ESF Network on PHILOSOPHICAL
AND FOUNDATIONAL PROBLEMS OF MODERN PHYSICS
ESF Network on
The European Science Foundation
Network for Philosophical and Foundational Problems of Modern Physics
ESF Conference on Philosophical
and Foundational Issues in Spacetime Theories, Oxford, 24–27 March 2004
Local organisation
Jeremy Butterfield (jb56@cus.cam.ac.uk)
Oliver Pooley (oliver.pooley@philosophy.oxford.ac.uk)
Faculty of Philosophy
10 Merton St
Oxford OX1 4JJ
PROGRAMME (as of March 22th 2004)
Wednesday 24 March
Wednesday 24 March
9.00
Dr Harvey Brown (Oxford)
Relativity as a "constructive" theory: a defence of the
Pauli-Eddington-Bell interpretation
10.15
Dr Henrik Zinkernagel (Grenada)
Cosmology and the Meaning of Time
11.15
Coffee
11.45
Dr Edward Anderson (London)
Plausible first principles for
geometrodynamics? General relativity can be formulated in a
number of ways. One such is geometrodynamics: the dynamics of
3-geometries. Whereas Arnowitt--Deser--Misner and Dirac obtained
this by laborious rearrangement of the Einstein field equations, Wheeler
asked whether it could be made to rest instead on ``plausible first
principles". Hojman--Kuchar--Teitelboim derived geometrodynamics
from spacetime first principles. More recently Barbour, Foster,
Kelleher, O Murchadha and I have been working on the derivation from
3-space principles. In this talk I explain the 3-space approach
(TSA). I briefly mention how general relativity is not uniquely
picked out by the TSA. I relate the TSA to Kuchar's scheme which
presupposes spacetime. I show that the TSA is ``plausible" in that
the usual full set of fundamental matter fields can be included. I
investigate how the relativity principles, the principle of equivalence
and the gauge principle may arise in the
TSA. References: S.A. Hojman, K.V. Kuchar and C. Teitelboim,
Ann. Phys. 96 p 88 (1976). J.B. Barbour, B.Z. Foster and N. O
Murchadha, Class. Quantum Grav 19 p 3217 (2002), gr-qc/0012089. E.
Anderson and J.B. Barbour, Class. Quantum Grav. 19 p 3249 (2002),
gr-qc/0201092. E. Anderson, Phys. Rev. D68 p 104001 (2003), gr-qc/0302035. E.
Anderson, PhD Thesis, University of London (2004). E. Anderson, J.B.
Barbour, B.Z. Foster, N. O' Murchadha, Class. Quantum Grav. 20 p 157
(2003), gr-qc/0211022. E.
Anderson, J.B. Barbour, B.Z. Foster, B. Kelleher and N. O'
Murchadha, forthcoming. K.V. Kuchar, J. Math Phys 17 p 777; p
792; p 801 (1976).
14.00
Dr Simon Saunders (Oxford)
Frame-dependence: pros and cons
15.15
Prof Andreas Bartels and Prof Holger Lyre (Bonn)
Structural realism and the generality of the hole
argument
16.15
Tea
16.45
Dr Oliver Pooley (Oxford)
What is Observable in Special and General Relativity?
Thursday 25 March
9.00
Prof Gerard Emch (Florida and Oxford)
Symmetry and the Symplectic Geometry of Gravitational Wave
Causality
10.15
Prof Dennis Dieks (Utrecht)
Another look at general covariance and the equivalence of frames of
reference In his general theory of relativity Einstein
sought to generalize his special relativistic principle of relativity to a
principle according to which all frames of reference, regardless of their
motion, are equivalent. He thought to have achieved this aim through the
general covariance of the equations of GRT: because the equations take the
same form in every frame of reference, all frames are physically
equivalent. There seems to be a consensus among philosophers of relativity
that Einstein was mistaken here: form invariance of the equations does not
imply physical equivalence of frames. We will argue, however, that
Einstein's position is not unreasonable at all. Although there are
certainly physical differences between reference frames in general
relativity, these differences should be seen as fact-like rather than
law-like. By contrast, in classical mechanics and in special relativity
the differences between inertial systems and accelerated systems have a
law-like status. The fact-like character of the differences between frames
in general relativity justifies regarding them as equivalent in the same
sense as inertial frames in special relativity are
equivalent.
