9
1 Astro-Particle Physics 9 Gravitational waves Manfred Jeitler

1 Astro-Particle Physics 9 Gravitational waves Manfred Jeitler

Embed Size (px)

Citation preview

Page 1: 1 Astro-Particle Physics 9 Gravitational waves Manfred Jeitler

1

Astro-Particle Physics 9Gravitational waves

Manfred Jeitler

Page 2: 1 Astro-Particle Physics 9 Gravitational waves Manfred Jeitler

2

Mass is always positive

Differently from electric charge, magnetic fields and color charge, there is no “negative” mass

Even antimatter has “positive” mass

Therefore there cannot be gravitational monopole or dipole fields

Have to look for quadrupole fields

Page 3: 1 Astro-Particle Physics 9 Gravitational waves Manfred Jeitler

3

Page 4: 1 Astro-Particle Physics 9 Gravitational waves Manfred Jeitler

4

Page 5: 1 Astro-Particle Physics 9 Gravitational waves Manfred Jeitler

5

Hulse-Taylor binary

indirect demonstration of gravitational waves

Orbital decay of PSR B1913+16.The data points indicate the observed change in the epoch of periastron with date while the parabola illustrates the theoretically expected change in epoch according to general relativity.

Nobel prize 1993 to Hulse and Taylor

Page 6: 1 Astro-Particle Physics 9 Gravitational waves Manfred Jeitler

6

Michelson interferometer

Page 7: 1 Astro-Particle Physics 9 Gravitational waves Manfred Jeitler

7

Northern leg (x-arm) of LIGO interferometer on Hanford Reservation

Page 8: 1 Astro-Particle Physics 9 Gravitational waves Manfred Jeitler

8

Page 9: 1 Astro-Particle Physics 9 Gravitational waves Manfred Jeitler

9

Ground-based detectors like the Laser Interferometer Gravitational-Wave Observatory (LIGO) will view the high-frequency waves from transient phenomena, like supernovae and the final minutes of inspiraling neutron-star binaries. LISA will observe the lower frequency waves from quasi-periodic sources, like compact star binaries long before coalescence, and supermassive black-hole binaries in the final months of coalescence.