How to interpret the LIGO signal on the

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How to interpret the LIGO signal on the back of an envelope Alexander Penin

How to interpret the LIGO signal on the back of an envelope Alexander Penin University of Alberta & TTP Karlsruhe NYU, New York October 6 th, 2016

LIGO experiment

LIGO experiment

LIGO experiment

LIGO experiment

LIGO data

LIGO data

Can we hear the shape of a drum?

Can we hear the shape of a drum?

Can we hear the shape of a drum? Yes! for convex planar drums with

Can we hear the shape of a drum? Yes! for convex planar drums with analytic boundary Steve Zelditch (2000)

Can we hear the shape of a drum? Yes! for convex planar drums with

Can we hear the shape of a drum? Yes! for convex planar drums with analytic boundary Steve Zelditch (2000) LIGO event reconstruction: fitting with templates based on numerical gravity

Is it possible to identify the astrophysical origin of the LIGO event by hand

Is it possible to identify the astrophysical origin of the LIGO event by hand rather than by a supercomputer?

Tools

Tools

Plan • Gravitational waves in a nutshell polarization radiation energy flow detection • Data

Plan • Gravitational waves in a nutshell polarization radiation energy flow detection • Data analysis Initial phase: linear regime, determination of the mass Final phase: nonlinear regime, determination of the distance

Gravitational waves

Gravitational waves

General properties Linearized/weak field approximation Gravity Coordinate transformation Einstein equations Electrodynamics Gauge transformation Maxwell

General properties Linearized/weak field approximation Gravity Coordinate transformation Einstein equations Electrodynamics Gauge transformation Maxwell equations

Polarization Gravity Electrodynamics

Polarization Gravity Electrodynamics

Detection Geodesic equation: Length variation: no acceleration!

Detection Geodesic equation: Length variation: no acceleration!

Energy flow Electrodynamics Gravity

Energy flow Electrodynamics Gravity

Radiation Gravity quadrupole Newtonian binary system: (Hulse/Taylor NP 92) Electric dipole

Radiation Gravity quadrupole Newtonian binary system: (Hulse/Taylor NP 92) Electric dipole

Innermost stable orbit Effective potential Innermost stable orbit Energy release

Innermost stable orbit Effective potential Innermost stable orbit Energy release

Data analysis

Data analysis

Two regions

Two regions

Linear region Weak time dependence of period/amplitude

Linear region Weak time dependence of period/amplitude

Determination of the mass Theory: Data: Results (equal masses, e=0): Stable orbit condition: e

Determination of the mass Theory: Data: Results (equal masses, e=0): Stable orbit condition: e 0 Mass upper bound:

Non-Linear region strong time dependence of the period and the amplitude

Non-Linear region strong time dependence of the period and the amplitude

Determination of the distance Theory: Data: Result:

Determination of the distance Theory: Data: Result:

Comparison to numerical gravity

Comparison to numerical gravity

Summary

Summary