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Douglas Osheroff Mahidol University Stanford University 12 How Advances In Science Are Made and How Science Changes Our Lives

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Douglas Osheroff Mahidol University Stanford University 12 December 2012

How Advances In Science Are Made and How Science Changes Our Lives �

ose discoveries that most change the way we think about nature cannot be anticipated. How, then, are such

discoveries made, and are there research strategies that can increase ones chances of making such a discovery?

A Linked Chain of Discoveries and Inventions

1853-1926

1853-1926

Heike Kammerlingh

Onnes first liquified

in 1908

Nobel Prize for Physics

1913

Gilles Holst

The process of advancing science often leads to inventions and technologies that directly benefit mankind. However, it is impossible to know from where the advance will come that

might solve a problem facing mankind. Consider, for example, nuclear magnetic resonance.

What Is Nuclear Magnetic Resonance? Just as a gyroscope precesses about the

Earth’s gravitational !eld when its axis of rotation is tipped away from the direction of the gravitational !eld, a

nuclear spin precesses in a magnetic !eld when the direction of its spin is tipped away from the direction of the magnetic

!eld. "e nuclear spins carry a magnetic dipole moment, and as this moment

precesses, it will generate an oscillating voltage in a pickup coil."e strength of this voltage depends upon the number of spins that are

precessing, and the frequency of this oscillating voltage is the same as the frequency of precession of the spin.

Chemical and Spin Shifts in NMR

Richard Ernst

Nobel Prize Chemistry

1991

Three Dimensional Conformation of Organic Molecules Kurt Wütrich

…in Aqueous Solutions

Kurt Wütrich

Nobel Prize for Chemistry

2002

Magnetic Resonance Imaging: MRI

Weatherwax High School Science Club

The 3He-4He Dilution Refrigerator Invented 1965

Thanks to the Helsinki low temperature lab.

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1950

Tinitial = 15 mK

Strategies: 1.  Utilize new technologies. • View nature from a new perspective or in a different realm. 2.  Don’t give up when things are going badly. • Failure may be an invitation to try something new. 3.  Spend a little time doing something different. • Curiosity driven research is fun, and can be rewarding! 4.  Avoid too many commitments. • The demands of good research do not adhere to a schedule. 5.  Back off from what you are doing occasionally to gain

a better perspective on the task at hand. • We become myopic when we focus too tightly on our work.

Stratey and Adams

Bloch and Purcell

Edwards and Hall

Hammel, Wheatley Landau …

Bardeen, Cooper

and Schreiffer Anderson,

Pomeranchuk ….

Advances in science are seldom made

by individuals alone. ey result

from progress of the scienti"c

community, asking questions,

developing new technologies to answer

those questions, and sharing their

results and their ideas with others. To

have rapid progress, one must support

scienti"c research broadly, and

encourage scientists to interact with one

another and to spend a bit of their

time satisfying their own curiosities.

!is is how advances in science are made.

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Galileo is often considered the father of modern astronomy. He improved the telescope, supported the helocentric view of the solar system first postulated by Copernicus, and discovered the four largest moons of Jupiter, now called the Galilean moons. Jupiter

Io Europa Ganymede Calisto

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Isaac Newton: Mathematician and Scientist Born 4 January 1643 Died 31 March 1727 (84 years)

We perhaps owe more to Sir Isaac Newton than to any other early scientist. He developed

the mathematics of calculus to understand particle motion, and the idea of a gravitational

!eld, thus explaining the motion of the planets.

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James Watt: Scottish Inventor born 1736 died 1819

Watt invented the rotary steam engine and used thermodynamics to vastly

increase the efficiency of steam engines.

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Industrial Pollution: Our Atmosphere and Waterways

Often human activity has a negative impact on our planet.

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1000 Years of Global CO2 and Temperature Change

Records of northern hemisphere surface temperatures, CO2 concentrations, and carbon emissions show a close correlation. Temperature Change: reconstruction of annual-average northern hemisphere surface air temperatures derived from historical records, tree rings, and corals (blue), and air temperatures directly measured (purple). CO2 Concentrations: record of global CO2 concentration for the last 1000 years, derived from measurements of CO2 concentration in air bubbles in the layered ice cores drilled in Antarctica (blue line) and from atmospheric measurements since 1957. Carbon Emissions: reconstruction of past emissions of CO2 as a result of land clearing and fossil fuel combustion since about 1750 (in billions of metric tons of carbon per year).

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Paleontology

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Life on Earth and Our Place in the Cosmos

The study of fossil remains of animals and plants that lived millions of years ago provides us with an understanding of the history of life on our planet. This is a story which helps us to better understand the origins

and evolution of life on Earth, and also to better appreciate the complex processes that produced the human race.

The evidence suggests that this planet is some 4.5 billion years old, and that our universe is some 14 billion years old. Our sun is one of

perhaps 100 billion stars in our galaxy, and we estimate that there are roughly 100 billion galaxies presently observable from Earth.

These studies do not enable us to create new technologies to improve our lives, but they pave the way for the exploration of our solar system

and beyond.

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James Clerk Maxwell and Electromagnetic Radiation James Maxwell was born in 1831 and died in 1879. He is the

father of the modern theory of electromagnetic radiation, which includes light. He found that a term was missing from

the four equations which described electric and magnetic !elds, and once he added that term, he quickly realized that

oscillating electric and magnetic !elds could propagate as waves.

Electromagnetic waves include radio waves, microwaves, light, X-rays and

Gamma rays.

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Charles Darwin

born 12 Feb. 1809 died 19 April 1882

Visited Galapagos

Islands in 1835

Theory of Natural Selection

Origin of the Species

published in 1859

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Alexander Fleming was born in 1881. He discovered penicillin in 1928, and was awarded the Nobel Prize in 1945. This was just the first of many antibiotics

to follow.

Health care in the US cost 2.4 trillion dollars in 2007

Born 6 Aug. 1881

Died 11 March 1955

Antibiotics and Modern Medical Science

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DNA: "e Double Helix

Nobel Prize for Physiology or Medicine 1962 James Watson, Francis Crick and Maurice Wilkins

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Rosalind Franklin

born July 25, 1920 died April 16, 1958

In 1953 Rosalind Franklin played a key role in the

discovery of the structure and function of DNA through her X-ray diffraction studies of DNA.

Only three people can share a Nobel Prize.

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The Transistor Invented

1947

by Bardeen Brattain

and Schockl

ey

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Apple iPhone G3

Bell System Telephone, 1950

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2.93 GHz Intel Duo Core Processor 8 GB Ram

320 (500) GB Hard Drive

Computers and the Internet

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Hubble Space Telescope Launched April 24, 1990

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NASA: Monitoring "e Health of Our Planet

NASA has launched satellites to monitor continuously the CO2 content in our atmosphere. Such Earth-looking probes

help give us our weather forecasts, assist with telecommunications, defense, and many other important

tasks that can best be done from orbit.

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Mars and the Mars Rovers: Robotic Exploration

Spirit and Opportunity

4,400,000 lb launch weight 7,125,000 lb initial thrust 1,125,000 lb thrust Orbiter 6,000,000 lb thrust SRB’s Maximum payload: 56,000 lb to 28º orbit + 220,000 lb orbiter

Thank You for your attention!