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Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Mar 31, 2015

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Page 1: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.
Page 2: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Science starts with curiosity ...something that is born in all of us

The starting point is to find patterns in the natural world

Page 3: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Seeing the Universe

Visible light is a half-tone range where EM spectrum is full piano

Page 4: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

108

1600 1700 1800 1900 2000

Ga

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Improvement over the Eye

Year of Observation

Telescopes alone

Photographic & electronic detection

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Improving on the Eye

2012

1011

Page 5: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

The largest telescope can see 1011 times (100 billion x) fainter than the naked eye

WHERE DOES THIS GAIN COME FROM?

The first factor is light gathering power

A gain of 10m over 1cm (or 0.01m) squared, a factor of 106

A Factor of Ten Billion

Page 6: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

The second factor is efficiency of detecting photons

The eye must “read out” every 1/10 of a second, like a movie camera, to give the illusion of motion. On the other hand, a CCD can integrate for hours before the image is read out.

For a gain of nearly 100% efficiency over 1% or so, or a factor of 100

WHAT IS THE LAST FACTOR OF 1000?

Page 7: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

The Copernican Revolution

The history of astronomy displaces us from cosmic importance

Page 8: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Estimation

Scientists often use estimation or order of magnitude calculations in their work. Often it is not possible, or necessary, to derive very accurate numbers. This is particularly true in astronomy where the objects under consideration are usually very faint and very far away.

X 10 Accuracy For most exploratory calculations X 2 Accuracy For most numbers in cosmology 10% Accuracy For the best-measured parameters

Page 9: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

DEDUCTIONDeduction combines statements or premises and combines them to reach a conclusion.

The conclusion is valid only if the premises are justified and the logical construction is correct.

Deduction preserves truth but doesn’t always expand knowledge.

i.e. symbolic logic, arithmetic, algebra

2 + 2 = 4

Page 10: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

DEDUCTIONInduction involves a generalization from a limited amount of data to a broad conclusion.

Induction cannot yield certainty, but backed by a lot of data, gives reliable conclusions.

Induction can expand knowledge so is a basic tool of science.

i.e. data is always finite so theories are always subject to verification.

INDUCTION

Page 11: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Science Limitations

Uncertainty, imprecision, and error arise three different ways:

CONCEPTUAL

MACROSCOPIC

MICROSCOPIC

Making a false premise, confusing correlation with causation, inferring a pattern where none is present

There is no such thing as perfect data. Every data set is limited and every instrument has limitations

Heisenberg’s uncertainty principle sets a fundamental limit to precision for measurement of particle position and velocity, or energy and time

Page 12: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Evidence is:

• based on data

• reproducible

• quantitative

• not subjective

• never perfect

Science is Evidence

Page 13: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

The Importance of Evidence • There is no science without evidence• All assertions must be supported by data• Every claim in science is subject to

verification

Science is data-driven, so progress is made by:

1. Gathering more data

2. Repeating the experiment

3. Someone else repeating the experiment

GOOD!

BETTER!!

BEST!!!

Page 14: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.
Page 15: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

• Science seeks robust explanations for observed phenomena that rely solely on natural causes.

• Science progresses by creating and testing models of nature that explain the observations as simply as possible.

Occam’s Razor (there may be more than one explanation for any particular data set)

• A scientific model must make testable predictions that may force us to revise or abandon the model.

• Plus, the role of luck and persistence: Science is a very human enterprise!

Good Science

: a model which survives repeated testingTheory

Page 16: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

For 99.999999999999999999999999999% of the universe, including all stars and all galaxies, the evidence is indirect.

Page 17: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.
Page 18: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Distance Units

1 pc

1 Mpc

10 Gpc

Typical distance between stars is 1 pc = 3.36 light years = 6 trilllion km, or 6,000,000,000,000 km.

Typical distance between galaxies is 1 Mpc = 106 pc or 3 million light years. It’s an incredible 1019 km.

The size of the observable universe is about 10 Gpc = 1010 pc, or 30 billion light years. That distance is an unimaginable 1023 km.

Page 19: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Us

Milky Way

Earth

THE UNIVERSE AND US

Solar System

Universe Multiverse?

