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View webinar videos and learn more about BMSA at www.nas.edu /MathFrontiers Board on Mathematical Sciences & Analytics
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Page 1: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

View webinar videos and learn more about BMSA at www.nas.edu/MathFrontiers

Board on

Mathematical Sciences & Analytics

Page 2: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

View webinar videos and learn more about BMSA at www.nas.edu/MathFrontiers

February 12: Machine Learning for Materials Science*

March 12: Mathematics of Privacy*

April 9: Mathematics of Gravitational Waves

May 14: Algebraic Geometry

June 11: Mathematics of Transportation

July 9: Cryptography & Cybersecurity

August 13: Machine Learning in Medicine

September 10: Logic and Foundations

October 8: Mathematics of Quantum Physics

November 12: Quantum Encryption

December 10: Machine Learning for Text

MATHEMATICAL FRONTIERS2019 Monthly Webinar Series, 2-3pm ET

2

Made possible by support for BMSA from the National Science Foundation

Division of Mathematical Sciences and the

Department of Energy Advanced Scientific Computing Research

* Recordings posted

Page 3: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

View webinar videos and learn more about BMSA at www.nas.edu/MathFrontiers

Thomas Baumgarte, Bowdoin College

Mark Green, UCLA (moderator)

MATHEMATICAL FRONTIERSMathematics of Gravitational Waves

3

Manuela Campanelli, Rochester Institute of Technology

Page 4: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

View webinar videos and learn more about BMSA at www.nas.edu/MathFrontiers

MATHEMATICAL FRONTIERSMathematics of Gravitational Waves

4

Professor of MathematicsDirector, Center for Computational

Relativity and Gravitation

Revealing the Hidden Universe with

Gravitational WavesManuela Campanelli, Rochester Institute of Technology

Page 5: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

5

Manuela Campanelli

Image credit: LIGO/T. Pyle

Frontiers in Mathematics Webinar, April 9th, 2019, National Academies of Sciences, Engineering, and Medicine

Page 6: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

• Understanding the most extreme astrophysical objects!

• Dangerous distant places where gravity is very strong, matter is very dense and magnetic fields are very extreme!

Page 7: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

Regions of space where gravity is so intense that it prevents all matter and even light from

escaping!

Page 8: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

Im a g e : M ild e M a rk e tin g 2 0 0 8

“Space tells matter how to

move and matter tells space

how to curve” English translation by John Archibald Wheeler

1915

It predicts the existence of Black Holes …

… and of Gravitational Waves

Page 9: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

Gravitational waves stretchand compressspace-time itself!

Animation created by R. Hurt, Caltech/MIT/LIGO Lab

A lot of mass in very rapid

acceleration moving at speeds

close to

the speed of light!

This stretching and squeezing of space is no more than one ten thousandth the width of a proton ~10-19!

Page 10: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

Solving the Einstein’s

equations with the

use of

supercomputers!

Video Credits: Nicole Rosato RITTraveling at 60% of the speed of light!

Ripping space-time apart as they go!

Page 11: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

LIGO -Laser Interferometer Gravitational Wave Detector

These waves are

entirely different

spectrum than

light …

You need a special

ruler to measure the

stretching and

squeezing of space

Page 12: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

Was detected on September 14, 2015

Abbott et al, Phys. Rev. Lett. 116, 061102 (2016)

GW150914 occurred at a distance of more than one billion light years away!

Original Black Holes: 36 + 29 solar massesFinal Black Hole: 62 solar masses

Page 13: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

M c2 = E

3 solar masses x c2 = 4.5 x 1047 Joules

in 0.3 sec = 1 x 1048 Watts

radiated away in gravitational waves

19 000 000 000 000 000 000 000 000 000 000 000

000 000 000 000, 60W light bulbs

13

3 solar masses missing …1 Solar Mass = 333,000 Earth Masses!

This is more than 10 times the combined the light power

of every star and galaxy in the observable Universe!

Page 14: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

LIGO Hanford H1

LIGO Linvingston L1

Virgo Cascina PISA

"for decisive contributions to the LIGO

detector and the observation of

gravitational waves"

Page 15: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

LIGO Hanford H1

LIGO Linvingston L1

Virgo Cascina PISA

LIGO/Virgo scientific collaboration (LVC):

1000 scientists, 16 countries

Page 16: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

Abbott et al, Phys. Rev. Lett. 116, 061102 (2016)

Page 17: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

• They also change

character

depending on the

freedom we have

to explicitly write

them down!

• And black holes

have singularities!

A system of nonlinear, coupled, partial

differential equations with hundreds of terms!

The BSSN formalism developed by

Baumgarte and collaborators in 1999

Page 18: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

NCSA's Blue Waters

This requires very advanced numerical algorithms, which

translates into in hundred thousands lines of code!

And the processing power

of several petabytes

(one thousand million

million bytes —

1,000,000,000,000,000

bytes) of information at

once!

Page 19: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

Kip S. Thorne, 2017 Nobel Prize

lecture.

It took more

than four

decades for

researchers

to solve the

problem

But in 2005,

we finally

did it!

Page 20: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

Figure courtesy the SXS Collaboration

To compare them to LIGO data, and extract information about the black holes!

Page 21: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

21

1 Solar Mass = 333,000 Earth Masses!

But stay

tuned as

LIGO/Virgo

just restarted

taking new

data!

The LIGO/Virgo

detectors found 10

black hole binary

mergers and one

neutron star merger!

Page 22: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

Hubble Optical

More than 70 astronomy follow-up

observations!

NGC 4993130 million light-years from Earth, in the

constellation Hydra.

GW170817

Page 23: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

E = M c2

Energy

23

Page 24: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

Their masses can range from few times the one of our Sun to billions of Suns!

