Why is our universe fine-tuned for life? | Brian Greene

4,583,811 views ・ 2012-04-23

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Translator: Jenny Zurawell
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翻译人员: Zhixue Su 校对人员: Yuguo Zhang
00:15
A few months ago
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几个月以前,
00:17
the Nobel Prize in physics
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诺贝尔物理学奖
00:19
was awarded to two teams of astronomers
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颁发给两个天文学家团队,
00:21
for a discovery that has been hailed
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他们的发现被誉为
00:24
as one of the most important
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史上最重要的
00:26
astronomical observations ever.
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天文观测之一。
00:28
And today, after briefly describing what they found,
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今天呢,在简要描述他们的发现之后,
00:30
I'm going to tell you about a highly controversial framework
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我会告诉你一个颇有争议的理论框架
00:33
for explaining their discovery,
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用于解释他们的发现,
00:36
namely the possibility
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这种框架大大超越了
00:38
that way beyond the Earth,
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我们所认知的地球,
00:40
the Milky Way and other distant galaxies,
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银河系和其他遥远星系,
00:43
we may find that our universe
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我们可能会发现我们的宇宙
00:45
is not the only universe,
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不是唯一的宇宙,
00:47
but is instead
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相反只是
00:49
part of a vast complex of universes
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一个庞大复合宇宙的一部分,
00:51
that we call the multiverse.
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我们称之为多元宇宙。
00:53
Now the idea of a multiverse is a strange one.
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多元宇宙是个很怪的想法。
00:56
I mean, most of us were raised to believe
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我是说,大部分人从出生就被教育相信
00:58
that the word "universe" means everything.
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“宇宙”这个词包含一切。
01:01
And I say most of us with forethought,
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我是说我们中的绝大多数(都被从小教导有关“一元宇宙”的概念)
01:04
as my four-year-old daughter has heard me speak of these ideas since she was born.
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就像我四岁大的女儿从一出生就在听我讲这些想法(多元宇宙)一样。
01:07
And last year I was holding her
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去年,我抱着她,
01:09
and I said, "Sophia,
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对她说,“索非亚,
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I love you more than anything in the universe."
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我爱你胜过宇宙的一切。”
01:14
And she turned to me and said, "Daddy,
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她转过来对我说,“爸爸,
01:16
universe or multiverse?"
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是宇宙还是多元宇宙?”
01:18
(Laughter)
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(笑)
01:21
But barring such an anomalous upbringing,
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但是除了这样一个不同寻常的教育的例子,
01:24
it is strange to imagine
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我们总是很难让人们(从小接受了一元宇宙观点的人)去想象
01:26
other realms separate from ours,
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哪些其他与我们的宇宙所分离的国度(宇宙),
01:28
most with fundamentally different features,
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而其中的大部分又拥有完全不同于我们所处宇宙的特征,
01:30
that would rightly be called universes of their own.
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而这些宇宙可以被称作他们自己的宇宙。
01:33
And yet,
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尽管
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speculative though the idea surely is,
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这个想法是个推理,
01:37
I aim to convince you
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我想让你相信
01:39
that there's reason for taking it seriously,
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我们有理由把它当回事,
01:41
as it just might be right.
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因为它有可能是正确的。
01:43
I'm going to tell the story of the multiverse in three parts.
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我会分三部分来讲多元宇宙的故事。
01:46
In part one,
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第一部分,
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I'm going to describe those Nobel Prize-winning results
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我会描述这些获诺贝尔奖的结果,
01:50
and to highlight a profound mystery
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并且强调这些成绩
01:52
which those results revealed.
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揭示的一个意义深远的奥秘。
01:54
In part two,
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第二部分,
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I'll offer a solution to that mystery.
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我会解开这个奥秘。
01:58
It's based on an approach called string theory,
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它基于一种叫“弦理论”的方法,
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and that's where the idea of the multiverse
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通过它我们把多元宇宙
02:02
will come into the story.
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引入了这个故事。
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Finally, in part three,
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最后第三部分,
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I'm going to describe a cosmological theory
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我将讲述一个宇宙理论
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called inflation,
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叫暴涨,
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which will pull all the pieces of the story together.
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通过这个你就能把整个故事完整起来。
02:13
Okay, part one starts back in 1929
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好吧,故事的第一部分回到1929年,
02:17
when the great astronomer Edwin Hubble
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当伟大的天文学家爱德温•哈勃
02:19
realized that the distant galaxies
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意识到,遥远的星系
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were all rushing away from us,
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都匆匆离我们而去
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establishing that space itself is stretching,
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建立属于它自身的空间
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it's expanding.