Page 20: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

A Scale Model

Set the Earth to the size of a walnut, or a 1:10,000,000 scale model

=

• The Moon is a pea at arm’s length

• The Sun is a 3 m ball 100 m away

• Neptune is another pea 2 km away

• The nearest star is 50,000 km away

Page 21: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

• The Moon is a seconds walk away

• The Sun is 8 minutes walk away• 10 hours to walk the Solar System

• A year to walk to the nearest stars

And at this scale, light is reduced to very slow walking speed. There’s no way information in the universe can travel any faster

Page 22: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Reduce the scale by a factor of 100,000,000

• The Solar System is a grain of sand

• The distance between stars is 10 m

• The Milky Way is the size of India

• The MW has 100,000,000,000 stars

Page 23: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Now reduce by another factor of 100,000,000

• The Milky Way is the size of a plate

• The nearest galaxy is 10 m away

• The universe is the size of India• Billions of galaxies within this space

Page 24: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

How Empty is Space?

A one-inch cube of the air you’re breathing holds 1020 atoms in it

The average density of the universe is 1022 times lower, about 1 atom per cubic meter

Page 25: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Lookback Time

If the speed of light were infinite, light from everywhere in the universe would reach us at exactly the same time and we would see the entire universe as it is now.

But it is not, so we see distant regions as they were in the past.

Page 26: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

How can we know what the universe was like in the past?

• Light travels at a finite speed (300,000 km/s).

• Thus, we see objects as they were in the past:

The farther away we look in distance, the further back we also look in time.

Destination Light travel time

Moon 1 second

Sun 8 minutes

Sirius 8 years

Andromeda (M31) 2.5 million years

Page 27: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Nearby “Now”

“Long Ago” Galaxies

LOOKBACK TIME

“Recent” Stars

“Ancient” Universe

Page 28: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Scattered in a universe 46 billion light years across

Galaxies

Page 29: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

The Milky Way is typical with 400 billion stars

Stars

Page 30: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Almost all the simple elements hydrogen and helium

Atoms

1080

Page 31: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

A hundred million photons for every particle

Photons

1088

Page 32: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Mediocrity

We therefore live on an:

• Average planet around

• An average star in an

• Average galaxy in a• Very large universe

Copernicus

Page 33: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.
Page 34: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Science is Seeing

A Timeline

Page 35: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

How do our lifetimes compare to the age of the universe?

• The Cosmic Calendar: a scale on which we compress the 13.7 billion year history of the universe into 1 year.

• This is a time scale model that used a scale factor of 14,000,000,000:1.

• Our lives would scale similarly, so 80 years goes down by a factor of 14 billion too.

• In the scale model, a human life lasts about 2 tenths of a second!

Page 36: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

No Arrow of Time

Arrow of Time

Black Holes

TIME SENSE

Single Atoms

Sentient Life

Lots of Atoms

Page 37: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Speed of Light

Size

Time

The Universe

The early universe expanded much faster than the speed of light, so there are objects and large regions of space we have never seen.

This violates no law of physics since the cosmic expansion is governed by general relativity, which sets no limit on the speed of expanding space.

Page 38: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Galaxy spectra show redshifts, where all the spectral features shift to longer wavelengths. The amount of the shift increases with growing distance: more distant galaxies are moving away faster.

This linear relation was discovered by Edwin Hubble back in 1929.

Hubble Expansion

Page 39: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

The redshift is not a Doppler shift; it is due to the expansion of space itself. Photons are stretched.

Page 40: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

• Galaxies are all moving away from each other, so every galaxy sees the same Hubble expansion, i.e there is no center.

• The cosmic expansion is the unfolding of all space since the big bang,

i.e. there is no edge.

• We are limited in our view by the time it takes distant light to reach us,

i.e. the universe has an edge in time not space.

Page 41: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Space really does expand, like the material of the balloon. The balloon surface area is finite but unbounded. The universe is close to flat so imagine a large balloon with little curvature

Photons in this 2D space have their wavelengths stretched or redshifted by the expansion as they travel

Nature of the Expansion

Galaxies are held together by gravity and do not expand, so imagine coins glued to the balloon

Page 42: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Dark matter binds galaxies and dark energy drives cosmic acceleration.

