们感到不知所措。处于星系边缘的恒星的旋转速度高于预期。而它们的运动只能用许多我们看不见的隐形物质来解释。

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