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这个空间在不断地扩展。
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Now this was revolutionary.
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现在我们要讨论的问题开始富有革命性了。
02:31
The prevailing wisdom was that on the largest of scales
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普遍的观点是在最大的尺度下
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the universe was static.
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宇宙是静态的。
02:36
But even so,
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但即便如此,
02:38
there was one thing that everyone was certain of:
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有一件事大家都是确定的,
02:41
The expansion must be slowing down.
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就是扩张必须放缓。
02:44
That, much as the gravitational pull of the Earth
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就像万有引力
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slows the ascent of an apple tossed upward,
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减慢了抛向空中的苹果上升的速度,
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the gravitational pull
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每个星系
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of each galaxy on every other
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对其他星系的万有引力
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must be slowing
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必须减缓
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the expansion of space.
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空间的扩展。
02:58
Now let's fast-forward to the 1990s
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现在让我们快进到二十世纪90年代,
03:01
when those two teams of astronomers
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我开始提到的
03:03
I mentioned at the outset
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那两个天文学家小组
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were inspired by this reasoning
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受到这个推理的启发
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to measure the rate
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来测量
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at which the expansion has been slowing.
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这种扩张放缓的速率。
03:11
And they did this
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他们辛勤地
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by painstaking observations
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观察了
03:15
of numerous distant galaxies,
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为数众多的遥远星系,
03:17
allowing them to chart
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并据此画出了
03:19
how the expansion rate has changed over time.
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膨胀率随时间变化的图表。
03:22
Here's the surprise:
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令人惊讶的是,
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They found that the expansion is not slowing down.
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他们发现扩张并没有减速。
03:28
Instead they found that it's speeding up,
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相反速度在加快,
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going faster and faster.
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越来越快。
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That's like tossing an apple upward
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就像抛一个苹果,
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and it goes up faster and faster.
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它快速地上升。
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Now if you saw an apple do that,
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如果你看到一个苹果这样的话,
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you'd want to know why.
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你一定想知道为什么。
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What's pushing on it?
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是一种什么力量推动它呢?
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Similarly, the astronomers' results
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同样,天文学家的结果
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are surely well-deserving of the Nobel Prize,
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肯定配得诺贝尔奖,
03:47
but they raised an analogous question.
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但他们提了一个类似的问题。
03:51
What force is driving all galaxies
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是什么力量驱动所有的星系
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to rush away from every other
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不断加速地
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at an ever-quickening speed?
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远离其它的呢?
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Well the most promising answer
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最有希望的答案
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comes from an old idea of Einstein's.
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还是来自爱因斯坦的老观点。
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You see, we are all used to gravity
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你看,我们都习惯于认为,
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being a force that does one thing,
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地心引力这种力量就做一件事,
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pulls objects together.
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就是把东西拉在一起。
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But in Einstein's theory of gravity,
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但在爱因斯坦的引力理论中,
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his general theory of relativity,
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他的广义相对论,
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gravity can also push things apart.
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引力也可以把东西推开的。
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How? Well according to Einstein's math,
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怎么说呢?根据爱因斯坦的数学,
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if space is uniformly filled
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如果空间是
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with an invisible energy,
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被无形的能量均匀地充满,
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sort of like a uniform, invisible mist,
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就像一种统一,无形的雾,
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then the gravity generated by that mist
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这种雾所产生的重力
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would be repulsive,
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会是
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repulsive gravity,
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排斥重力,
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which is just what we need to explain the observations.
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这正是我们需要解释的观测。
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Because the repulsive gravity
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因为空间中的
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of an invisible energy in space --
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这种无形能量的排斥重力--
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we now call it dark energy,
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我们把它叫做暗能量,
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but I've made it smokey white here so you can see it --
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但这里我把它用白色烟雾表示是为了便于看到--
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its repulsive gravity
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它的排斥重力
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would cause each galaxy to push against every other,
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会导致每个星系互相推斥,
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driving expansion to speed up,
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驱使扩张加快
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not slow down.
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而不是减缓。
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And this explanation
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这个解释
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represents great progress.
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代表着很大的进步。
04:59
But I promised you a mystery
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我答应过你这是
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here in part one.
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第一部分的一个谜。
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Here it is.
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这个就是。
05:06
When the astronomers worked out
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在天文学家计算出
05:08
how much of this dark energy
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必须注入多少暗能量
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must be infusing space
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到空间
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to account for the cosmic speed up,
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去证明宇宙的加速时,
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look at what they found.
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看看他们发现了什么。
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This number is small.
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这是个小数目。
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Expressed in the relevant unit,
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用相关的单位来表现,
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it is spectacularly small.
