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Gnigdrib
Posted: Wed Mar 03, 2004 4:14 pm
Guest
Will the LIGO Experiment Work?

An ambitious experiment to detect gravitational waves from distant
astronomical sources is currently in preparation (Laser Interferometric
Gravitational Observatory - LIGO). A typical source for such waves would be two
stars circling each other in close proximity. It is proposed to detect these
waves by means of a two axis laser array to measure the relativistic effects of
the waves as they pass by. It is postulated that these waves will cause the
distance between the ends of the array, as sensed by Laser inteferometry, to be
moved by the "distortion of space" as they pass the Earth. It is expected that
this movement will be detectible by an interference pattern observable in Laser
signals sent between the ends of the arrays. Calculations have shown that the
gravitational wave produced by a massive star in close orbit about another
should contain enough energy to be readily detectible by this method. What does
not seem to be mentioned is the fact that LIGO is only capable of detecting
longitudinal waves. In addition in none of these reports does mention seem to
have been made of the fact that such waves must always be generated as multiple
waves which cancel completely for longitudinal waves and cancel in the far
field for transverse waves. Considering the distances involved and the size of
the LIGO array, all such observations will be made as distant far field
observations.

The generation of multiple waves (e.g.- two for a binary system) results
from the fact that, as is the case with a single gravitational object, the
center of gravity of a gravitationally coupled multiple object must remain
stationary as its component parts move with respect to each other. As a result,
the gravitational wave (as seen at an "infinite distance") from one of the
objects in a binary system will be equal in amplitude and opposite in phase to
the gravitational wave from the other. The net gravitational radiation from the
pair will consist of both longitudinal and transverse waves which are equal in
amplitude. The longitudinal waves will be opposite in phase and shoud therefore
cancel completely. The transverse waves will have a very small phase angle
between them equal to the radius of the orbit(so) involved divided by the
distance to the source.

The transverse waves are only observable if the two objects can be
resolved as separate objects (near field radiation). If they cannot be so
resolved (far field radiation) by the gravitational wave detector, they will be
impossible to detect because the detector will experience only the static field
from their common center of gravity. The cyclical field which for which
detection was hoped for will cancel. A further complication in the detection of
the transverse wave is the fact that they will not produce a 'stretching" of
the local horizontal, they will produce a "tilting" of the local vertical. The
LIGO array should not capable of detecting the effect even if it has sufficinet
amplitude.

The longitudinal waves emanating from the center of gravity of the
emitting system always produce far field radiation which cancels completely. An
additional complication results from the fact that any residual component of
the gravitational radiation is attenuated not only by the expected inverse
square law, it suffers an additional attenuation in proportion to the cube of
distance rather than the square of distance do the transverse waves. It would
seem reasonable to assert that there are no longitudinal waves for LIGO to
detect.

Gravitational waves certainly do exist, we live on a world with an
enormous gravity wave detector, the oceans. The tides in the ocean are produced
by the Moon's gravitational field. The time of high tide advances about an hour
a day. This advancement can be considered to be the output of a gravity wave
detector, but, that gravity wave would be undetectable at interplanetary
distances because the gravitational waves from the Earth and the Moon would
cancel each other virtually completely! The writer has received arguments that
the fact that binary stellar systems are observed to lose energy over time due
to radiation of gravitational energy to the Universe shows that the limitation
described does not occur and that gravitational waves will therefore be
detectible. Such an argument is faulty. The radiating objects are embedded in
the Universe and, as a result, all of the radiated gravitational energy is
absorbed as "near field" radiation. It is only the shrimpy detectors that man
is capable of building which will have difficulty in detecting transverse
gravitational waves. (In addition to the expected attenuation in wave strength
imposed by the inverse square law, the energy received by the far field
detector represented by the LIGO array will be reduced in proportional to the
square of the ratio of the orbital radius of the sources divided by the
distance to the sourced. Rotsa Ruck Fellows!

