What is the universe expanding into? - Sajan Saini

1,790,738 views ・ 2018-09-06

TED-Ed


Please double-click on the English subtitles below to play the video.

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The universe began its cosmic life in a big bang
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nearly fourteen billion years ago,
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and has been expanding ever since.
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But what is it expanding into?
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That's a complicated question.
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Here's why:
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Einstein's equations of general relativity
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describe space and time as a kind of inter-connected
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fabric for the universe.
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This means that what we know of as space and time
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exist only as part of the universe and not beyond it.
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Now, when everyday objects expand, they move out
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into more space.
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But if there is no such thing as space to expand into,
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what does expanding even mean?
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In 1929 Edwin Hubble's astronomy observations
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gave us a definitive answer.
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His survey of the night sky found all faraway galaxies
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recede, or move away, from the Earth.
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Moreover, the further the galaxy, the faster it recedes.
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How can we interpret this?
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Consider a loaf of raisin bread rising in the oven.
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The batter rises by the same amount in between each
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and every raisin.
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If we think of raisins as a stand-in for galaxies,
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and batter as the space between them,
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we can imagine that the stretching or expansion
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of intergalactic space will make the galaxies recede from each other,
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and for any galaxy, its faraway neighbors will recede a larger
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distance than the nearby ones
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in the same amount of time.
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Sure enough, the equations of general relativity predict a cosmic
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tug-of-war between gravity and expansion.
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It's only in the dark void between galaxies where expansion wins out,
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and space stretches.
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So there's our answer.
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The universe is expanding unto itself.
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That said, cosmologists are pushing the limits of mathematical models
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to speculate on what, if anything, exists beyond our spacetime.
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These aren't wild guesses, but hypotheses that tackle
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kinks in the scientific theory of the Big Bang.
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The Big Bang predicts matter to be distributed evenly across the universe,
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as a sparse gas --but then, how did galaxies and stars come to be?
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The inflationary model describes a brief era
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of incredibly rapid expansion
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that relates quantum fluctuations in the energy of the early universe,
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to the formation of clumps of gas that eventually led to galaxies.
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If we accept this paradigm, it may also imply our universe represents
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one region in a greater cosmic reality that undergoes endless, eternal inflation.
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We know nothing of this speculative inflating reality,
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save for the mathematical prediction that its endless expansion
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may be driven by an unstable quantum energy state.
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In many local regions, however, the energy may settle by random
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chance into a stable state, stopping inflation and forming bubble universes.
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Each bubble universe —ours being one of them
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—would be described by its own Big Bang and laws of physics.
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Our universe would be part of a greater multiverse,
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in which the fantastic rate of eternal inflation makes it impossible
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for us to encounter a neighbor universe.
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The Big Bang also predicts that in the early, hot universe, our fundamental forces
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may unify into one super-force.
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Mathematical string theories suggest descriptions of this unification,
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in addition to a fundamental structure for sub-atomic quarks and electrons.
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In these proposed models, vibrating strings are the building blocks of the universe.
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Competing models for strings have now been consolidated into a unified description,
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and suggest these structures may interact with massive, higher dimensional surfaces called branes.
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Our universe may be contained within one such brane,
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floating in an unknown higher dimensional place, playfully named “the bulk,” or hyperspace.
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Other branes—containing other types of universes—may co-exist in hyperspace,
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and neighboring branes may even share certain fundamental forces like gravity.
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Both eternal inflation and branes describe a multiverse,
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but while universes in eternal inflation are isolated, brane universes could bump into each other.
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An echo of such a collision may appear in the cosmic microwave background
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—a soup of radiation throughout our universe, that’s a relic from an early Big Bang era.
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So far, though, we’ve found no such cosmic echo.
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Some suspect these differing multiverse hypotheses may eventually coalesce into a common description,
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or be replaced by something else.
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As it stands now, they’re speculative explorations of mathematical models.
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While these models are inspired and guided by many scientific experiments,
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there are very few objective experiments to directly test them, yet.
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Until the next Edwin Hubble comes along,
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scientists will likely be left to argue about the elegance of their competing models…
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and continue to dream about what, if anything, lies beyond our universe.
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