Page 43: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Nature of the Expansion

Early expansion is rapid, driven by radiation. It slows as dark matter begins to dominate and more recently

has begun to accelerate due to dark energy.

Page 44: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.
Page 45: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Life occurs in a range of scales that extends from galaxies to the atomic nucleus, as symbolized by the ancient symbol of the ouroboros, the snake

that eats its tail

Unity

Page 46: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Science is Seeing

Ouroboros

Page 47: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

A sand grain of diameter 0.5mm weighs about 3 grams. The sand is SiO2, molecules 60 times hydrogen mass.

1019 atoms

Page 48: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

A normal monk, one who does not like “momos” too much, weighs about 50 kg. Monks are made of water, H2O, molecules 17 times hydrogen mass.

1028 atoms

NOTE: EVERYTHING THAT HAS MASS EXPERIENCES THE GRAVITY FORCE, INCLUDING ATOMS. HOWEVER, THE BEHAVIOR OF ALL SMALL OBJECTS, SUCH AS MONKS AND MOUNTAINS, IS GOVERNED BY THE FAR STRONGER ELECTRIC FORCE BETWEEN ATOMS. FOR ANY OBJECT WITH MORE THAN ABOUT 1045 ATOMS, OR A SIZE ABOUT 100 KILOMETERS, GRAVITY BECOMES THE DOMINANT. SO GRAVTY DRIVES THE BEHAVIOR OF PLANETS, STARS, GALAXIES, AND THE UNIVERSE.

Page 49: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

One solar mass is 2 x 1030 kg. Which is an enormous factor larger than a hydrogen atom 2 x 10-27 kg. Earth is 330,000 times less massive.

1057 atoms

Page 50: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

The typical galaxy contains 1012 stars

The whole universe contains 1011 galaxies

1069 atoms 1080 atoms

Page 51: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

What is Dark

Matter? THE SHORT ANSWER IS: WE DON’T KNOW. BUT SEVERAL LINES OF EVIDENCE INDICATE 10X MORE INVISIBLE THAN VISIBLE MATTER

The rotation speed of galaxies does not decline with radius, violating Kepler’s law unless without a halo of unseen matter

Page 52: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Light from distant galaxies is bent by an intervening cluster to form little arcs. The amount of bending indicates a lot of unseen matter in the cluster.

Light from all distant galaxies is very slightly distorted and bent as it travels through the “sea” of dark matter. With the best images, these distortions of 0.1% in shape can be seen.

Page 53: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Why are astronomer so confidentthat dark matter really exists?

Because the law of gravity haspassed so many tests, and if weput dark matter into computersimulations, we evolve structurethat looks just like the universe.

So far, we can only rule items out:

Stars: (normal matter) census of stars does not allow it

MACHOs: (sub-stars & planets) gravitational lensing rules it out

Black holes: (dark, collapsed stars) no sign of preceding supernovae

Dust: (dust up to rocks) re-radiation in infrared not seen

Which leaves: weakly interacting particles, supersymmetric extension to standard model

Page 54: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Experiments in the 1960’s and 1970’s showed that, just as atoms are not simple and fundamental, so protons and neutrons are made of much smaller particles that were named quarks.

Page 55: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

This scheme has multiple generations of particles and their anti-particles, so it is not very elegant or simple. This has led physicists to suppose that there may be an even deeper level of sub-atomic structure

Page 56: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Objects

Atoms

Universe

TOP DOWN

Dark Matter

Molecules

Page 57: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

String Theory

String theory postulates dynamic 1-dimensional entities that are only noticeable on scales of 10-43 meters, 33 orders of magnitude smaller than atoms!

Page 58: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

In string theory, the smoothness and the emptiness of space are illusions. If we could imagine ourselves at the incredibly tiny Planck scale, 10-43 meters, we would see a chaotic version of space-time. At every point, the six hidden dimensions that are not apparent in the everyday world would be manifested...