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它非常小。
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And the mystery is to explain this peculiar number.
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谜团是去解释这个奇特的数字。
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We want this number
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我们希望这一数字
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to emerge from the laws of physics,
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可能摆脱物理定律,
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but so far no one has found a way to do that.
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但到目前为止还没有人找到一个方法。
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Now you might wonder,
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你现在可能想知道,
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should you care?
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你应该担忧吗?
05:45
Maybe explaining this number
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也许解释这个数字
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is just a technical issue,
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只是个技术问题,
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a technical detail of interest to experts,
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一个专家感兴趣的技术细节,
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but of no relevance to anybody else.
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根别人没什么关系。
05:54
Well it surely is a technical detail,
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这的确是一个技术上的细节,
05:57
but some details really matter.
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但有些细节至关重大。
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Some details provide
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一些细节
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windows into uncharted realms of reality,
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给未知的现实领域提供窗口,
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and this peculiar number may be doing just that,
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这个奇特的数字可能只有这个用途,
06:06
as the only approach that's so far made headway to explain it
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至今为止作为唯一方法取得了进展,
06:09
invokes the possibility of other universes --
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去解释它调用奇特宇宙的可能性--
06:12
an idea that naturally emerges from string theory,
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这个想法自然地脱离弦理论,
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which takes me to part two: string theory.
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带我进入第二部分:弦理论。
06:18
So hold the mystery of the dark energy
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先把暗能量的谜团
06:22
in the back of your mind
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放在脑后,
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as I now go on to tell you
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我继续讲
06:26
three key things about string theory.
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有关弦理论的三个关键的事情。
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First off, what is it?
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第一个,是什么呢?
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Well it's an approach to realize Einstein's dream
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那是实践爱因斯坦的物理统一理论的
06:34
of a unified theory of physics,
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梦想的一种途径,
06:37
a single overarching framework
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一个总体框架
06:39
that would be able to describe
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能够描述
06:41
all the forces at work in the universe.
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宇宙所有的力量在起作用。
06:43
And the central idea of string theory
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而弦理论的中心思想
06:45
is quite straightforward.
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非常简单。
06:47
It says that if you examine
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它说,如果你非常细致地检查
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any piece of matter ever more finely,
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任何一样物质。
06:51
at first you'll find molecules
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起初你会发现分子,
06:53
and then you'll find atoms and subatomic particles.
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然后你会发现原子和亚原子粒子。
06:56
But the theory says that if you could probe smaller,
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但这个理论说,如果你能够探测到更小的,
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much smaller than we can with existing technology,
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比我们现有技术能做到的更小的,
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you'd find something else inside these particles --
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你会在这些粒子里找到别的东西--
07:04
a little tiny vibrating filament of energy,
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一个小小的能量震动纤维,
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a little tiny vibrating string.
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一个小小的震动弦。
07:10
And just like the strings on a violin,
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就像小提琴上的弦一样,
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they can vibrate in different patterns
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它们通过不同的震动
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producing different musical notes.
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来产生不同的音符。
07:16
These little fundamental strings,
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这些小小的基本的弦,
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when they vibrate in different patterns,
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当他们以不同的模式震动时,
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they produce different kinds of particles --
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它们产生不同种类的粒子--
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so electrons, quarks, neutrinos, photons,
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所以,电子,夸克,中微子,光子,
07:24
all other particles
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所有的粒子
07:26
would be united into a single framework,
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会合并成一个单一的框架,
07:28
as they would all arise from vibrating strings.
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它们会通过震动的弦而出现。
07:31
It's a compelling picture,
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那是个令人信服的场面,
07:34
a kind of cosmic symphony,
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一种宇宙交响乐,
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where all the richness
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我们看到的
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that we see in the world around us
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从周围世界的音乐
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emerges from the music
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而展现的丰富,
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that these little, tiny strings can play.
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这些小小的弦也能演奏出。
07:45
But there's a cost
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但这种优雅的统一
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to this elegant unification,
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是有代价的,
07:49
because years of research
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因为多年的研究
07:51
have shown that the math of string theory doesn't quite work.
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表明弦理论的数学也不是行得通的。
07:54
It has internal inconsistencies,
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它内部不一致,
07:56
unless we allow
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除非我们考虑
07:58
for something wholly unfamiliar --
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完全陌生的事--
08:01
extra dimensions of space.
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即额外纬度空间。
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That is, we all know about the usual three dimensions of space.
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我们都知道通常的三维空间。
08:07
And you can think about those
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你可以用
08:09
as height, width and depth.
