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{{Short description|Physics conference of 1957}}
The '''Conference on the Role of Gravitation in Physics''', also known as the '''Chapel Hill Conference''', was an invitation-only [[scientific conference]] held at [[Chapel Hill, North Carolina]], United States from January 18 to January 23, 1957. It discussed experimental proposals to tfind [[gravitational wave]]s and discussed ways to find a theory of [[quantum gravity]]. It was also one of the first large conferences to discuss the [[many-worlds interpretation]].

The '''Conference on the Role of Gravitation in Physics''', better known as the '''Chapel Hill Conference''' or '''GR1''', was an invitation-only international [[scientific conference]] held at [[Chapel Hill, North Carolina]], United States from January 18 to January 23, 1957. It discussed topics in [[general relativity]], including the possible existence of [[gravitational wave]]s and ways to find a theory of [[quantum gravity]]. It was also the first conference were the [[many-worlds interpretation]] was discussed. After the Chapel Hill Conference, conferences on general relativity and gravitation became frequent.

Historian [[Dean Rickles]] has suggested that the Chapel Hill Conference did for general relativity what the 1947 [[Shelter Island Conference]] did for [[quantum field theory]] in reviving the field with a younger generation of physicists.<ref name=":3" />


== Organization ==
== Organization ==
The conference was organized by the Institute of Field Physics established a year before the conference in the [[University of North Carolina at Chapel Hill]] by physicists [[Cécile DeWitt-Morette]] and [[Bryce DeWitt]].<ref name=":0">{{Cite book |title=The Role of Gravitation in Physics: Report from 1957 Chapel Hill Conference |date=2017 |publisher=Edition Open Access |editor-last=DeWitt |editor-first=Cécile M. |editor-last2=Dicke |editor-first2=Dean}}</ref> The institute was financed by bussinessmen Agnew Bahson and [[Roger Babson]].<ref name=":0" /> The later had founded the [[Gravity Research Foundation]] for looking into [[anti-gravity]] research.<ref name=":0" />
The conference was organized by the Institute of Field Physics established a year before the conference in the [[University of North Carolina at Chapel Hill]]. The institute was financed by industrialist [[Agnew Hunter Bahnson]].<ref name=":3">{{Citation |last=Rickles |first=Dean |title=The Chapel Hill Conference in Context |date=2011-02-14 |work=The Role of Gravitation in Physics: Report from the 1957 Chapel Hill Conference |url=https://edition-open-sources.org/sources/5/3/index.html |access-date=2024-12-16 |series=EOS Sources |place=Berlin |publisher=Max-Planck-Gesellschaft zur Förderung der Wissenschaften |language=english |isbn=978-3-945561-29-4}}</ref>


Aside from the DeWitts, in the steering comittee there was also [[Frederik Belinfante]], [[Peter Bergmann]], [[Freeman Dyson]] and [[John Archibald Wheeler]].<ref name=":0" />
The conference was organized by physicists [[Cécile DeWitt-Morette]] and [[Bryce DeWitt]]. Aside from the DeWitts, in the steering committee there was also [[Frederik Belinfante]], [[Peter Bergmann]], [[Freeman Dyson]] and [[John Archibald Wheeler]].<ref name=":0" />


The conference was divided into 4 sessions on unquantized general relativity, a single session on cosmology, and 3 sessions on quantum gravity.<ref name=":0" />
== Energy of gravitational waves ==
During the conference, the nature of gravitational waves and their ability to transfer energy was discussed. [[Richard Feynman]] remembers <ref name="Preskill">Preskill, John and Kip S. Thorne. Foreword to ''Feynman Lectures On Gravitation''. Feynman et al. (Westview Press; 1st ed. (June 20, 2002) p. xxv–xxvi.[http://www.theory.caltech.edu/~preskill/pubs/preskill-1995-feynman.pdf Link PDF (page 17-18)]</ref>