Page 59: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Atoms

Strings

BOTTOM UP

Bosons

Quarks

Leptons

Electrons

Page 60: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Four Forces

Strength: 10-38 10-19 0.0073 1

Range: Long Subatomic Long Subatomic

Page 61: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

The forces are associated with particular families of particles. But just as these particles are secondary manifestations of strings, the individual forces are manifestations of a single underlying “superforce”

Page 62: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.
Page 63: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Energy is a very broad concept. It is anything that can make matter move or change

Energy changes forms constantly but is not created or destroyed: this is a law of physics

Page 64: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Energy can be kinetic, the overall motion of an object

Energy can be radiant, light or other electromagnetic waves

Energy can be potential, stored in a number of ways

• Chemical bonds• Electric fields• Magnetic fields• Gravity fields• Elastic (materials)

Page 65: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Light is an electromagnetic

wave

Page 66: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Photons: they are “pieces” of light, each with a precise wavelength, frequency, and energy. Think of photons as tiny bullets, localized in space

Photon energy is proportional to frequency of the wave

Within the visible spectrum, blue light has higher energy than red light

Within the electromagnetic spectrum, X-rays have the highest energy, followed by UV, visible light, IR, and radio

Remember: Light is just one form of electromagnetic wave of energy, the kind we can detect with our eyes.

Light is a Particle

Page 67: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.
Page 68: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

If you pass white light through a prism, it separates into its component colors

ROY G B I V

spectrum

long wavelengths

short wavelengths

Page 69: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

• Emission• Absorption• Transmission• Reflection or Scattering

Terminology: • Transparent: transmits light• Opaque: blocks (absorbs) light

Everything we know about the universe is a result of these effects

Light Interacts with Matter

Page 70: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

• Electrons in every atom have distinct energy levels

• Each chemical element, ion or molecule, has a unique set of energy levels

Atomic Energy Levels

Page 71: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Distinct energy levels lead to distinct emission or absorption lines

Hydrogen Energy Levels

Emission: atom loses energy

Absorption: atom gains energy

Page 72: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

• Atoms, ions, and molecules have unique spectral “fingerprints”• We identify chemicals in a gas by their spectral fingerprints• With additional physics, we can figure out abundances of the

chemicals, and often temperature, pressure, and much more.

Chemical Fingerprints

Page 73: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Continuous Spectrum

Hot/Dense Energy Source prism

Emission Line Spectrum

prismHot low density cloud of Gas

Absorption Line SpectrumCooler low density cloud of Gas

Hot/Dense Energy Source prism

Types of Spectra

Page 74: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Anywhere in the universe, atoms and molecules are always in constant, microscopic motion

Temperature is a measure of the average kinetic energy of the particles in a substance

COOLER HOTTER

Page 75: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

All the atoms and molecules in the universe are in constant (invisible) microscopic motion or vibration:

Thermal energy

As a result, every substance emits a smooth spectrum of radiation, mostly at invisible infrared wavelengths:

Thermal radiation

Page 76: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.
Page 77: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

E = mc2

Mass-Energy

Another way to think about this is that the energy that holds the helium nucleus together has a tiny amount of equivalent mass, and that energy gets released going by fusion from hydrogen to helium

small numberbig number huge number

Page 78: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

When 0.7% of the mass of a hydrogen atom is converted to radiant energy it is a huge amount relative to the mass involved

The mass-energy in the ink in the dot at the end of a sentence in a book could power a typical family home for an entire year

Page 79: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

What is Dark

Energy? THE SHORT ANSWER IS: WE DON’T KNOW. BUT ONE OBSERVATION OF DISTANT SUPERNOVAE POINTED TO A COSMIC ACCELERATION

Page 80: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Re

dsh

ift c

z (k

m/s

)

Riess et al. (1998)Perlmutter et al. (1999)

Constant or faster in past (expected)

Slower in past (big surprise!)

Riess, Press, & Kirshner (1996)

30,000

300,000

3,000100 1,000 10,000

Distance (Mpc)

Farther in the past

Expansion History of the Universe

Page 81: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Einstein’s Theory: General

Relativity

Riess et al. 1998Perlmutter et al. 1999

Accelerating

Decelerating

No Big

Bang

0

1

2

3

1 2

ClosedOpen

Strength of matter

Str

engt

h of

cos

mol

ogic

al c

onst

ant,

L

x

If the acceleration is caused by Einstein’s cosmological constant, HST data on 8 SN Ia have increased our cosmology knowledge by a factor of 7

Riess et al. 2004Tonry et al. 20038 HST SN Ia z > 1

Page 82: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Dark energy is much moremysterious than even darkmatter. It’s existence restson the unexpectedly faintdistant supernovae, and afew less direct arguments.The direct detection of darkenergy is very challenging.

