What is the universe expanding into Sajan Saini

The universe began its
cosmic life in a big bang

nearly fourteen billion
years ago,

and has been expanding
ever since.

But what is it expanding into?

That’s a complicated question.

Here’s why:

Einstein’s equations of
general relativity

describe space and time
as a kind of inter-connected

fabric for the universe.

This means that what we know of
as space and time

exist only as part of the universe
and not beyond it.

Now, when everyday objects
expand, they move out

into more space.

But if there is no such thing
as space to expand into,

what does expanding
even mean?

In 1929 Edwin Hubble’s
astronomy observations

gave us a definitive answer.

His survey of the night sky
found all faraway galaxies

recede, or move away,
from the Earth.

Moreover, the further the galaxy,
the faster it recedes.

How can we interpret this?

Consider a loaf of raisin bread
rising in the oven.

The batter rises by the same
amount in between each

and every raisin.

If we think of raisins as a
stand-in for galaxies,

and batter as the space
between them,

we can imagine that the
stretching or expansion

of intergalactic space will make
the galaxies recede from each other,

and for any galaxy, its faraway
neighbors will recede a larger

distance than the nearby ones

in the same amount of time.

Sure enough, the equations of
general relativity predict a cosmic

tug-of-war between gravity
and expansion.

It’s only in the dark void between
galaxies where expansion wins out,

and space stretches.

So there’s our answer.

The universe is expanding
unto itself.

That said, cosmologists are pushing
the limits of mathematical models

to speculate on what, if anything,
exists beyond our spacetime.

These aren’t wild guesses,
but hypotheses that tackle

kinks in the scientific theory
of the Big Bang.

The Big Bang predicts matter to be
distributed evenly across the universe,

as a sparse gas –but then, how
did galaxies and stars come to be?

The inflationary model
describes a brief era

of incredibly rapid expansion

that relates quantum fluctuations
in the energy of the early universe,

to the formation of clumps of gas
that eventually led to galaxies.

If we accept this paradigm, it may
also imply our universe represents

one region in a greater cosmic reality
that undergoes endless, eternal inflation.

We know nothing of this
speculative inflating reality,

save for the mathematical prediction
that its endless expansion

may be driven by an unstable
quantum energy state.

In many local regions, however,
the energy may settle by random

chance into a stable state, stopping
inflation and forming bubble universes.

Each bubble universe
—ours being one of them

—would be described by its own
Big Bang and laws of physics.

Our universe would be part
of a greater multiverse,

in which the fantastic rate of eternal
inflation makes it impossible

for us to encounter a neighbor universe.

The Big Bang also predicts that in the early,
hot universe, our fundamental forces

may unify into one super-force.

Mathematical string theories suggest
descriptions of this unification,

in addition to a fundamental structure
for sub-atomic quarks and electrons.

In these proposed models, vibrating strings
are the building blocks of the universe.

Competing models for strings have now
been consolidated into a unified description,

and suggest these structures may interact
with massive, higher dimensional surfaces called branes.

Our universe may be contained
within one such brane,

floating in an unknown higher dimensional
place, playfully named “the bulk,” or hyperspace.

Other branes—containing other types of
universes—may co-exist in hyperspace,

and neighboring branes may even share
certain fundamental forces like gravity.

Both eternal inflation and branes
describe a multiverse,

but while universes in eternal inflation are
isolated, brane universes could bump into each other.

An echo of such a collision may appear
in the cosmic microwave background

—a soup of radiation throughout our universe,
that’s a relic from an early Big Bang era.

So far, though, we’ve found
no such cosmic echo.

Some suspect these differing multiverse hypotheses
may eventually coalesce into a common description,

or be replaced by something else.

As it stands now, they’re speculative
explorations of mathematical models.

While these models are inspired and
guided by many scientific experiments,

there are very few objective experiments
to directly test them, yet.

Until the next Edwin Hubble comes along,

scientists will likely be left to argue about
the elegance of their competing models…

and continue to dream about what,
if anything, lies beyond our universe.

宇宙在近 140 亿年前的一次大爆炸中开始了它的宇宙生命

并从那时起一直在膨胀

但它扩展成什么?