The Chapel Hill Conference is considered part a still on-going series of modern conferences on gravitation, sometimes referred as GR''n.''<ref>{{Cite web |title=The GRn conferences |url=http://www.isgrg.org/pastconfs.php |access-date=17 December 2024 |website=International Society on General Relativity and Gravitation}}</ref> Chapel Hill Conference succeeded the 1955 Bern Conference held in the 50th anniversary of general relativity, the first ever conference focused entirely on the topic of gravitation. The Bern Conference was referred popularly as the GR0, while the Chapel Hill Conference was considered the GR1.<ref name=":4">{{Cite book |last=DeWitt-Morette |first=Cécile |url=https://books.google.com/books?id=kz0_jin-9XAC&dq=1957+chapel+hill+dewitt&pg=PA87 |title=The Pursuit of Quantum Gravity: Memoirs of Bryce DeWitt from 1946 to 2004 |date=2011-02-15 |publisher=Springer Science & Business Media |isbn=978-3-642-14270-3 |language=en}}</ref><ref name=":3" />
{{Quote|text=I was surprised to find a whole day at the conference devoted to this question, and that ‘experts’ were confused. That is what comes from looking for conserved energy tensors, etc. instead of asking ‘can the waves do work?}}


== Discussed topics ==
Feynman suggested during the conference the [[sticky bead argument]] which intuitively demonstrated that gravitational waves must carry energy.<ref name="Preskill" /> This argument was published by [[Hermann Bondi]] right after the conference.<ref name="Preskill" />

=== Lack of new experiments ===
After the introductory lecture by Wheeler, [[Robert H. Dicke]] reviewed the experimental [[tests of general relativity]]. He concluded that there was no much progress, he contrasted it with quantum mechanics:<ref>{{Cite book |last=Peebles |first=P. J. E. |url=https://books.google.com/books?id=kjVVEAAAQBAJ&dq=dicke+chapel+hill+1957&pg=PT59 |title=The Whole Truth: A Cosmologist's Reflections on the Search for Objective Reality |date=2022-08-02 |publisher=Princeton University Press |isbn=978-0-691-23136-5 |language=en}}</ref>
{{Quote|text=It is unfortunate to note that the situation with respect to the experimental checks of general relativity theory is not much better than it was a few years after the theory was discovered - say in 1920. This is in striking contrast to the situation with respect to quantum theory, where we have literally thousands of experimental checks... Professor Wheeler has already discussed the three famous checks of general relativity; this is really very flimsy evidence on which to hang a theory.}}
Dicke discussed the [[Eötvös experiment]] and provided ideas for further experiments.<ref>{{Cite journal |last=Bergmann |first=Peter G. |date=1957 |title=Summary of the Chapel Hill Conference |url=https://journals.aps.org/rmp/abstract/10.1103/RevModPhys.29.352 |journal=Reviews of Modern Physics |volume=29 |issue=3 |pages=352–354 |doi=10.1103/RevModPhys.29.352}}</ref>

=== Gravitational waves ===
During the conference, the nature of gravitational waves and their ability to transfer energy was discussed. [[Richard Feynman]] remembers<ref name="Preskill">Preskill, John and Kip S. Thorne. Foreword to ''Feynman Lectures On Gravitation''. Feynman et al. (Westview Press; 1st ed. (June 20, 2002) p. xxv–xxvi.[http://www.theory.caltech.edu/~preskill/pubs/preskill-1995-feynman.pdf Link PDF (page 17-18)]</ref>

{{Quote|text="I was surprised to find a whole day at the conference devoted to this question, and that ‘experts’ were confused. That is what comes from looking for conserved energy tensors, etc. instead of asking ‘can the waves do work?"}}

[[Felix Pirani]] presented for the first time how to mathematically treat gravitational waves using the [[geodesic deviation]] introduced by [[John Lighton Synge]].<ref name=":2">{{Cite book |last1=Goenner |first1=Hubert |url=https://books.google.com/books?id=5mGZno8CvnQC&dq=Chapel+Hill+Conference+1957+gravitational+waves&pg=PA219 |title=The Expanding Worlds of General Relativity |last2=Renn |first2=Jürgen |last3=Ritter |first3=Jim |last4=Sauer |first4=Tilman |date=1998-12-01 |publisher=Springer Science & Business Media |isbn=978-0-8176-4060-6 |language=en}}</ref> He showed how two masses would move relative from each other from ripples in [[spacetime]].<ref name=":2" /> Based on Pirani's argument, Feynman suggested during the conference the [[sticky bead argument]] which intuitively demonstrated that gravitational waves must carry energy.<ref name="Preskill" /><ref>{{Cite book |last=Feynman |first=Richard |url=https://books.google.com/books?id=AEtnDwAAQBAJ&dq=1957+chapel+hill+conference&pg=PT19 |title=Feynman Lectures On Gravitation |date=2018-05-04 |publisher=CRC Press |isbn=978-0-429-98248-4 |language=en}}</ref><ref name=":2" /> A version of this argument was published by [[Hermann Bondi]] right after the conference.<ref name="Preskill" />