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高度,宽度和深度来考虑。
08:12
But string theory says that, on fantastically small scales,
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但弦理论认为,在极其小的尺度下,
08:15
there are additional dimensions
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在这么小的尺寸下
08:17
crumpled to a tiny size so small
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还有附加的维度,因为太小
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that we have not detected them.
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我们还探测不出。
08:21
But even though the dimensions are hidden,
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但即使这些维度是隐藏的,
08:23
they would have an impact on things that we can observe
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它们对一些东西的影响我们能够观察到,
08:26
because the shape of the extra dimensions
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因为额外维度的形状
08:29
constrains how the strings can vibrate.
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限制着弦的震动。
08:32
And in string theory,
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在弦理论中,
08:34
vibration determines everything.
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振动决定一切。
08:37
So particle masses, the strengths of forces,
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所以呢,粒子的质量,力量的强度,
08:39
and most importantly, the amount of dark energy
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最重要的,暗能量的总量
08:42
would be determined
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会取决于
08:44
by the shape of the extra dimensions.
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额外维度的形状。
08:46
So if we knew the shape of the extra dimensions,
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如果我们了解额外维度的形状,
08:49
we should be able to calculate these features,
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我们就能计算出这些特征,
08:52
calculate the amount of dark energy.
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计算出暗能量的总量。
08:55
The challenge
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目前的挑战是
08:57
is we don't know
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我们不知道
08:59
the shape of the extra dimensions.
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额外维度的形状。
09:02
All we have
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我们有的
09:04
is a list of candidate shapes
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是通过数学算出的
09:06
allowed by the math.
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一些候选形状。
09:09
Now when these ideas were first developed,
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当这些想法首次推出的时候,
09:11
there were only about five different candidate shapes,
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只有5个候补形状,
09:13
so you can imagine
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你可以想象到
09:15
analyzing them one-by-one
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一个一个分析它们
09:17
to determine if any yield
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来决定哪一个符合
09:19
the physical features we observe.
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我们观察的物理特征。
09:21
But over time the list grew
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可是随着时间的迁移,
09:23
as researchers found other candidate shapes.
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研究人员发现了更多的候选形状。
09:25
From five, the number grew into the hundreds and then the thousands --
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从起初的5个到几百个,最后几千个--
09:28
A large, but still manageable, collection to analyze,
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数目很多但还管得过来,
09:31
since after all,
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去分析这些的工作
09:33
graduate students need something to do.
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就交给刚毕业的学生了。
09:36
But then the list continued to grow
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但是这个数目单继续增加到了
09:38
into the millions and the billions, until today.
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几百万,到今天有数十亿了。
09:41
The list of candidate shapes
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候选形状的清单
09:43
has soared to about 10 to the 500.
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也飙升到10至500个。
09:48
So, what to do?
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那,怎么办呢?
09:51
Well some researchers lost heart,
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有些研究人员失去信心,
09:54
concluding that was so many candidate shapes for the extra dimensions,
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结论是额外维度有这么多的候选形状,
09:57
each giving rise to different physical features,
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每一个都有不同的物理特征,
10:00
string theory would never make
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弦理论永远不会做出
10:02
definitive, testable predictions.
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确定的,可检验的预测。
10:04
But others turned this issue on its head,
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但是另一些从另一个角度考虑,
10:08
taking us to the possibility of a multiverse.
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把我们带到多元宇宙的可能性。
10:10
Here's the idea.
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想法是这样的。
10:12
Maybe each of these shapes is on an equal footing with every other.
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也许这些性状之间是互相平等的。
10:15
Each is as real as every other,
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每一个都很真实,
10:17
in the sense
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就是说
10:19
that there are many universes,
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有很多的宇宙,
10:21
each with a different shape, for the extra dimensions.
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每个对额外维度都有不同的形状。
10:24
And this radical proposal
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这种激进的建议
10:26
has a profound impact on this mystery:
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对这个谜团有着深刻的影响:
10:29
the amount of dark energy revealed by the Nobel Prize-winning results.
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诺贝尔得奖结果揭示了暗能量的总量。
10:32
Because you see,
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因为你看,
10:34
if there are other universes,
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如果有很多的其他宇宙,
10:37
and if those universes
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而这些宇宙
10:39
each have, say, a different shape for the extra dimensions,
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每个都有不同的额外维度形状,
10:43
then the physical features of each universe will be different,
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那么每个宇宙的物理特征将会不同,
10:45
and in particular,
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特别是,
10:47
the amount of dark energy in each universe
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每个宇宙的暗能量
10:49
will be different.
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将会不同。
10:51
Which means that the mystery
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也就意味着,
10:53
of explaining the amount of dark energy we've now measured
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我们现在测量到的暗能量总量的解释谜呢,
10:55
would take on a wholly different character.