1 billion Solar Masses = 1,000,000,000 Solar Masses

1 Solar Mass = 333,000 Earth Masses

~2,400 billion Solar Masses

Page 25: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated
Page 26: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

T G 2 0 1 9 – Va n c o uve r Ja n ua ry 2 4, 2 0 1 9

Supermassive black holes

at the center of galaxies

are surrounded by

accreting hot gas and emit

powerful radio jets!

Because galaxies do merge,

the supermassive black holes

at their cores should merge too

Page 27: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

We are working on the modeling and observations of these

monster collisions!

Credits: RIT/NASA simulation

Page 28: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

General Relativity. + Magneto-Hydrodynamics

Several physics scales from microphysics to astrophysics!Vey long simulations and many parameters!

Page 29: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

We have just opened a new

window into the universe.

There might be surprises

awaiting for us!

“The most incomprehensible

thing about the Universe is

that it is comprehensible!

Stay Tuned for More Soon!

Page 30: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

View webinar videos and learn more about BMSA at www.nas.edu/MathFrontiers

MATHEMATICAL FRONTIERSMathematics of Gravitational Waves

30

William R. Kenan Professor of Physics

Einstein’s Gravity and the Geometry of

Black HolesThomas Baumgarte,

Bowdoin College

Page 31: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

View webinar videos and learn more about BMSA at www.nas.edu/MathFrontiers

Page 32: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

View webinar videos and learn more about BMSA at www.nas.edu/MathFrontiers

Page 33: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

View webinar videos and learn more about BMSA at www.nas.edu/MathFrontiers

Page 34: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

View webinar videos and learn more about BMSA at www.nas.edu/MathFrontiers

Page 35: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

View webinar videos and learn more about BMSA at www.nas.edu/MathFrontiers

Page 36: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

View webinar videos and learn more about BMSA at www.nas.edu/MathFrontiers

Page 37: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

View webinar videos and learn more about BMSA at www.nas.edu/MathFrontiers

Page 38: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

View webinar videos and learn more about BMSA at www.nas.edu/MathFrontiers

Page 39: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

View webinar videos and learn more about BMSA at www.nas.edu/MathFrontiers

Page 40: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

View webinar videos and learn more about BMSA at www.nas.edu/MathFrontiers

Page 41: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

View webinar videos and learn more about BMSA at www.nas.edu/MathFrontiers

Page 42: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

View webinar videos and learn more about BMSA at www.nas.edu/MathFrontiers

Page 43: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

View webinar videos and learn more about BMSA at www.nas.edu/MathFrontiers

Page 44: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

View webinar videos and learn more about BMSA at www.nas.edu/MathFrontiers

Page 45: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

View webinar videos and learn more about BMSA at www.nas.edu/MathFrontiers

Page 46: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

View webinar videos and learn more about BMSA at www.nas.edu/MathFrontiers

Page 47: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

View webinar videos and learn more about BMSA at www.nas.edu/MathFrontiers

The Schwarzschild solution

• Astrophysical significance not appreciated until 1960’s

• Describes non-rotating black holes, characterized by

‣ Curvature singularity at center:

‣ Event horizon at : “one-way” membrane

ds2 = −(

1−2M

r )dt2 +

(1−

2M

r )

−1

dr2 + r2dΩ2

Rabcd →∞

rS = 2M

Page 48: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

View webinar videos and learn more about BMSA at www.nas.edu/MathFrontiers

Page 49: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

View webinar videos and learn more about BMSA at www.nas.edu/MathFrontiers

Page 50: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

View webinar videos and learn more about BMSA at www.nas.edu/MathFrontiers

Page 51: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

View webinar videos and learn more about BMSA at www.nas.edu/MathFrontiers

Page 52: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

View webinar videos and learn more about BMSA at www.nas.edu/MathFrontiers

…and a breakthrough!• First successful simulations of

binary black hole mergers in

2005

• Pretorius

• Campanelli et.al.

• Baker et.al.

Campanelli et.al., 2006

Page 53: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

View webinar videos and learn more about BMSA at www.nas.edu/MathFrontiers

Page 54: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

View webinar videos and learn more about BMSA at www.nas.edu/MathFrontiers

Page 55: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

View webinar videos and learn more about BMSA at www.nas.edu/MathFrontiers

Page 56: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

View webinar videos and learn more about BMSA at www.nas.edu/MathFrontiers

Page 57: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

View webinar videos and learn more about BMSA at www.nas.edu/MathFrontiers

Thomas Baumgarte, Bowdoin College

Mark Green, UCLA (moderator)

MATHEMATICAL FRONTIERSMathematics of Gravitational Waves

57

Manuela Campanelli, Rochester Institute of Technology

Page 58: Board on Mathematical Sciences & Analyticssites.nationalacademies.org/cs/groups/depssite/... · M c2 = E 3 solar masses x c2 = 4.5 x 1047 Joules in 0.3 sec = 1 x 1048 Watts radiated

View webinar videos and learn more about BMSA at www.nas.edu/MathFrontiers

February 12: Machine Learning for Materials Science*

March 12: Mathematics of Privacy*

April 9: Mathematics of Gravitational Waves

May 14: Algebraic Geometry

June 11: Mathematics of Transportation

July 9: Cryptography & Cybersecurity

August 13: Machine Learning in Medicine

September 10: Logic and Foundations

October 8: Mathematics of Quantum Physics

November 12: Quantum Encryption

December 10: Machine Learning for Text

MATHEMATICAL FRONTIERS2019 Monthly Webinar Series, 2-3pm ET

58

Made possible by support for BMSA from the National Science Foundation

Division of Mathematical Sciences and the

Department of Energy Advanced Scientific Computing Research

* Recordings posted


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