11.15
Coffee
11.45
Prof Massimo Pauri (Parma) and Dr Luca
Lusanna (Florence)
General Covariance and the Objectivity of Spacetime
Point-events We show the unique capabilities of the ADM
Hamiltonian approach to metric gravity to get new insights into a series
of foundational issues of GR. Our results - valid for the
Christodoulou-Klainermann class of models of the theory - include: a)
finding the "last remnant of physical objectivity of space-time" by means
of a physical individuation of point-events in terms of the
intrinsic degrees of freedom of the gravitational field; b) a
counter-example to the frozen-evolution picture; c) the definition
of extended, non-inertial, space-time laboratories in which
tidal-like and generalized inertial effects can be separated
(though not invariantly); d) a main conjecture (which would entail
invariance of the above separation) about the relation of the Dirac and
the Bergmann definitions of observable; e) a disclosure of the
dynamical nature that the traditional "conventions" about distant
simultaneity assume in canonical metric gravity: different "conventions"
within the same üniverse" are simply gauge-related options;
f) an implementation of the physical individuation of point-events
through a well-defined empirical procedure leading to an operational
definition of space-time. At the end, a peculiar holistic and
structuralist view of space-time
emerges. References: * L.Lusanna and M.Pauri, The Physical
Role of Gravitational and Gauge Degrees of Freedom in General Relativity -
I: Dynamical Synchronization and Generalized Inertial Effects,
pre-print. * L.Lusanna and M.Pauri, The Physical Role of
Gravitational and Gauge Degrees of Freedom in General Relativity - II :
Dirac versus Bergmann Observables and the Objectivity of Space-Time,
pre-print. * M.Pauri and M.Vallisneri, Ephemeral Point-Events: is
there a Last Remnant of Physical Objectivity?, essay for the 70th
birthday of R.Torretti, Dialogos 79, 263 (2002) (gr-qc/0203014). *
L.Lusanna and M.Pauri, General Covariance and the Objectivity of
Space-Time Point-Events: The Physical Role of Gravitational and Gauge
Degrees of Freedom in General Relativity (gr-qc/0301040). *
M.Dorato and M.Pauri, Holism and Structuralism in Classical and Quantum
General Relativity, Pittsburgh-Archive, ID code 1606, February 10,
2004. * L.Lusanna, The Rest-Frame Instant Form of Metric
Gravity, Gen.Rel.Grav. 33, 1579 (2001) (gr-qc/0101048). *
L.Lusanna and S.Russo, A New Parametrization for Tetrad Gravity,
Gen.Rel.Grav. 34, 189 (2002)(gr-qc/0102074). * R.De
Pietri, L.Lusanna, L.Martucci and S.Russo, Dirac's Observables for the
Rest-Frame Instant Form of Tetrad Gravity in a Completely Fixed
3-Orthogonal Gauge, Gen.Rel.Grav. 34, 877 (2002) (gr-qc/0105084). * D.Alba
and L.Lusanna, Simultaneity, Radar 4-Coordinates and the 3+1 Point of
View about Accelerated Observers in Special Relativity
(gr-qc/0311058). * J.Agresti, R.DePietri, L.Lusanna and L.Martucci,
Hamiltonian Linearization of the Rest-Frame Instant Form of Tetrad
Gravity in a Completely Fixed 3-Orthogonal Gauge: a Radiation Gauge for
Background-Independent Gravitational Waves in a Post-Minkowskian Einstein
Space-Time, to appear in Gen.Rel.Grav. (gr-qc/0302084). *
L.Lusanna, Towards a Unified Description of the Four Interactions in
Terms of Dirac-Bergmann Observables, invited contribution to the book
Quantum Field Theory: a 20th Century Profile, of the Indian
National Science Academy, ed.A.N.Mitra, forewards by F.J.Dyson (Hindustan
Book Agency, New Delhi, 2000) (hep-th/9907081).