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将会是 一个完全不同的角色。
10:58
In this context,
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在这种背景下,
11:00
the laws of physics can't explain one number for the dark energy
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物理定律不能解释暗能量的一个数,
11:03
because there isn't just one number,
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因为不知一个数,
11:06
there are many numbers.
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有很多数。
11:08
Which means
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也意味着,
11:10
we have been asking the wrong question.
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我们一直问错了问题。
11:13
It's that the right question to ask is,
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应该问的正确问题是,
11:15
why do we humans find ourselves in a universe
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为什么我们人类在一个宇宙中测量
11:18
with a particular amount of dark energy we've measured
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一种特定量的暗能量,
11:21
instead of any of the other possibilities
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而不是在另外的
11:24
that are out there?
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其他外围宇宙呢?
11:26
And that's a question on which we can make headway.
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我们在这个问题上能取得进展。
11:29
Because those universes
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因为那些宇宙
11:31
that have much more dark energy than ours,
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有着比我们的更多的暗能量,
11:33
whenever matter tries to clump into galaxies,
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当物质要聚成星系时,
11:36
the repulsive push of the dark energy is so strong
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暗能量的排斥力太强,
11:39
that it blows the clump apart
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把物质快吹散,
11:41
and galaxies don't form.
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星系就无法形成。
11:43
And in those universes that have much less dark energy,
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这些宇宙中的暗能量较少,
11:46
well they collapse back on themselves so quickly
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它们非常快地崩溃后回来,
11:48
that, again, galaxies don't form.
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也形成不了星系。
11:51
And without galaxies, there are no stars, no planets
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没有星系,就没有星星,没有行星,
11:54
and no chance
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所以在别的宇宙中
11:56
for our form of life
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没法有
11:58
to exist in those other universes.
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像我们这样的生命存在。
12:00
So we find ourselves in a universe
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我们发现我们自己存在于
12:02
with the particular amount of dark energy we've measured
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一个我们简单测量的有一个特别数量的暗能量的宇宙中,
12:05
simply because our universe has conditions
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只因为我们的宇宙有合适的条件
12:08
hospitable to our form of life.
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供我们生命的存在。
12:12
And that would be that.
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就是那个。
12:14
Mystery solved,
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谜团破解了,
12:16
multiverse found.
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多元宇宙被发现。
12:18
Now some find this explanation unsatisfying.
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有些人对这个解释不满意。
12:23
We're used to physics
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我们习惯于物理学
12:25
giving us definitive explanations for the features we observe.
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给我们观察的特征的明确解释。
12:28
But the point is,
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但问题是,
12:30
if the feature you're observing
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如果你观察的特征
12:33
can and does take on
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能够并且确实承担
12:35
a wide variety of different values
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现实中的
12:37
across the wider landscape of reality,
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不同价值,
12:40
then thinking one explanation
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那么对一种
12:42
for a particular value
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特定值用一种解释
12:44
is simply misguided.
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就会简单地误导人。
12:47
An early example
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一个早期的例子
12:49
comes from the great astronomer Johannes Kepler
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来自于伟大的天文学家约翰 开普勒,
12:52
who was obsessed with understanding
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他很着迷于研究
12:54
a different number --
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不同的数字--
12:56
why the Sun is 93 million miles away from the Earth.
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为什么太阳离地球9千3百万英里。
13:00
And he worked for decades trying to explain this number,
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他花了几十年的时间试图解释这个数字,
13:03
but he never succeeded, and we know why.
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但从未成功,我们知道为什么。
13:06
Kepler was asking
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开普勒
13:08
the wrong question.
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问错了问题。
13:10
We now know that there are many planets
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现在我们知道有许多行星
13:13
at a wide variety of different distances from their host stars.
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距离它们的宿主恒星有不同的距离。
13:16
So hoping that the laws of physics
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单单希望物理定律
13:19
will explain one particular number, 93 million miles,
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能解释一个特殊的数据,9千3百万,
13:22
well that is simply wrongheaded.
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是执迷不悟。
13:25
Instead the right question to ask is,
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正确的问题应该是,
13:27
why do we humans find ourselves on a planet
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为什么我们人类发现我们在一个行星上的
13:30
at this particular distance,
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距离是特定的,
13:32
instead of any of the other possibilities?
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而不是别的可能呢?
13:35
And again, that's a question we can answer.
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同样,这个问题我们能回答。
13:38
Those planets which are much closer to a star like the Sun
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那些行星更接近于一颗星就像太阳
13:41
would be so hot
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一样热,
13:43
that our form of life wouldn't exist.