这是一个复杂的问题。

原因如下:

爱因斯坦的广义相对论方程

将空间和时间描述
为宇宙的一种相互关联的

结构。

这意味着我们所知道
的空间和时间

仅作为宇宙的一部分而存在,
而不是超越它。

现在,当日常物品
扩展时,它们会

移出更多空间。

但是,如果没有
空间可以扩展,

那么
扩展意味着什么呢?

1929 年,埃德温·哈勃的
天文学观测

给了我们一个明确的答案。

他对夜空的调查
发现,所有遥远的星系都在

远离地球。

此外,星系
越远,它后退的速度就越快。

我们如何解释这一点?

考虑一条
在烤箱中升起的葡萄干面包。

面糊
在每个葡萄干之间上升相同的量

如果我们把葡萄干想象
成星系的替身,

把面糊想象成
它们之间的空间,

我们可以想象星系间空间的
拉伸或膨胀

会使星系彼此后退

,对于任何一个星系来说,它遥远的
邻居都会 在相同的时间内后退

比附近的距离更大的距离

果然,
广义相对论方程预测了

引力
和膨胀之间的宇宙拉锯战。

只有在星系之间的黑暗虚空中
,扩张胜出

,空间延伸。

所以这就是我们的答案。

宇宙正在
向自身膨胀。

也就是说,宇宙学家正在推动
数学模型的极限,

以推测在
我们的时空之外存在什么,如果有的话。

这些不是疯狂的
猜测,而是解决

大爆炸科学理论中的扭结的假设。

大爆炸预言物质会以稀薄的气体
均匀分布在整个宇宙中——但是,

星系和恒星是如何形成的呢?

暴胀模型
描述了一个

令人难以置信的快速膨胀的短暂时代,

它将
早期宇宙能量中的量子涨落与最终导致星系

的气体团块的形成联系起来

如果我们接受这个范式,它也可能
意味着我们的宇宙代表

了一个更大的宇宙现实中的一个区域,
它经历着无尽的、永恒的膨胀。

我们对这种
推测性的膨胀现实一无所知,

除了数学
预测它的无限膨胀

可能是由不稳定的
量子能态驱动的。

然而,在许多局部地区,
能量可能会

随机进入稳定状态,阻止
暴胀并形成气泡宇宙。

每个泡泡宇宙——
我们就是其中之一

——都将由它自己的
大爆炸和物理定律来描述。

我们的宇宙将
是一个更大的多元宇宙的一部分,在这个宇宙中,

永恒膨胀的惊人速度

使我们不可能遇到邻近的宇宙。

大爆炸还预测,在早期
炽热的宇宙中,我们的基本力量

可能会统一为一种超级力量。 除了亚原子夸克和电子的基本结构之外,

数学弦理论还提出了
对这种统一的描述

在这些提出的模型中,振动弦
是宇宙的基石。

弦的竞争模型现在
已被整合为一个统一的描述,

并表明这些结构可能
与称为膜的大量、更高维度的表面相互作用。

我们的宇宙可能包含
在一个这样的膜中,

漂浮在一个未知的更高维度的
地方,被戏称为“大块”或超空间。

包含其他类型宇宙的其他膜
可能共存于超空间中

,相邻的膜甚至可能共享
某些基本力,如重力。

永恒暴胀和膜都
描述了一个多元

宇宙,但虽然永恒暴胀中的
宇宙是孤立的,但膜宇宙可能会相互碰撞。

这种碰撞的回声可能会出现
在宇宙微波背景中

——整个宇宙的辐射汤,
这是大爆炸早期的遗迹。

不过,到目前为止,我们还
没有发现这样的宇宙回声。

一些人怀疑这些不同的多元宇宙假设
最终可能会合并成一个共同的描述,

或者被其他东西所取代。

就目前而言,它们是
对数学模型的推测性探索。

虽然这些模型
受到许多科学实验的启发和指导,

但很少有客观的实验
可以直接测试它们。

直到下一个埃德温·哈勃出现之前,

科学家们可能会争论
他们竞争模型的优雅……

并继续梦想
在我们的宇宙之外有什么,如果有的话。