Martin Hendry- Why are we here?

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    Dr Martin Hendry

    Dept of Physics and AstronomyUniversity of Glasgow

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    A little old lady at the back of the room

    got up and said: What you have told us is

    rubbish. The world is really a flat plate

    supported on the back of a giant tortoise.

    The scientist gave a superior smile before

    replying What is the tortoise standing on?

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    A little old lady at the back of the room

    got up and said: What you have told us is

    rubbish. The world is really a flat plate

    supported on the back of a giant tortoise.

    The scientist gave a superior smile before

    replying What is the tortoise standing on?

    Youre very clever young man, very

    clever, said the old lady. But its turtlesall the way down!

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    Science:

    The intellectual and practical activityencompassing the systematic study of the

    structure and behaviour of the physical

    and natural world through observationand experiment

    From the New Oxford dictionary

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    Bernard Carr

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    Bernard Carr

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    Bernard Carr

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    Bernard Carr

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    Two talks in one:

    Why are we here?...

    Why are we here?...

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    Why are we here?...

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    Edwin Hubble

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    Space is big. You justwon't believe how vastly,

    hugely, mind- bogglinglybig it is. I mean, you maythink it's a long way down

    the road to the chemist's,but that's just peanuts tospace.

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    HubbleHubbles Laws Law

    Distant galaxies are moving away from uswith a speed proportional to their distance

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    Spacetime is expanding like

    the surface of a balloon.

    As the balloon expands,

    galaxies are carried farther

    apart

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    How fast is the Universe expanding?

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    What is driving the cosmic acceleration?What is driving the cosmic acceleration?

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    CMBR: all-sky temperature map from WMAP satellite.

    Temperature fluctuations from

    ~380,000 years after the Big Bang

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    CMBR fluctuations, are theseeds of todays galaxies

    Galaxies and Cosmology: the Basic Paradigm

    Structure we see today was assembledby gravity, causing density fluctuations

    in the early Universe (which we see

    imprinted on the CMBR) to grow, as thebackground smooth Universe expands

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    So what exactly is

    this dark energy?...

    Einsteinscosmologicalconstant?...

    Energy of thequantum vacuum?...

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    4%

    74%

    22%

    Dark Energy

    Cold Dark

    Matter

    Atoms

    State of the Universe Apr 2008

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    4%

    74%

    22%

    State of the Universe Apr 2008

    Why does 96% of the Universe consist

    of strange matter and energy?

    CDM

    b

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    From Lineweaver (1998)

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    Why now?

    CDM

    Value of

    Present-day

    Age of theUniverse

    Big Bang

    0

    0.2

    0.4

    0.6

    0.8

    1

    0 1 2 3

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    Hydrogen fusion fuelling a stars nuclear furnace

    E = mc 2

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    Hydrogen fusion fuelling a stars nuclear furnace

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    Why are we here?...

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    Why are we (and only we)here?...

    If the Universe is so big, andso old, and so finely balanced

    to support life like us, whyare we seemingly alone?....

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    Why are we (and only we)here?...

    If the Universe is so big, andso old, and so finely balanced

    to support life like us, whyare we seemingly alone?....

    Where is everybody?Where is everybody?Enrico Fermi, 1950

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    Where is Everybody?by Stephen Webb

    Fifty solutions to the Fermi Paradoxand the problem of extraterrestrial

    life:

    o They are here

    o They exist but have not yet

    communicated

    o They do not exist

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    They are here and are meddling in Human affairsThey are here and are meddling in Human affairs

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    They exist but have not yet communicatedThey exist but have not yet communicated

    We are Solar chauvinists

    Perhaps there are simply

    too many other interesting

    places to visit?

    25000 10000 8000 6000 5000 4000 3000

    Surface temperature (K)

    O5 B0 A0 F0 G0 K0 M0 M8

    Luminosity(Sun=1)

    Spectral Type

    1

    102

    104

    106

    10-2

    10-4

    -10

    -5

    0

    +5

    +10

    +15

    AbsoluteM

    agnitude

    . . . . .

    . . ..

    .

    .

    .... ...

    .

    ................

    .......

    .......

    ......

    .... ...

    .

    ..

    . ....

    .

    ..

    .......

    ..

    ...

    ........

    .

    . ..

    ..

    ..

    .......... .

    ..

    ....RegulusVega

    Sirius A

    Altair Sun

    Sirius B

    Procyon B

    BarnardsStar

    Procyon A

    ..

    ...

    .. Aldebaran

    Mira

    Pollux

    Arcturus

    Rigel

    Deneb

    Antares

    Betelgeuse

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    They exist but have not yet communicatedThey exist but have not yet communicated

    Cloudy skies are common!

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    They exist but have not yet communicatedThey exist but have not yet communicated

    They stay at home

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    They exist but have not yet communicatedThey exist but have not yet communicated

    They stay at home

    and surf the net

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    They exist but have not yet communicatedThey exist but have not yet communicated

    They are signalling but we dont know how to listen

    The Waterhole: strong H and OH emission between1.42 GHz and 1.64 GHz

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    They do not existThey do not exist

    Perhaps emergence of Life depends on astrophysics

    o e.g. carbon-based life may

    appear only after peak in

    cosmic carbon production

    o This peak occurred ~ 7 billion

    years ago.

    o Still leaves a ~ 3 billion-year

    head start for some ETC

    o Shouldnt that give plenty of

    time to colonise the galaxy?...