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以至像我们这样的生命无法存在。
13:45
And those planets that are much farther away from the star,
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而那些离这个星太远的行星,
13:48
well they're so cold
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因为太冷,
13:50
that, again, our form of life would not take hold.
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同样也没法有我们这样的生命。
13:52
So we find ourselves
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所以,我们发现我们
13:54
on a planet at this particular distance
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在这颗行星的特定距离
13:56
simply because it yields conditions
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只是因为它的条件
13:58
vital to our form of life.
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符合我们生命的存在。
14:01
And when it comes to planets and their distances,
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讲到行星和它们的距离时,
14:04
this clearly is the right kind of reasoning.
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这显然是合理的推理。
14:08
The point is,
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关键是,
14:10
when it comes to universes and the dark energy that they contain,
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讲到宇宙和他们所含的暗能量时,
14:13
it may also be the right kind of reasoning.
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它也可能是合适的推理。
14:17
One key difference, of course,
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一个重要的区别是,
14:20
is we know that there are other planets out there,
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我们知道外边还有很多别的行星,
14:22
but so far I've only speculated on the possibility
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但到目前为止,我只是推测可能
14:25
that there might be other universes.
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会有其他的宇宙。
14:27
So to pull it all together,
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把这些合起来,
14:29
we need a mechanism
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我们需要一个机制,
14:31
that can actually generate other universes.
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实际上可以生成其它宇宙。
14:34
And that takes me to my final part, part three.
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这样我就来到最后一部分,第三部分。
14:37
Because such a mechanism has been found
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因为宇宙学家们在试图了解
14:40
by cosmologists trying to understand the Big Bang.
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大爆炸时发现了这个机制。
14:43
You see, when we speak of the Big Bang,
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你看,但我们说起大爆炸时,
14:45
we often have an image
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我们常常有一个
14:47
of a kind of cosmic explosion
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宇宙爆炸的图画,
14:49
that created our universe
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这个爆炸创造了我们的宇宙,
14:51
and set space rushing outward.
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且把空间向外扩。
14:54
But there's a little secret.
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但有一个小秘密。
14:56
The Big Bang leaves out something pretty important,
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大爆炸留下了很重要的就是,
14:59
the Bang.
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爆炸。
15:01
It tells us how the universe evolved after the Bang,
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它告诉我们宇宙在爆炸后时如何进化,
15:04
but gives us no insight
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但没有给我们
15:06
into what would have powered the Bang itself.
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提供爆炸本身的力量。
15:10
And this gap was finally filled
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最终,这个差距
15:12
by an enhanced version of the Big Bang theory.
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被一个增强版的大爆炸理论填补上了
15:14
It's called inflationary cosmology,
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它被称为暴胀宇宙学,
15:17
which identified a particular kind of fuel
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找到了一种特殊的燃料,
15:21
that would naturally generate
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会自然产生
15:23
an outward rush of space.
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向往冲的空间。
15:25
The fuel is based on something called a quantum field,
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燃料基于一种叫做量子场的东西,
15:28
but the only detail that matters for us
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但对我们有关的唯一细节是
15:31
is that this fuel proves to be so efficient
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这种燃料被证明是如此高效,
15:34
that it's virtually impossible
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它几乎不可能
15:36
to use it all up,
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完全用尽,
15:38
which means in the inflationary theory,
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这就意味着在暴胀理论中,
15:40
the Big Bang giving rise to our universe
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大爆炸出现在我们宇宙
15:43
is likely not a one-time event.
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不是一次性的事件。
15:46
Instead the fuel not only generated our Big Bang,
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相反,燃料不仅产生了我们的大爆炸,
15:49
but it would also generate countless other Big Bangs,
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它也产生了无数的别的爆炸,
15:55
each giving rise to its own separate universe
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每个形成它自己的宇宙,
15:58
with our universe becoming but one bubble
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我们的宇宙变成
16:00
in a grand cosmic bubble bath of universes.
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大宇宙泡泡浴里的一个泡泡。
16:03
And now, when we meld this with string theory,
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现在,当我们把这融合到弦理论,
16:05
here's the picture we're led to.
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我们就看到了这张图片。
16:07
Each of these universes has extra dimensions.
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这些宇宙中的每一个都有额外维度。
16:09
The extra dimensions take on a wide variety of different shapes.
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额外维度有不同的形状。
16:12
The different shapes yield different physical features.
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不同的形状产生不同的物理特征。
16:15
And we find ourselves in one universe instead of another
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我们发现我们自己在一个而不是
16:18
simply because it's only in our universe
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另一个宇宙中单单因为我们的宇宙的
16:21
that the physical features, like the amount of dark energy,
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物理特征,譬如暗能量的总量
16:24
are right for our form of life to take hold.
