+56'0+0)614#8+6#6+10#.#8'5U +056'+0510).+0'5(41/6*'0+8'45' Barry C. Barish

Transcription

1 +56'0+0)614#8+6#6+10#.#8'5U +056'+0510).+0'5(41/6*'0+8'45' Barry C. Barish

2 .$' '+0

3 +45##%'9610 Perhaps the most important scientist of all time! Invented the scientific method in Principia Greatest scientific achievement: universal gravitation

4 %+'06+(+%'6*1& 4+0%+2+# ❶ We are to admit no more causes of natural things such as are both true and sufficient to explain their appearances ❷ the same natural effects must be assigned to the same causes ❸ qualities of bodies are to be esteemed as universal ❹ propositions deduced from observation of phenomena should be viewed as accurate until other phenomena contradict them.

5 ' '45#.4#8+6#6+10 Three laws of motion and law of gravitation (centripetal force) disparate phenomena» eccentric orbits of comets» cause of tides and their variations» the precession of the earth s axis» the perturbation of the motion of the moon by gravity of the sun Solved most known problems of astronomy and terrestrial physics» Work of Galileo, Copernicus and Kepler unified.

6 .$' '+0 The Special Theory of Relativity (1905) overthrew commonsense assumptions about space and time. Relative to an observer, near the speed of light, both are altered» distances appear to stretch» clocks tick more slowly The General Theory of Relativity and theory of Gravity (1916)

7 +056'+05 2#%'6+/' 4+0-.'5 Discards concept of absolute motion; instead treats only relative motion between systems space and time no longer viewed as separate; rather as four dimensional space-time gravity described as a warpage of space-time, not a force acting at a distance

8 +056'+05*'14;1(4#8+6#6+10 ':2'4+/'06#.6'565 Einstein Cross The bending of light rays gravitational lensing Mercury s orbit perihelion shifts forward twice Newton s theory

9 +056'+05*'14;1(4#8+6#6+10 ':2'4+/'06#.6'565 Newton s Theory instantaneous action at a distance Einstein s Theory information carried by gravitational radiation at the speed of light

10 4#8+6#6+10#.#8'5 6*''8+&'0%' Neutron Binary System PSR Timing of pulsars 17 / sec ~ 8 hr

11 7.5'#0&#;.14 4'57.65 emission of gravitational waves due to loss of orbital energy period speeds up 14 sec from measured to ~50 msec accuracy deviation grows quadratically with time

12 +056'+05 10).+0'5 Radiation of Gravitational Waves from binary inspiral system Leslie is an applicant LISA

13 06'4('41/'6'45 52#%' The Laser Interferometer Space Antenna (LISA) The center of the triangle formation will be in the ecliptic plane 1 AU from the Sun and 20 degrees behind the Earth.

14 56412*;5+%5174%'5 (4'37'0%;4#0)' EM waves are studied over ~20 orders of magnitude» (ULF radio > HE γ rays) Audio band Gravitational Waves over ~10 orders of magnitude» (terrestrial + space)

15 06'4('41/'6'45 6'44'564+#. Suspended mass Michelson-type interferometers on earth s surface detect distant astrophysical sources International network (LIGO, Virgo, GEO, TAMA) enable locating sources and decomposing polarization of gravitational waves.

16 06'40#6+10#. '6914- LIGO Simultaneously detect signal (within msec) GEO Virgo TAMA detection confidence locate the sources AIGO decompose the polarization of gravitational waves

17 4#8+6#6+10#.#8'5 6*''(('%6 Leonardo da Vinci s Vitruvian man The effect is greatly exaggerated!! stretch and squash in perpendicular directions at the frequency of the gravitational waves If the man was 4.5 light years high, he would grow by only a hairs width LIGO (4 km), stretch (squash) = m will be detected at frequencies of 10 Hz to 10 4 Hz. It can detect waves from a distance of light years

18 '6'%614 %10%'26 The concept is to compare the time it takes light to travel in two orthogonal directions transverse to the gravitational waves. The gravitational wave causes the time difference to vary by stretching one arm and compressing the other. The interference pattern is measured (or the fringe is split) to one part in 10 10, in order to obtain the required sensitivity.

19 #2#0 Schematic of TAMA 300m interferometer The effects of gravitational waves appear as a fluctuation in the phase differences between two orthogonal light paths of an interferometer.

20 5+6'5 Hanford Observatory Livingston Observatory

21 +8+0)5610

22 #0(14&

23 '#/7$' LIGO beam tube under construction in January ft spiral welded sections girth welded in portable clean room in the field

24 8#%77/'37+2/'06

25 26+%5 Optics polished & coated» Microroughness within spec. (<10 ppm scatter)» ROC within spec. (δr/r < 5%, except for BS)» Coating defects within spec. (pt. defects < 2 ppm, 10 optics tested)» Coating absorption within spec. (<1 ppm, 40 optics tested) Optics polished at CSIRO in Australia

26 +056'+05 10).+0'5 AIGO will soon listen for Einstein s Songlines with gravitational waves Basic tests of General Relativity will be possible (eg. Black holes)

27 174%'51(4#8+6#6+10#.#8'5 Inspiral of Neutron Stars Chirp Signal

28 *+42+)0#. $+0#4;+052+4#. determine distance from the earth r masses of the two bodies orbital eccentricity e and orbital inclination i

29 174%'51(4#8+6#6+10#.#8'5 Supernovae gravitational stellar collapse The Collapse Optical Light Curve

30 174%'51(4#8+6#6+10#.#8'5 Supernovae optical observations Crab Nebula 1054 AD Supernovae - SN1994I

31 72'4018#' ' (41/EMLK

32 72'4018#' 4#8+6#6+10#.#8'5 Non axisymmetric collapse burst signal Rate 1/50 yr - our galaxy 3/yr - Virgo cluster

33 174%'51(4#8+6#6+10#.#8'5 Murmurs from the Big Bang signals from the early universe Cosmic microwave background

34 100'%66*'')+00+0)1(6*' 0+8'45'6170&#/'06#.*;5+%5

35 56412*;5+%5#0&15/1.1); More than 95% of the Universe is non luminous matter (dark matter) Gravitational waves will open up an entirely new window on the Universe

36 Australian Consortium for Interferometric Gravitational Astronomy (ACIGA) The University of Western Australia The Australian National University The University of Adelaide CSIRO Lindfield Monash University The First Stage of the Laser Interferometer Gravitational Wave Observatory