The source material for this posting may be found in "Gravity" (1987),
"The Einstein Hoax" (1997), and "Corrections to Residual Errors in Special
Relativity (1999) located at http://www.members.aol.com/einsteinhoax/site.htm.
EVERYTHING WHICH WE ACCEPT AS TRUE MUST BE CONSISTENT WITH EVERYTHING ELSE WE
HAVE ACCEPTED AS TRUE, IT MUST BE CONSISTENT WITH ALL OBSERVATIONS, AND IT MUST
BE MATHEMATICALLY VIABLE. PRESENT TEACHINGS DO NOT ALWAYS MEET THIS
REQUIREMENT. THE WORLD IS ENTITLED TO A HIGHER STANDARD OF WORKMANSHIP FROM
THOSE IT HAS GRANTED WORLD CLASS STATUS.

Please make any response via E-mail as Newsgroups are not monitored on a
regular basis. Objective responses will be treated with the same courtesy as
they are presented. To prevent the wastage of time on both of our parts, please
do not raise objections that are not related to material that you have read at
the Website. This posting is merely a summary.

E-mail:- einsteinhoax@aol.com

The material at the Website has been posted continuously for over 5 years.
In that time THERE HAVE BEEN NO OBJECTIVE REBUTTALS OF ANY OF THE MATERIAL
PRESENTED. There have only been hand waving arguments by individuals who have
mindlessly accepted the prevailing wisdom without questioning it. If anyone
provides a significant rebuttal that cannot be objectively answered, the
material at the Website will be withdrawn.
G=EMC^2 Glazier
Posted: Wed Mar 03, 2004 4:14 pm
Guest
Hi Sam LIGO will find no gravity waves. I know because my theory of
gravity is so good this helps prove it. Bert
Gregory L. Hansen
Posted: Wed Mar 03, 2004 4:14 pm
Guest
In article <982-40466067-73@storefull-3178.bay.webtv.net>,
G=EMC^2 Glazier <herbertglazier@webtv.net> wrote:
Quote:
Hi Sam LIGO will find no gravity waves. I know because my theory of
gravity is so good this helps prove it. Bert



Well, that's settled. We can move on to the next problem now.


--
"'No user-serviceable parts inside.' I'll be the judge of that!"
Sam Wormley
Posted: Wed Mar 03, 2004 4:17 pm
Guest
Gnigdrib wrote:
Quote:

Will the LIGO Experiment Work?



Most likely LIGO will detect gravitational waves.
See: http://www.ligo.caltech.edu/
http:/www.edu-observatory.org/eo/cosmology.html

PHYSICS NEWS UPDATE
The American Institute of Physics Bulletin of Physics News
Number 632 April 9, 2003 by Phillip F. Schewe, Ben Stein, and James
Riordon