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正好适合我们生命的存在。
16:28
And this is the compelling but highly controversial picture
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这是具有吸引力但对更广阔宇宙的
16:31
of the wider cosmos
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又极有争议的图片,
16:33
that cutting-edge observation and theory
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尖端的观察与理论
16:35
have now led us to seriously consider.
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让我们去更严肃地思考。
16:39
One big remaining question, of course, is,
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一个悬而未决的问题,当然是,
16:43
could we ever confirm
399
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我们能否确认
16:46
the existence of other universes?
400
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其他宇宙的存在?
16:49
Well let me describe
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让我来描述一种
16:51
one way that might one day happen.
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可能有一天会发生的方法。
16:54
The inflationary theory
403
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通胀理论
16:56
already has strong observational support.
404
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已经有强大的观测支持。
16:58
Because the theory predicts
405
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因为这个理论预言
17:00
that the Big Bang would have been so intense
406
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大爆炸将是如此强烈
17:02
that as space rapidly expanded,
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以至于空间快速扩张,
17:05
tiny quantum jitters from the micro world
408
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微小的量子从微观世界
17:07
would have been stretched out to the macro world,
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延伸到宏观世界,
17:10
yielding a distinctive fingerprint,
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产生一种独特的指纹,
17:13
a pattern of slightly hotter spots and slightly colder spots,
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一种既有微热和微冷的
17:15
across space,
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斑点模式
17:17
which powerful telescopes have now observed.
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已经被功能强大的望远镜观察到了。
17:20
Going further, if there are other universes,
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讲的远点,如果有其他的宇宙,
17:23
the theory predicts that every so often
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这个理论预测这些宇宙
17:25
those universes can collide.
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可能互相碰撞。
17:27
And if our universe got hit by another,
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如果我们的宇宙被别的宇宙撞上了,
17:29
that collision
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碰撞
17:31
would generate an additional subtle pattern
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会在空间里产生额外的
17:33
of temperature variations across space
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微妙的温度变化,
17:35
that we might one day
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我们可能有一天
17:37
be able to detect.
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能探测到。
17:39
And so exotic as this picture is,
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正像这张奇特的照片,
17:42
it may one day be grounded
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有一天也许会基于
17:44
in observations,
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观测,
17:46
establishing the existence of other universes.
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建立其它宇宙的存在。
17:49
I'll conclude
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最后,
17:51
with a striking implication
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我将用一个有关遥远未来的
17:54
of all these ideas
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所有想法
17:56
for the very far future.
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的令人瞩目的暗示来结束。
17:58
You see, we learned
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你看,我们得知
18:00
that our universe is not static,
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我们的宇宙不是静态的,
18:02
that space is expanding,
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空间是在扩张的,
18:04
that that expansion is speeding up
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这个扩张是在加速的,
18:06
and that there might be other universes
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可能会有别的宇宙,
18:08
all by carefully examining
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我们可以通过仔细检查
18:10
faint pinpoints of starlight
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微弱的星光
18:12
coming to us from distant galaxies.
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来确定那些遥远的星系。
18:15
But because the expansion is speeding up,
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但是因为这种扩张太快,
18:18
in the very far future,
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在遥远的未来,
18:20
those galaxies will rush away so far and so fast
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这些星系会离我们很远很远
18:23
that we won't be able to see them --
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以至我们再也看不到它们--
18:26
not because of technological limitations,
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不是因为技术的限制,
18:28
but because of the laws of physics.
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而是因为物理定律。
18:30
The light those galaxies emit,
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这些星系发出的光,。
18:32
even traveling at the fastest speed, the speed of light,
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即使以很快的速度行走,以光速行走,
18:35
will not be able to overcome
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也克服不了
18:37
the ever-widening gulf between us.
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我们之间已经扩展的鸿沟
18:40
So astronomers in the far future
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所以在将来天文学家
18:42
looking out into deep space
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遥望远空
18:44
will see nothing but an endless stretch
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除了静静的漆黑的沉寂
18:47
of static, inky, black stillness.
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什么也看不到。
18:51
And they will conclude
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他们就会下结论
18:53
that the universe is static and unchanging
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说宇宙是安静的不变的,
18:55
and populated by a single central oasis of matter
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由一个中央绿洲的居民
18:58
that they inhabit --
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占据着--
19:00
a picture of the cosmos
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这幅宇宙的图画
19:02
that we definitively know to be wrong.