=== Wormholes ===
During the conference, Wheeler coined the term [[wormhole]].<ref>{{Cite web |title=Section III |url=https://physics.unc.edu/home/department-history/section-iii/ |access-date=2024-12-16 |website=Department of Physics and Astronomy |language=en-US}}</ref>

=== Numerical relativity ===
When discussing the presentations of [[Yvonne Choquet-Bruhat|Yvonne Fourès-Bruhat]] and [[Charles W. Misner]], Bruce DeWitt pointed out the importance of using computers to solve [[Einstein field equations]]. This line of research led to the development of [[numerical relativity]].<ref>{{Cite journal |last1=Cervantes-Cota |first1=Jorge L. |last2=Galindo-Uribarri |first2=Salvador |last3=Smoot |first3=George F. |date=2016 |title=A Brief History of Gravitational Waves |journal=Universe |language=en |volume=2 |issue=3 |pages=22 |doi=10.3390/universe2030022 |doi-access=free |arxiv=1609.09400 |bibcode=2016Univ....2...22C |issn=2218-1997}}</ref><ref name=":4" />

=== Many-worlds interpretation ===
The relative state formulation, better known today as the [[many-worlds interpretation]] of quantum mechanics, was being developed by [[Hugh Everett III]], a student of Wheeler, who submitted an edited version of his thesis for the conference but did not attend.<ref name=":1">{{Cite book |last=Byrne |first=Peter |url=https://books.google.com/books?id=dqgqPjqIyJoC&dq=The+Many+Worlds+of+Hugh+Everett+III+chapel+hill&pg=PT278 |title=The Many Worlds of Hugh Everett III: Multiple Universes, Mutual Assured Destruction, and the Meltdown of a Nuclear Family |date=2012-12-13 |publisher=OUP Oxford |isbn=978-0-19-165522-7 |language=en}}</ref> The paper was well received by Bryce DeWitt.<ref name=":1" /> Wheeler and [[Charles W. Misner]] presented some of Everett's ideas near the end of the conference.<ref name=":1" /> Feynman publicly criticized the idea of an [[universal wavefunction]], suggested by Wheeler, saying<ref name=":1" />

{{Quote|text="The concept of a 'universal wave function' has serious difficulties. This is so since the function must contain amplitudes for all possible worlds depending upon all quantum mechanical possibilities in the past and thus one is forced to believe in the equal reality of an infinity of possible worlds."}}

Everett's paper was published in the proceedings of the conference.<ref name=":1" />


== List of participants ==
== List of participants ==
The list of participants according to DeWitt-Morette report is:<ref name=":0">{{Cite book |url=https://edition-open-sources.org/sources/5/index.html |title=The Role of Gravitation in Physics: Report from 1957 Chapel Hill Conference |series=EOS – Sources |date=2017 |publisher=Edition Open Access |isbn=978-3-945561-29-4 |editor-last=DeWitt |editor-first=Cécile M. |editor-last2=Dicke |editor-first2=Dean}}</ref>{{columns-list|colwidth=30em|
{{columns-list|colwidth=30em|
* From United States:
* From United States:
** [[James Leroy Anderson]] (born 1926)
** [[James Leroy Anderson]] (born 1926)
Line 22: Line 50:
** [[Peter Bergmann]]
** [[Peter Bergmann]]
** [[Dieter R. Brill]] (born 1933)
** [[Dieter R. Brill]] (born 1933)
** [[Michael J. Buckingham]] (born 1933)
** [[Michael J. Buckingham]] (born 1927)
** [[William R. Davis]]
** [[William R. Davis]] (PhD in 1956)
** [[Bryce DeWitt]]
** [[Bryce DeWitt]]
** [[Cécile DeWitt-Morette]]
** [[Cécile DeWitt-Morette]]
Line 32: Line 60:
** [[Joshua N. Goldberg]]
** [[Joshua N. Goldberg]]
** [[Arthur Lilley]] (born 1928)
** [[Arthur Lilley]] (born 1928)
** [[Richard Lindquist|Richard W. Lindquist]]
** [[Richard W. Lindquist]] (PhD in 1962)
** [[Charles W. Misner]]
** [[Charles W. Misner]]
** [[Raymond Mjolsness]]
** [[Raymond Mjolsness]] (PhD in 1963)
** [[Ezra T. Newman]]
** [[Ezra T. Newman]]
** [[Alfred Schild]]
** [[Alfred Schild]]
** [[Ralph S. Schiller]]
** [[Ralph S. Schiller]]
** [[Joseph Weber]]
** [[Joseph Weber]]
** [[John Archibald Wheeler]]
** [[John Archibald Wheeler]]
Line 47: Line 75:
** [[Dennis W. Sciama]]
** [[Dennis W. Sciama]]
* From France:
* From France:
** [[Yvonne Choquet-Bruhat|Yvonne Fourès]]
** [[Yvonne Choquet-Bruhat|Yvonne Fourès-Bruhat]]
** [[André Lichnerowicz]]
** [[André Lichnerowicz]]
** [[Marie-Antoinette Tonnelat]]
** [[Marie-Antoinette Tonnelat]]
Line 53: Line 81:
** [[Helmut Salecker]]
** [[Helmut Salecker]]
* From Japan:
* From Japan:
** [[Ryoyu Utiyama]]
** {{ill|Ryoyu Utiyama|de}}
* From Denmark:
* From Denmark:
** [[Stanley Deser]]
** [[Stanley Deser]] (born 1931)
* From Sweden
* From Sweden
** [[Bertel Laurent]]
** [[Bertel Laurent]]
* From Turkey
* From Turkey
** [[Behram Kurşunoğlu]]
** [[Behram Kurşunoğlu]]
}}[[Nathan Rosen]] was invited but did not participate.
}}


