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

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Presentation transcript:

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

LIGO experiment

LIGO experiment

LIGO data

Can we hear the shape of a drum?

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 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 rather than by a supercomputer?

Tools

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

Gravitational waves

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

Polarization Gravity Electrodynamics

Detection Geodesic equation: no acceleration! Length variation:

Energy flow Electrodynamics Gravity

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

Innermost stable orbit Effective potential Innermost stable orbit Energy release

Data analysis

Two regions

Linear region Weak time dependence of period/amplitude

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

Determination of the distance Theory: Data: Result:

Comparison to numerical gravity

Summary