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Article #3737Re: That Great Pulsar Timing Flame War
From: Loren I. Petrich
Date: Mon, 11 Jan 1993 05:04
Date: Mon, 11 Jan 1993 05:04
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4747 bytes
In article <1993Jan9.203021.10884@Princeton.EDU> steve@puppsr.princeton.edu writes: >In article <C0IoBJ.4x8@well.sf.ca.us>, metares@well.sf.ca.us (Tom Van Flandern) writes: > : lip@s1.gov (Loren I. Petrich) writes: : > So, we have the following parameters all from observation: : > - The projected semimajor axis a1*sin(i) : > - The period P : > - Its first derivative dP/dt [*] : > - The eccentricity e : > - The periapsis angle omega : > - Its rate of change d(omega)/dt [*] : > - The redshift parameter gamma = sqrt(a/m)*(mc*(mp+2*mc)/m^2)*e [*] : The three parameters I have marked with [*] actually form a single : solution parameter, according to Taylor and Damour. There is insufficient : observational power to separate them. The masses and orbit must be : determined from observations along with this single relativistic parameter. : So the relationship between the three components of the relativistic : parameter must be set by theory, since it cannot be measured by observations. >As Loren has already pointed out, this is not correct. [detailed explanation followed...] I'm glad to see that someone else agrees with me on this subject :-) [About consistency with GR, Brans-Dicke (scalar-tensor) theory, and Damour's biscalar-tensor theorie...] ...No >matter how good the test becomes, as the data continues to come in, you >can always sneak through this alternative theory by making the small >parameters smaller. Certainly correct, and it does not support van Flandern's contention of serious departures from GR being in evidence. >Note this is not the end of the story with binary pulsars. As Taylor and >others pointed out in a Nature article recently, PSR~B1534+12 offers >a new "test" which uses Shapiro time delay measurements rather than >P_b_dot and is thus "nonradiative", and useful in squeezing on a >different set of alternative theories. [Exactly what is the article?] The Shapiro time delay in the isotropic PPN gauge is 2*(1+gamma)*mc*log(r0/(r + n.r)) where gamma is a PPN parameter, mc is the companion mass, r is the separation from the companion to the pulsar, and n is the direction to the observer. Note: gamma = 1 from GR and is constrained to within 10^-3 by Solar System experiments. There are additional effects that manifest themselves as eccentricity offsets; these have sizes of [2*(1+gamma)*mc - mp*mc*(mp+2*mc)/m^2]*e*sin(i) and [2*(1+gamma)*mc - mp*mc^2/m^2]*e*sin(i) The sizes of these effects are essentially independent of the orbit's size, and are, for mp = mc = 1.4 solar masses, 4*mc = 28 microseconds mp*mc*(mp+2*mc)/(2*m^2) = 2.7 microseconds mp*mc^2/(2*m^2) = 0.9 microseconds How good is the timing accuracy for PSR~B1534+12? These estimates suggest that one needs accuracies of at least a few microseconds to get good results on these effects. >As a scientist working in the field, let me restate my own opinion, >offered some weeks ago. Taylor and Weisberg, in their observations of >the binary pulsar PSR~B1913+16, have demonstrated the existence of >gravity waves beyond any real doubt. The fact is that a prediction of >an orbital decay rate due to the loss of energy and angular momentum >into gravitational radiation was made, and the measurement was done and >the results matched to better than 1%. Any serious claim against GR >or gravitational waves must now reproduce this result in a natural >way. I am all in favor of the continued exploration of alternative >models, done so well recently by Damour. My PhD thesis included much >discussion of alternative models. Someday the real limits of GR will >be reached, and it will be quantized and perhaps folded into a GUT, and >I believe this explorations of the underpinning of GR may show the >way. But in the meantime, there is no reason to believe that the >"standard model" is incorrect. One interesting question about GUT's that include gravity is whether they predict any Brans-Dicke-like effects, any field dependencies of the gravitational constant. I don't recall any discussion of this question in any of the GUT literature I have read. -- /Loren Petrich, the Master Blaster /lip@s1.gov
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Newsgroups: sci.astro,sci.physics Path: arc1-ca.pugleaf.net!sparky!uunet!gatech!usenet.ins.cwru.edu!agate!overload.lbl.gov!s1.gov!lip From: lip@s1.gov (Loren I. Petrich) Subject: Re: That Great Pulsar Timing Flame War Message-ID: <1993Jan11.050428.25805@s1.gov> Sender: usenet@s1.gov Nntp-Posting-Host: s1.gov Organization: LLNL References: <1993Jan8.010157.13539@s1.gov> <C0IoBJ.4x8@well.sf.ca.us> <1993Jan9.203021.10884@Princeton.EDU> Date: Mon, 11 Jan 1993 05:04:28 GMT Lines: 100