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    They do not existThey do not exist

    Rocky planets are rare

    Most exoplanetsfound to date arehot Jupiters:massive planets

    close to theirparent star.

    This is largely a

    selection effect.

    K lK l

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    KeplerKepler

    Launch: Feb 2009

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    They do not existThey do not exist

    Jupiters are rare

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    They do not existThey do not exist

    Jupiters are rare

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    Why are we (and only we)here?...

    If the Universe isso big, and soold, and so finelybalanced tosupport life likeus, why are we

    seeminglyalone?....

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    Why are we (and only we)here?...

    If the Universe isso big, and soold, and so finelybalanced tosupport life likeus, why are we

    seeminglyalone?....

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    Why are wehere?...Selection effects can address the

    fine-tuning of our location within theUniverse.

    But what about theglobal properties ofthe Universe?...

    Theconstants of nature

    Thelaws of nature

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    The Anthropic Principle

    "Although our situation is not

    necessarily central, it is inevitably privilegedto some extent"

    Introduced by Brandon Carter (1973).

    A reaction to over-zealous use of the

    Copernican Principle: we are not at

    a special position in the Universe.

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    Why are wehere?...Selection effects can address the

    fine-tuning of our location within theUniverse.

    But what about theglobal properties ofthe Universe?...

    Theconstants of nature

    Thelaws of nature

    Weak

    A.P.

    StrongA.P

    .

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    The W.A.P. merely summarises the

    idea of selection effects for differentlocations in our Universe.

    The S.A.P. requires the existenceof other universes with different

    constants / laws of nature.

    Th i id t f

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    There is a w ide spectrum ofviews on the Anthropic Principle:

    Freeman Dyson:

    I do not feel like an alien in this

    universe. The more I examine theuniverse and the details of itsarchitecture, the more evidence Ifind that the universe in some

    sense must have known we werecoming.

    Th i id t f

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    There is a w ide spectrum ofviews on the Anthropic Principle:

    Heinz Pagels:

    The influence of the anthropic principle on

    contemporary cosmological models has been sterile.It has explained nothing and it has even had anegative influence. I would opt for rejecting theanthropic principle as needless clutter in the

    conceptual repertoire of science.

    Th i id t f

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    There is a w ide spectrum ofviews on the Anthropic Principle:

    Brandon Carter:

    The anthropic principle is a middle

    ground between the primitiveanthropocentrism of the pre-Copernican age and the equallyunjustifiable antithesis that no

    place or time in the universe canbe privileged in any way.

    Th k M l i

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    Three ways to make a Multiverse:

    1. Cosmological inflation

    2. M-theory / String Landscape

    3. Quantum cosmology

    Th t k M lti

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    Three ways to make a Multiverse:

    1. Cosmological inflation

    2. M-theory / String Landscape

    3. Quantum cosmology

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    Three ways to make a Multiverse:

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    Three ways to make a Multiverse:

    1. Cosmological inflation

    2. M-theory / String Landscape

    3. Quantum cosmology

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    Present Day

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    Big Bang

    Present Day

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    Big Bang

    String TheoryString Theory

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    Particle representation String representation

    Point particles replaced by string loops

    Avoids infinities

    No unique theory

    (Branes in higherdimensions)

    MM--TheoryTheory

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    yy

    More than the 3 spatial dimensionswhich we actually observe.

    Our observed spacetime emergesfrom the way in which the extradimensions are compactified.

    Calabi-Yau manifold

    There could be up to 10500 different compactifications

    each with a different set of constants of nature.

    We find ourselves in one that is anthropically selected.

    Three ways to make a Multiverse:

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    Three ways to make a Multiverse:

    1. Cosmological inflation

    2. M-theory / String Landscape

    3. Quantum cosmology

    Present Day

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    Big Bang

    Summary of QM InterpretationsSummary of QM Interpretations

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    Summary of QM InterpretationsSummary of QM Interpretations

    CopenhagenMany

    Worlds

    Transactional

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    But is it science?....

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    But is it science?....

    We cant observe the other universes.

    How do we test theories?

    How do we make predictions?...

    Much heated debate on these points.

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    Thomas Bayes

    (1702 1761 AD)

    Steven Weinberg

    Ockhams Razor

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    Frustra fit per plura, quodfieri potest per pauciora.

    It is vain to do with morewhat can be done with less.

    William of Ockham

    (1288 1348 AD)

    Everything else being equal,we favour models which aresimple.

    How do we measure the simplicity ofuniverse versus multiverse models?

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    Martin Gardner

    There is not the slightestshred of evidence that thereis any universe other thanthe one we are in. No

    multiverse theory has so farprovided a prediction thatcan be tested. As far as wecan tell, universes are notas plentiful as even twoblackberries

    Evolving constants of nature?...

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    g

    Paul Davies

    Lee Smolin

    CosmologicalNatural Selection?

    But why do we live in thismultiverse?....

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    y

    Hierarchical picture

    Different constants of nature

    Different laws of nature

    Different mathematical and logical structures

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