Changes

#:The topology of wormholes is an interesting topic, widely discussed among theoretical physicists and mathematicians.  There is much speculation about what they would be like (if they could exist at all under quantum gravity), and what kind of "cosmic censorship" or "chronology protection" theorems might make practical time travel impossible.  The nature of these theorems seems to be intertwined with theories of quantum gravity and "grand unification", so the exact form of the "cosmic censorship", if it exists, can't be known until quantum mechanics and relativistic geometry are unified.  It is an exciting field of research.  No one believes that the "cosmic censorship" will take the form of relativity not being a true non-quantum approximation to reality.

#:The topology of wormholes is an interesting topic, widely discussed among theoretical physicists and mathematicians.  There is much speculation about what they would be like (if they could exist at all under quantum gravity), and what kind of "cosmic censorship" or "chronology protection" theorems might make practical time travel impossible.  The nature of these theorems seems to be intertwined with theories of quantum gravity and "grand unification", so the exact form of the "cosmic censorship", if it exists, can't be known until quantum mechanics and relativistic geometry are unified.  It is an exciting field of research.  No one believes that the "cosmic censorship" will take the form of relativity not being a true non-quantum approximation to reality.

#''The theory predicts natural formation of highly ordered (and thus low entropy) black holes despite the increase in entropy required by the Second Law of Thermodynamics.''

#''The theory predicts natural formation of highly ordered (and thus low entropy) black holes despite the increase in entropy required by the Second Law of Thermodynamics.''

#:(not done yet)

#: Since the 70's much works has been done on the subject of black hole thermodynamics <ref>http://adsabs.harvard.edu/abs/1973CMaPh..31..161B</ref><ref>http://arxiv.org/pdf/gr-qc/9307035v1.pdf</ref>, most notably by the Lucasian Professorship of Mathematics at Cambridge [[Stephen Hawking]]. When quantum field theory is added to the analysis of black holes it is found that they do not possess "low entropy" (quite the opposite, in fact) and are consistent with the laws of thermodynamics <ref>http://adsabs.harvard.edu/abs/1973PhRvD...7.2333B</ref>. The [[Counterexamples to Relativity]] article has labelled this work in a footnote as "[c]ontrived explanations", with no explanation for this characterization given.

#''Data from the PSR B1913+16 increasingly diverge from predictions of the General Theory of Relativity such that, despite a Nobel Prize in Physics being awarded for early work on this pulsar, no data at all have been released about it for over five years.''

#''Data from the PSR B1913+16 increasingly diverge from predictions of the General Theory of Relativity such that, despite a Nobel Prize in Physics being awarded for early work on this pulsar, no data at all have been released about it for over five years.''

#:Please read the cited paper carefully.  It is a survey of their observations over a 30 year period.  They point out that their data matches general relativity to within 0.2 percent, and is now down in the "noise" of other effects, such as lack of accurate knowledge of just how far away the pulsars are, and lack of accurate knowledge of galactic constants.  As they say in the abstract, "tighter bounds will be difficult to obtain."  The paper, written in 2004, also notes that, because the pulsar beams are slowly tilting out of the line of sight to Earth, "A core component [of the emission] is quite prominent in the data taken in 1980-81, but it faded very significantly between 1980 and 1998 and was nearly gone by 2003."

#:Please read the cited paper carefully.  It is a survey of their observations over a 30 year period.  They point out that their data matches general relativity to within 0.2 percent, and is now down in the "noise" of other effects, such as lack of accurate knowledge of just how far away the pulsars are, and lack of accurate knowledge of galactic constants.  As they say in the abstract, "tighter bounds will be difficult to obtain."  The paper, written in 2004, also notes that, because the pulsar beams are slowly tilting out of the line of sight to Earth, "A core component [of the emission] is quite prominent in the data taken in 1980-81, but it faded very significantly between 1980 and 1998 and was nearly gone by 2003."