FIRST LIGO SCIENTIFIC RESULTS. With two controlling partners, MIT and
Caltech, and two branch offices (two completely independent detectors)
located in Washington State and Louisiana, the Laser Interferometer
Gravitational-Wave Observatory (LIGO) is essentially a giant strain gauge.
In the LIGO setup laser light reflects repeatedly in each of two
perpendicularly oriented 4-km-long pipes. A passing gravity wave will
distort the local spacetime, stretching very slightly one of the paths while
shrinking the other, causing the interference pattern of the two merging
laser light beams to shift in a characteristic way. LIGO does not measure
static gravitational fields, such as those from the sun or the Earth itself.
Rather it strives to see ripples in spacetime radiated by such events as
the inspiral of two neutron stars toward each other, a phenomenon which
would typically produce a strain in the LIGO apparatus as large as one part
in 10^20. That is, a passing gravity wave is expected to change the
distance between mirrors some 4 km apart by about 10^-18 meters, a
displacement 1000 times smaller than a proton. Such a measurement
represents a physics and engineering feat of great delicacy. But at long
last the LIGO team has prepared its instrument and at this week's APS
meeting, reported its first official results from the initial "science" run
conducted over 17 days in September 2002.
In this first run no gravitational wave events were observed, but palpable
knowledge was gained as to what the sky should look like when viewed in the
form of gravity waves. So great is LIGO's sensitivity that it has been able
to set the best upper limit on the output of gravitational waves from three
of the four prime source categories. These four expected waveforms are as
follows: bursts from sources such as supernovas or gamma bursters; chirps
from inspiraling objects such as coalescing binary stars; periodic signals,
perhaps from sources like spherically asymmetric pulsars; and a stochastic
background source arising from gravity waves originating from the big bang
itself. LIGO deputy director Gary Sanders (Caltech,
sanders_g@ligo.caltech.edu) said that in three of these four categories,
had set new upper limits on the rate at which gravitational waves were being
produced. In the coalescing binary category, for instance, LIGO has
established an upper limit of 164 per year from the Milky Way, a factor of
26 better than the previous limit. Erik Katsavounidis (MIT,
kats@ligo.mit.edu) said that LIGO could establish an upper limit on
periodic signals from bright pulsars with a sensitivity of about 10^-22.
Sheila Rowan (Stanford Univ and Univ Glasgow) spoke of future operations at
LIGO. First of all, the second scientific run currently underway will be
some ten times more sensitive than the first run, the one being reported at
the meeting. If in the first science run LIGO was essentially sensitive to
gravity waves from the whole of the Milky Way, then in the second science
run (conducted Feb-Apr 2003), featuring a ten-times improvement in
sensitivity, the region of space patrolled would effectively reach out to
about 15 million light years, a realm that includes the nearby Andromeda
galaxy. (For more information about LIGO and a complete collaboration list,
see www.ligo.caltech.edu ) In its search for gravity waves, LIGO (which with
about 440 scientists is as big as the large particle physics experiments
underway at accelerators) is also collaborating with other interferometer
devices such as GEO (in Germany, www.geo600.uni-hannover.de ) and TAMA
(Japan).


Crank Information
http://groups.google.com/groups?q=group%3Asci.physics+author%3Areticher
http://groups.google.com/groups?q=group%3Asci.physics+author%3Areticher1
Uncle Al
Posted: Wed Mar 03, 2004 5:48 pm
Guest
Gnigdrib wrote:
Quote:

Will the LIGO Experiment Work?
[snip ignorant crap]


It's up and running, you idiot.

Psychotic ineducable boring spammer retic (Ernest Wittke),

You see yourself this way,
http://www.mazepath.com/uncleal/effete6.jpg
The entire remainder of the planet sees you this way,
http://www.mazepath.com/uncleal/effete3.png

http://b5.sdvc.uwyo.edu/bab5/snds/argcstpd.wav
http://w0rli.home.att.net/youare.swf
http://www.mazepath.com/uncleal/sunshine.jpg
http://www.you-moron.com/
http://groups.google.com/groups?q=group%3Asci.physics+author%3Awittke
http://www.mazepath.com/uncleal/effete0.jpg
http://www.mazepath.com/uncleal/effete1.png
http://www.mazepath.com/uncleal/effete2.png
http://www.mazepath.com/uncleal/effete3.png
http://www.mazepath.com/uncleal/effete4.png
http://www.mazepath.com/uncleal/effete5.jpg

http://www.apa.org/journals/psp/psp7761121.html
http://insti.physics.sunysb.edu/~siegel/quack.html
<http://www.firehead.org/~jessh/film/kubrick/Kubrick-Psycho.html>
<http://www.naturalchild.com/elliott_barker/prisons.html>

Quote:
The source material for this posting may be found in "Gravity" (1987),
"The Einstein Hoax" (1997), and "Corrections to Residual Errors in Special
Relativity (1999)
[snip]


