BBC Focus

(Marcin) #1
Brian Clegggisaprolificsciencewriter.Hismost
recent book isHowManyMoons Does The Earth
Have??(£6.99, Icon Books).

BuyWondersOfTheUniverse,
presented byBrianCox,for£4.99
intheBBCStoreatstore.bbc.com

DISCOVER MORE

BELOW:Dark
energy, as
visualised
here, is
causing the
Universe’s
expansion to
accelerate

1


THERE WILL BE
COSMIC DEATH
The Universe as we know it
can’t last forever. It’s not
just that stars will burn out


  • the whole cosmos is
    running down at the same
    time a s it expands f a ster
    and faster. Eventually,
    billions of years in the
    future, we expect our
    Universe to come to an end.


2


THERE ARE
ALTERNATIVE
ENDINGS
Exactly how the Universe
will end isn’t clear. However,
most cosmologists think
that the expansion of the
Universe will continue to
accelerate, ending up with
everything ripping apart.

3


THERE ARE
KNOWN
UNKNOWNS
As yet we still don’t
understand two
fundamental components
of the Universe: dark matter,
which makes up over 80 per
cent of the mass of the
Universe, and dark energy,
which drives the
accelerating expansion.
Until we do, which will
require us to combine our
understanding of gravity
and quantum theory, this
will all remain speculation.

IN A NUTSHELL

NEXT MONTH: HOW DO
WE KNOW WHAT MATTER
IS MADE OF?

Albert Einstein
establishedthe
relationship
between matter,
gravity, space and
time, allowing us
to crudelymodel
the Universe

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IEN


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O LIBRARY X


2


developedhis GeneralTheory of
Relativity, scientists have made simple
mathematical models of the Universe
and how it could developwith time.
Over the years, these have become
more and more sophisticated. But in
theendthemodels remainfar simpler
than thething they’re modelling. Bear
in mind that we can’t even predict the
weather more than afewdays ahead.
Modelling the behaviour of the whole
Universe for billions of years to come
isfarmoreofachallenge,especially
when we don’t understand what dark
energyis,northenatureofthe‘dark
matter’ that seems to makeupfar more
of the Universe than ordinary matter.

Could anything survive the end
ofthe universe?
In the favoured scenarios where
everything either runs down or splits
apart, it’shardto seehow this would
be possible. In a bounce, though, in
principlesomethinggcould survive,
thoughitismorelikelytobe
fundamentalproperties suchas the
laws of nature than anything with
structurelikealivingbeing.

Will another universe be born
after ours dies?
Ifeither theBigCrunchor Big Bounce
happens, definitely. However, even the
morelikelyever-expanding options
don’t mean the end of everything.
Most cosmologists believe that our
Universe is one of many in a larger
‘multiverse’, with Big Bangs
happening regularly. So even ifour
Universecomestoanend,thelarger
multiverse wouldcarry onforever. It’s
the universal circleoflife.

energy into themixandthe
acceleration could go on forever.

How is dark energy created?
‘Darkenergy’isjustalabel,andthere
are severalpossibleexplanations
foritsexistence.Itmightbea
fundamentalproperty of empty space


  • a kind of intrinsic energy that’s
    present throughout the Universe. This
    mightcomeaboutthroughstrange
    quantum effects, with the uncertainty
    of energy levels meaning thatparticles
    are constantlypopping in and out of
    existence. Alternatively,darkenergy
    mightbeanewkindofenergyfieldor
    fundamental force, filling all of space
    buthaving the opposite effects to
    normal energy and matter. Finally, it
    mightbethat Einstein’s theory of
    gravityisincorrect,andthatanew
    theory is needed.Theperson who
    solves this mystery will be an instant
    Nobel Prize-winner.
    On the scale with which we’re
    familiar, dark energy is trivially small

  • unnoticeable. But when taking the
    Universe as a whole, so muchenergy is
    requiredtoaccelerateitsexpansion
    thatdarkenergy is estimatedto make
    upabout 68per cent of the mass/
    energy content of the Universe.
    Whatever it is,it’s the dominant
    ingredient of our cosmos.


Can wepredict the end of the universe
with computer models?
To a degree. Ever since Einstein
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