Physics provides no assistance. The vacuum of space could have energyin quantum theory, but it would be 1080 times larger than is observed!

Dark energy is a repulsive force that counter gravity. It does not changeits strength with time (Einstein’s gravitational constant “blunder”)

The density of dark energy and dark matter are roughly equal, this is theonly time in the history of the universe that is true: is this a coincidence?

Page 83: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.
Page 84: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Hierarchies are the relationships between things, when few items are composed of many. This is represented as a tree or as a network.

Page 85: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Hierarchies in Astronomy

Mergers of black holes… …and galaxies

TIME

Page 86: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

A hierarchy of self-reproducing universes in the big bang

Page 87: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Sometimes the structures in physics and biology are strikingly similar, and can be described by similar mathematical forms

Page 88: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Matter is subject to gravity, which gives structure on many scales

Radiation does not interact with itself and has no form or structure

Page 89: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Superforce

Page 90: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

First instant after the big bang event

Most of the history of the universe

The underlying unity suggested by string theory and the unification of forces is only realized in the big bang itself

Page 91: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

A few dimensionless parameters govern the behavior of the universe:

• Matter Density• Energy Density• Fine Structure Constant• Entropy per Baryon• Dielectric Constant• Number of Space Dimensions

A few pure number occur over and over through mathematics

Page 92: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

The 92 stable elements in the periodic table lead to almost infinite complexity. Life uses only about 20.

Page 93: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Cosmological

The universe was initially very smooth; over time complex structures grew by the action of gravity

Page 94: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Quantum fluctuations are a mechanism for multiple realizations of the universe

Quantum fluctuations are a mechanism for multiple realizations of the universe…leading to the concept of the “multiverse”

Page 95: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

More than just this… More than just this…

LEVEL 1: regions we can not see in big bang model

LEVEL 2: many bubbles of space-time, unobservable by us, different properties

LEVEL 3: indeterminacy, and quantum variation

LEVEL 4: mathematical forms, multi-dimensional space-times, 10 preferred

Page 96: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

String Theory Landscape String Theory Landscape

Perhaps 10 different vacua Perhaps 10 different vacua

500500

de Sitter expansion in these vacua create quantum fluctuations and provide the initial conditions for inflation. String theory provides context for the “multiverse”

Page 97: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.
Page 98: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Knowing1 Space

2

Time3

Matter

4

Energy

5Structure

6

Life 7

Meaning 8

Page 99: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

As creatures who occupy a tiny portion of time and space we have learned much about our universe. But many important questions are still answered.

• WHAT IS TIME?• WHAT IS SPACE?• WHAT IS MATTER?• WHAT CAUSED THE BIG BANG?• IS THE UNIVERSE UNIQUE?• ARE WE ALONE?

Page 100: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

In the universe with ten thousand billion billion stars, and a likely myriad of life forms, we’re special in some ways yet we are not in a cosmic sense. This leads to another big question:

WHY ARE WE HERE?

Page 101: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Brandon Carter presented the “anthropic principle” in 1973 in Poland during the 500th birthday of Nicklaus Copernicus. The idea seems to subvert the sense that we are not special, by elevating the role of intelligent observers in the universe to central importance.

• The weak form of the anthropic principle states that we can only observe a universe with properties such that intelligent observers exist. This is self-evident and little more than a tautology.

• The strong form of the anthropic principle states that the universe has to be the way it is because intelligent observers exist. This is much more audacious because it implies a special role for life.

Anthropic Principle

Page 102: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

• Stars of the right type for sustaining life supportable planets only can occur during a certain range of ages for the universe– stars of the right type only can form for a narrow

range of values of the gravitational constant• Living cells consists of light and heavy elements

(hydrogen, carbon, oxygen, and metals such as iron, copper, etc.)– To make both the light and heavy elements in the

correct proportions, the strengths of the various fundamental forces must lie within a very narrow range of values

• But does this place too specific a requirement on life? Perhaps life just needs disequilibrium chemistry and an energy source, not necessarily carbon and a star.