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我们知道是完全错的。
19:05
Now maybe those future astronomers will have records
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或许这些未来的天文学家
19:08
handed down from an earlier era,
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会有早期时代传下来的纪录,
19:10
like ours,
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就像我们的,
19:12
attesting to an expanding cosmos
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证明有一个充满星系的
19:14
teeming with galaxies.
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膨胀的宇宙。
19:16
But would those future astronomers
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但这些未来的天文学家
19:18
believe such ancient knowledge?
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会相信这里古老的知识吗?
19:21
Or would they believe
466
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或者他们会相信
19:23
in the black, static empty universe
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他们自己最先进的观测
19:26
that their own state-of-the-art observations reveal?
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显示的这个黑色的静态的空旷的宇宙吗?
19:30
I suspect the latter.
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我怀疑后者。
19:32
Which means that we are living
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这意味着,我们正经历
19:34
through a remarkably privileged era
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一个非常特权的时代,
19:37
when certain deep truths about the cosmos
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宇宙某些深层的真理
19:39
are still within reach
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还在人类探索
19:41
of the human spirit of exploration.
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能及的范畴。
19:43
It appears that it may not always be that way.
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看来也许并不总是这样。
19:48
Because today's astronomers,
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因为当今的天文学家们,
19:50
by turning powerful telescopes to the sky,
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透过强大的望远镜,
19:53
have captured a handful of starkly informative photons --
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已经捕捉到少数可提供信息的光子--
19:56
a kind of cosmic telegram
479
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宇宙电报要走
19:59
billions of years in transit.
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10亿年的路程。
20:01
and the message echoing across the ages is clear.
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这个经历了不同的年代信息是清晰的。
20:05
Sometimes nature guards her secrets
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有时,自然通过
20:08
with the unbreakable grip
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牢不可破的物理定律
20:10
of physical law.
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来守护着她的秘密。
20:12
Sometimes the true nature of reality beckons
485
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有时现实的真实
20:16
from just beyond the horizon.
486
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在地平线那边呼唤。
20:19
Thank you very much.
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多谢!
20:21
(Applause)
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(鼓掌)
20:25
Chris Anderson: Brian, thank you.
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Chris Anderson:布赖恩,谢谢你。
20:27
The range of ideas you've just spoken about
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你刚刚谈到的这些想法的范围
20:29
are dizzying, exhilarating, incredible.
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真是令人眼花缭乱,兴奋不已,和难以置信。
20:32
How do you think
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从历史的角度来看,
20:34
of where cosmology is now,
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你认为现在的宇宙学
20:36
in a sort of historical side?
494
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走到了哪一步?
20:38
Are we in the middle of something unusual historically in your opinion?
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从你的观点来说,我们是在历史中的不寻常的一个时期吗?
20:41
BG: Well it's hard to say.
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BG:这个很难说。
20:43
When we learn that astronomers of the far future
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当我们知道将来的天文学家
20:46
may not have enough information to figure things out,
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没有足够的信息去把事情弄明白,
20:49
the natural question is, maybe we're already in that position
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很自然的问题是,也许我们已经
20:52
and certain deep, critical features of the universe
500
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在一个位置和深度,
20:55
already have escaped our ability to understand
501
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因为宇宙学的演化,
20:58
because of how cosmology evolves.
502
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宇宙的一些重要特性已经超出我们的理解能力。
21:00
So from that perspective,
503
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所以从这个角度来看,
21:02
maybe we will always be asking questions
504
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也许我们永远是问问题,
21:04
and never be able to fully answer them.
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永远无法完全解答它们。
21:06
On the other hand, we now can understand
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另一方面,现在我们能理解
21:08
how old the universe is.
507
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宇宙有多老。
21:10
We can understand
508
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我们知道
21:12
how to understand the data from the microwave background radiation
509
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如何理解137.2亿年前的
21:15
that was set down 13.72 billion years ago --
510
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微波背景辐射的数据--
21:18
and yet, we can do calculations today to predict how it will look
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我们今天可以计算并预测它将来会是什么样子,
21:20
and it matches.
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并如何与它匹配。
21:22
Holy cow! That's just amazing.
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不会吧!这太惊人了!
21:24
So on the one hand, it's just incredible where we've gotten,
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所以,一方面,我们得到的太不可思议了,
21:27
but who knows what sort of blocks we may find in the future.
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但谁知道我们将来会发现什么障碍呢?
21:31
CA: You're going to be around for the next few days.
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CA:你还要在这呆几天。
21:34
Maybe some of these conversations can continue.
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或许我们会继续讨论。
21:36
Thank you. Thank you, Brian. (BG: My pleasure.)
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谢谢!谢谢你,布莱恩。(BG:很荣幸。)
21:38
(Applause)
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(鼓掌)
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