14.00
Prof Istvan Nemeti and Prof Hajnal Andreka (Budapest)
On the logical foundation of spacetime theories We
will discuss two kinds of connections between logic and relativity. (1)
Logical foundation of relativity. Foundation of Mathematics (FOM)
bulletinboard (http://www.cs.nyu.edu/pipermail/fom/,
December 2003 - February 2004) contains several postings by leading
logician Harvey Friedman in which he proposes to export the methodology,
spirit, and machinery of Foundational Thinking from the area of
Foundations of Mathematics to a similar foundation of relativity which
eventually would provide logic-based axiomatic foundation for both special
relativity and general relativity. Of course, one begins with special
relativity (but keeping an eye open for the direction of general
relativity). The above aims coincide with the ones our group has been
pursuing (leading to a broader cooperation). A precise conceptual
analysis of relativity emerges on these foundations elaborated purely in
first-order logic (FOL). E.g. we formalize (in FOL) Einstein's SPR
(Special Principle of Relativity) and we calibrate its deductive
role/power in the hierarchy of axioms/postulates/principles of relativity
theory. As an example illustrating the uses of this precise logic-based
framework we do the following. Although it is customary to derive NoFTL
(No Faster Than Light travel) from SPR, we show that SPR does not entail
this conclusion logically. On the other hand, making some of the usual
tacit assumptions explicit, we prove NoFTL from these tacit assumptions
without using SPR. Then we discuss what extra power SPR adds to these
tacit assumptions. Material on the above can be found in the
web-site http://www.math-inst.hu/pub/algebraic-logic/Contents.html,
e.g. [1]-[4] below. (2) In the other direction, relativity theory
can influence FOM, too! The Relativity |--> Logic connection is
discussed in [5]-[7]. Besides Malament-Hogarth-Tipler (beyond Turing)
computability, we will also connect these ideas to CTC's in spacetimes
popularly named "time-travel". E.g. mathematical logic can be applied to
discussing how much of the consistency constraints imposed by the
possiblility of time-travel are dictated by purely logical considerations
and how much are generated by the resources of physical theories. Cf.
Christian Wuthrich [W], [ESW].
Quantum Superpositions of Spacetimes: do they Reduce Because of a
Clash of Principles?
16.15
Tea
16.45
Dr Nick Bostrom (Oxford)
Self-Locating Belief in an Infinite
Spacetime Background papers: 1.
"Self-Locating Belief in Big Worlds: Cosmology’s Missing Link to
Observation" Journal of Philosophy, Vol. 99, No. 12
(2002). Abstract. Current cosmological theories say that the world is
so big that all possible observations are in fact made. But then, how can
such theories be tested? What could count as negative evidence? To answer
that, we need to consider observation selection effects. A preprint of
this paper is available here: http://www.anthropic-principle.com/preprints/cos/big2.pdf
2. Anthropic Bias: Observation Selection Effects
in Science and Philosophy (Routledge: New York, 2002). Abstract.
This book presents the first mathematical theory of observation selection
effects - an important kind of bias that infests many branches of science
and philosophy. We can tame these biases! There are implications for
cosmology, evolutionary biology, game theory, the interpretation of
quantum mechanics, the Doomsday argument, the Sleeping Beauty problem, the
search for extraterrestrial life, the question of whether God exists, and
traffic planning. Five sample chapters are available online at: http://www.anthropic-principle.com/book/ 3.
I maintain a general preprint achieve of online papers on related topics
at: http://www.anthropic-principle.com/preprints.html
Friday 26 March
9.00
Dr Fay Dowker (London and Perimeter Institute, Waterloo)
The Causal Set as the Deep Structure of Spacetime One
approach to solving the problem of quantum gravity is based on the causal
set hypothesis, which states that the deep, quantum structure of spacetime
is discrete and is what is known in mathematics as a ``partial order'' or
``poset'', a kind of extended family tree. Causal set theory has now
reached a stage of maturity in which both foundational issues and
phenomenological questions can be addressed concretely. An example of the
former is the question of what the observables of quantum gravity are (in
other words, what is the solution of the ``problem of time'' in the causal
set context). An example of phenomenology is the ``Lucretius effect'' of
causal set discreteness on the propagation of massive
particles. Relevant papers: 1)Background Causal Set material,
all by Rafael Sorkin and available from his website http://www.physics.syr.edu/~sorkin/some.papers/ (i)
A Specimen of Theory Construction from Quantum Gravity (ii) First Steps
with Causal Sets (iii) Spacetime and Causal Sets 2) ``Observables''
in Causal Set Cosmology http://arxiv.org/abs/gr-qc/0210061 3)
The Lucretius effect (``swerves'') Quantum Gravity Phenomenology,
Lorentz Invariance and Discreteness http://arxiv.org/abs/gr-qc/0311055
10.15
Dr Carl Dolby (Oxford)
Life in an Energy Eigenstate: The Problem of Time in Quantum
Gravity
11.15
Coffee
11.45
Dr Joy Christian (Oxford)
Passage of Time in a Planck Scale Rooted Local Inertial
Structure http://arxiv.org/abs/gr-qc/0308028 It
is argued that the `problem of time' in quantum gravity necessitates a
refinement of the local inertial structure of the world, demanding a
replacement of the usual Minkowski line element by a 4+2n dimensional
pseudo-Euclidean line element, with the extra 2n being the number of
internal phase space dimensions of the observed system. In the refined
structure, the inverse of the Planck time takes over the role of
observer-independent conversion factor usually played by the speed of
light, which now emerges as an invariant but derivative quantity. In the
relativistic theory based on the refined structure, energies and momenta
turn out to be invariantly bounded from above, and lengths and durations
similarly bounded from below, by their respective Planck scale values.