Conditions for Life

Page 103: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

• Gravitational force– Attractive force between all objects with mass– Weakest, long range

• Electromagnetic force– Attractive and repulsive

– Long range, 1039 times stronger than gravity

• Nuclear Weak force– Cause neutrons to decay into protons– Range <10-17 m, 1028 times stronger than gravity

• Nuclear Strong force– Holds the nucleus together– Range <10-15 m, 1041 times stronger than gravity

Fundamental Forces

Page 104: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

• Some physical coincidences are noteworthy and so beg for an explanation. All the seemingly arbitrary, unrelated constants in physics have one strange thing in common – they have just the values that would create a universe capable of sustaining life. In other words, our universe could have quite different values of the fundamental forces and it would be physically sensible, but it would contain no carbon-based life forms.

Coincidences

Page 105: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

• Gravitational force– A bit stronger, and stars have rapid, unstable lives– A bit weaker, no supernovae, so no heavy elements

• Electromagnetic force– A bit stronger, no shared electrons, no chemistry

– A bit weaker, atoms cannot hold their electrons

• Nuclear Weak force– A bit stronger, neutrons all decay, no heavy elements– A bit weaker, all hydrogen converted to inert helium

• Nuclear Strong force– A bit stronger, nuclear reactions too efficient, H to Fe– A bit weaker, electrical repulsion splits apart nuclei

Fine-Tuning of Forces

Page 106: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

0 X

• The following incredibly precise tweaking of the Universe is known as the flatness-oldness problem

• The critical density is the matter density just required to eventually overcome the expansion of the big bang

• If X is critical density, what is the actual density?

• It could have any value, but the matter density has a huge impact on the evolution of the universe

• Only a value relatively close to the critical value leads to an old and flat universe

Cosmological Fine-Tuning

Page 107: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

The matter density is only ¼ critical; the other major component affecting the expansion is dark energy, which leads to another issue related to fine-tuning….

OPEN

FLAT

CLOSED

– If the density is much below critical, early expansion is too rapid for stars and galaxies to form, so no life

– If the density is much above critical, the universe will recollapse quickly, with not enough time for stellar evolution to create carbon, and once again, no life

Page 108: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Our universe emerged from a quantum space-time foam at the Planck epoch. Other universes may have been spawned this way, with physical properties that are randomly different.

Multiverse Redux

Most of the past, present and future universes in the multiverse would be inhospitable to life. Ours is just a mediocre member of the ensemble.

Page 109: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Is there really a logical basis for anthropic arguments about life?

1. We shouldn’t be surprised to see features of the universe that are compatible with our existence

2. We should be surprised not to see features of the universe that are incompatible with our existence

1 is true, but 2 does not follow from it

This universe has special features, like a double six thrown with dice. The multiverse hypothesis is akin to speculating that there are many possible outcomes, ours is “double six”

The odds of double six are always 1 in 36, so the supposition above doesn’t explain it

A double six will occur eventually in a long sequence of throws, sequential or parallel

This is the “inverse gamblers” fallacy

Applying Logic

Page 110: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

Let’s look at the strange conceptual journey we have just followed

We can only observe a universe that is capable of creating observers like us

Some features of the universe are very finely-tuned around the existence of life

But is this an unduly anthropocentric view of life based on stars and carbon?

Quantum creation and string theory give the context for the multiverse ensemble

Fine-tuning might be due to happenstance, providence, or self-selection in a multiverse

And how to assign likelihood or probability on an infinite set of hypothetical universes?

But these theories are not yet well-tested and other universes are unobservable

Epistemology

Page 111: Science starts with curiosity...something that is born in all of us The starting point is to find patterns in the natural world.

• The physical parameters of nature and the universe are tuned to values that allow carbon-based life.

• The big bang allows for other universes and other realities but most of these might be devoid of life.

• The universe is “built for life” in a profound way, but this begs the question of the definition again.

• Is it self-selection, coincidence, or evidence of design?• We share a planet with other sentient life forms, and it’s

very likely there is sentience elsewhere.• Our power carries moral responsibility and obligation.

Sentience and

mortality define the

human condition

Sentience and

mortality define the

human condition