==References==
==References==
{{reflist}}
{{reflist}}

[[Category:Physics conferences]]
[[Category:1957 in science]]

Latest revision as of 05:51, 28 December 2024

The Conference on the Role of Gravitation in Physics, better known as the Chapel Hill Conference or GR1, was an invitation-only international scientific conference held at Chapel Hill, North Carolina, United States from January 18 to January 23, 1957. It discussed topics in general relativity, including the possible existence of gravitational waves and ways to find a theory of quantum gravity. It was also the first conference were the many-worlds interpretation was discussed. After the Chapel Hill Conference, conferences on general relativity and gravitation became frequent.

Historian Dean Rickles has suggested that the Chapel Hill Conference did for general relativity what the 1947 Shelter Island Conference did for quantum field theory in reviving the field with a younger generation of physicists.[1]

Organization

[edit]

The conference was organized by the Institute of Field Physics established a year before the conference in the University of North Carolina at Chapel Hill. The institute was financed by industrialist Agnew Hunter Bahnson.[1]

The conference was organized by physicists Cécile DeWitt-Morette and Bryce DeWitt. Aside from the DeWitts, in the steering committee there was also Frederik Belinfante, Peter Bergmann, Freeman Dyson and John Archibald Wheeler.[2]

The conference was divided into 4 sessions on unquantized general relativity, a single session on cosmology, and 3 sessions on quantum gravity.[2]

The Chapel Hill Conference is considered part a still on-going series of modern conferences on gravitation, sometimes referred as GRn.[3] Chapel Hill Conference succeeded the 1955 Bern Conference held in the 50th anniversary of general relativity, the first ever conference focused entirely on the topic of gravitation. The Bern Conference was referred popularly as the GR0, while the Chapel Hill Conference was considered the GR1.[4][1]

Discussed topics

[edit]

Lack of new experiments

[edit]

After the introductory lecture by Wheeler, Robert H. Dicke reviewed the experimental tests of general relativity. He concluded that there was no much progress, he contrasted it with quantum mechanics:[5]

It is unfortunate to note that the situation with respect to the experimental checks of general relativity theory is not much better than it was a few years after the theory was discovered - say in 1920. This is in striking contrast to the situation with respect to quantum theory, where we have literally thousands of experimental checks... Professor Wheeler has already discussed the three famous checks of general relativity; this is really very flimsy evidence on which to hang a theory.

Dicke discussed the Eötvös experiment and provided ideas for further experiments.[6]

Gravitational waves

[edit]

During the conference, the nature of gravitational waves and their ability to transfer energy was discussed. Richard Feynman remembers[7]

"I was surprised to find a whole day at the conference devoted to this question, and that ‘experts’ were confused. That is what comes from looking for conserved energy tensors, etc. instead of asking ‘can the waves do work?"