Hey, stooopid spammer Ernest Wittke - Do you want EVIDENCE? Each of
the 24 GPS satellites carries either four cesium atomic clocks or
three rubidum atomic clocks in orbit, with full relativistic
corrections being applied.

http://arXiv.org/abs/hep-th/0307140
GR structure, especially Part 4/p. 7
<http://rattler.cameron.edu/EMIS/journals/LRG/Articles/Volume4/2001-4will/index.html>
Experimental constraints on General Relativity.
<http://tycho.usno.navy.mil/ptti/ptti2002/paper20.pdf>
Nature 425 374 (2003)
<http://rattler.cameron.edu/EMIS/journals/LRG/Articles/Volume6/2003-1ashby/index.html>
http://www.eftaylor.com/pub/projecta.pdf
Relativity in the GPS system
http://arXiv.org/abs/gr-qc/9909014
falling light
http://www.hawaii.edu/suremath/SRtwinParadox.html
<http://physics.syr.edu/courses/modules/LIGHTCONE/twins.html>
Twin Paradox
Science 303(5661) 1143;1153 (2004)
http://arXiv.org/abs/astro-ph/0401086
http://arxiv.org/abs/astro-ph/0312071
Deeply relativistic neutron star binaries
http://arXiv.org/abs/gr-qc/0301024
Nordtvedt Effect

Special Relativity is physics on a topologically trivial Lorentzian
manifold with a metric whose curvature tensor is zero. This is a
perfectly diffeomorphism-invariant condition and does not require
any particular coordinate choice. It is invariant under
the full group of diffeomorphisms. The Poincare group is
the group of *isometries* of the metric in special relativity.

The Special Relativity metric is *non-dynamical* (unlike GR). It
defines the coupling *constants* of your theory. If you change the
metric in any nontrivial way you are changing your theory. An
operation can only be called a "symmetry" of a special-relativistic
(non-gravitational) theory if it preserves the metric, and therefore
the symmetry of special-relativistic theories is the Poincare group
only. General Relativity (gravitation) has a dynamic metric.

NIM A 355 537 (1995)
Physics Letters B 328 103 (1994)
Physical Review Letters 64 1697 (1990)
Physical Review Letters 39 1051 (1977)
Physical Review 135 B1071 (1964)
Physics Letters 12 260 (1964)
Europhysics Letters 56(2) 170-174 (2001)
General Relativity and Gravitation 34(9) 1371 (2002)

http://fourmilab.to/etexts/einstein/specrel/specrel.pdf
<http://www.geocities.com/physics_world/sr/ae_1905_error.htm>
<http://www.physics.gatech.edu/people/faculty/finkelstein/relativity.pdf>
http://users.powernet.co.uk/bearsoft/Paper6.pdf
http://users.powernet.co.uk/bearsoft/LPHrel.html
Longitudinal and transverse mass

http://www.navcen.uscg.gov/pubs/gps/gpsuser/gpsuser.pdf
http://www.navcen.uscg.gov/pubs/gps/sigspec/default.htm
http://www.navcen.uscg.gov/pubs/gps/icd200/default.htm
http://www.trimble.com/gps/index.html
http://sirius.chinalake.navy.mil/satpred/
http://www.phys.lsu.edu/mog/mog9/node9.html
http://egtphysics.net/GPS/RelGPS.htm
http://www.schriever.af.mil/gps/Current/current.oa1
http://edu-observatory.org/gps/gps_books.html
<http://www-astronomy.mps.ohio-state.edu/~pogge/Ast162/Unit5/gps.html>

Quote:
If anyone
provides a significant rebuttal that cannot be objectively answered, the
material at the Website will be withdrawn.

Right, like your head has ever been withdrawn from your ass - even
when you shit.

--
Uncle Al
http://www.mazepath.com/uncleal/
(Toxic URL! Unsafe for children and most mammals)
"Quis custodiet ipsos custodes?" The Net!
 
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