Felix Pirani presented for the first time how to mathematically treat gravitational waves using the geodesic deviation introduced by John Lighton Synge.[8] He showed how two masses would move relative from each other from ripples in spacetime.[8] Based on Pirani's argument, Feynman suggested during the conference the sticky bead argument which intuitively demonstrated that gravitational waves must carry energy.[7][9][8] A version of this argument was published by Hermann Bondi right after the conference.[7]

Wormholes

[edit]

During the conference, Wheeler coined the term wormhole.[10]

Numerical relativity

[edit]

When discussing the presentations of Yvonne Fourès-Bruhat and Charles W. Misner, Bruce DeWitt pointed out the importance of using computers to solve Einstein field equations. This line of research led to the development of numerical relativity.[11][4]

Many-worlds interpretation

[edit]

The relative state formulation, better known today as the many-worlds interpretation of quantum mechanics, was being developed by Hugh Everett III, a student of Wheeler, who submitted an edited version of his thesis for the conference but did not attend.[12] The paper was well received by Bryce DeWitt.[12] Wheeler and Charles W. Misner presented some of Everett's ideas near the end of the conference.[12] Feynman publicly criticized the idea of an universal wavefunction, suggested by Wheeler, saying[12]

"The concept of a 'universal wave function' has serious difficulties. This is so since the function must contain amplitudes for all possible worlds depending upon all quantum mechanical possibilities in the past and thus one is forced to believe in the equal reality of an infinity of possible worlds."

Everett's paper was published in the proceedings of the conference.[12]

List of participants

[edit]

The list of participants according to DeWitt-Morette report is:[2]

Nathan Rosen was invited but did not participate.

References

[edit]
  1. ^ a b c Rickles, Dean (2011-02-14), "The Chapel Hill Conference in Context", The Role of Gravitation in Physics: Report from the 1957 Chapel Hill Conference, EOS – Sources, Berlin: Max-Planck-Gesellschaft zur Förderung der Wissenschaften, ISBN 978-3-945561-29-4, retrieved 2024-12-16
  2. ^ a b c DeWitt, Cécile M.; Dicke, Dean, eds. (2017). The Role of Gravitation in Physics: Report from 1957 Chapel Hill Conference. EOS – Sources. Edition Open Access. ISBN 978-3-945561-29-4.
  3. ^ "The GRn conferences". International Society on General Relativity and Gravitation. Retrieved 17 December 2024.
  4. ^ a b DeWitt-Morette, Cécile (2011-02-15). The Pursuit of Quantum Gravity: Memoirs of Bryce DeWitt from 1946 to 2004. Springer Science & Business Media. ISBN 978-3-642-14270-3.
  5. ^ Peebles, P. J. E. (2022-08-02). The Whole Truth: A Cosmologist's Reflections on the Search for Objective Reality. Princeton University Press. ISBN 978-0-691-23136-5.
  6. ^ Bergmann, Peter G. (1957). "Summary of the Chapel Hill Conference". Reviews of Modern Physics. 29 (3): 352–354. doi:10.1103/RevModPhys.29.352.
  7. ^ a b c Preskill, John and Kip S. Thorne. Foreword to Feynman Lectures On Gravitation. Feynman et al. (Westview Press; 1st ed. (June 20, 2002) p. xxv–xxvi.Link PDF (page 17-18)
  8. ^ a b c Goenner, Hubert; Renn, Jürgen; Ritter, Jim; Sauer, Tilman (1998-12-01). The Expanding Worlds of General Relativity. Springer Science & Business Media. ISBN 978-0-8176-4060-6.
  9. ^ Feynman, Richard (2018-05-04). Feynman Lectures On Gravitation. CRC Press. ISBN 978-0-429-98248-4.
  10. ^ "Section III". Department of Physics and Astronomy. Retrieved 2024-12-16.
  11. ^ Cervantes-Cota, Jorge L.; Galindo-Uribarri, Salvador; Smoot, George F. (2016). "A Brief History of Gravitational Waves". Universe. 2 (3): 22. arXiv:1609.09400. Bibcode:2016Univ....2...22C. doi:10.3390/universe2030022. ISSN 2218-1997.
  12. ^ a b c d e Byrne, Peter (2012-12-13). The Many Worlds of Hugh Everett III: Multiple Universes, Mutual Assured Destruction, and the Meltdown of a Nuclear Family. OUP Oxford. ISBN 978-0-19-165522-7.