Along the external timelike world-lines, the theory naturally captures the
`flow of time' as a genuinely structural attribute of the world. The
theory also predicts expected deviations--suppressed quadratically by the
Planck energy--from the dispersion relations for free fields in the
vacuum. The deviations from the special relativistic Doppler shifts
predicted by the theory are also suppressed quadratically by the Planck
energy. Nonetheless, in order to estimate the precision required to
distinguish the theory from special relativity, an experiment with a
binary pulsar emitting TeV range gamma-rays is considered in the context
of the predicted deviations from the second-order
shifts.
AFTERNOON FREE
Saturday 27 March
9.00
Prof Don Howard (Notre Dame USA)
Spin, Space, Symmetries, and Statistics: Some Questions about
Covariance, Nonseparability, and Particle Identity in the
1920s
10.15
Prof Michel Ghins (Louvain)
Revisiting the Equivalence Principle in General
Relativity Relevant paper: Studies In History and
Philosophy of Modern Physics 32, March 2001, 33--51 doi:10.1016/S1355-2198(00)00038-1
11.15
Coffee
11.45
Dr Julian Barbour (Oxford)
Absolute and Relative Motion: A Review
Aim
The conference intends to bring together physicists,
mathematicians, and philosophers of physics to discuss and analyse problems in
the foundations of spacetime theories from a variety of perspectives.
Particular attention will be devoted to the following topics:
Spacetime
in quantum gravity
Philosophical
issues about cosmology, including the meaning and the direction of time,
and self-locating belief
Gravitational
waves
The
equivalence principle
General
covariance and the nature of observables in general relativity
Philosophical
aspects of symmetries, including gauge symmetries and discrete symmetries,
in non-quantum and quantum contexts
Invited Speakers
Julian Barbour (Oxford)
Andreas Bartels (University of Bonn)
Nick Bostrom (University of Oxford)
Harvey R. Brown (University of Oxford)
Dennis Dieks (University of Utrecht)
Fay Dowker (University of London)
George Ellis (University of Capetown)
Gerard Emch (University of Florida)
Michel Ghins (University of Louvain)
Don Howard (University of Notre Dame, USA)
Luca Lusanna (University of Florence)
Holger Lyre (University of Bonn)
Istvan Nemeti (University of Budapest)
Massimo Pauri (University of Parma)
Sir Roger Penrose (University of Oxford) to be confirmed
Oliver Pooley (University of Oxford)
Sir Martin Rees (Astronomer Royal, University of Cambridge)
Carlo Rovelli (University of Marseilles)
Simon Saunders (University of Oxford)
John Stachel (Boston University)
Henrik Zinkernagel (University of Grenada)
Audience
The conference will be the second major conference organized
by the recently established European Science Foundation Network for Philosophical
and Foundational Problems of Modern Physics.The aims of this Network are to bring together European researchers from
relevant disciplines (e.g., in this case: physicists and mathematicians working
in spacetime theories and philosophers of physics) and to contribute to the
training of young researchers in these fields.The Network will serve as a platform for European research groups and
individual researchers in order to learn from and stimulate each other’s work
and initiate joint projects.
Participation
In order to
stimulate interaction and fruitful discussion the number of participants is
limited to a maximum of 55.
Support
The main sponsor of the conference is the European Science
Foundation.Additional support is
provided by British Academy.By this support we expect to be able to
cover the travel expenses (economy class), accommodation and lunches for
invited Speakers, and the costs of accommodation and lunches for some other
participants from ESF-member states. (This will be by reimbursement after the
conference.)However, participants who
are able to get reimbursements from their home institutions are strongly encouraged
to do so.Any participantfrom an ESF-member state who wishes to apply
for some financial support should send a CV of up to 3 pages.In awarding financial support, preference
will be given to more junior scholars.
Proceedings
The intention is to publish some of the papers presented at
the conference, after the usual refereeing procedure, as a special issue of
Studies in History and Philosophy of Modern Physics.
Programme
Venue
The conference will take place at the Philosophy Centre of
Oxford University, 10 Merton St, Oxford.
Accommodation
Participants will be accommodated in St Edmund Hall, an
Oxford College, which is 150 metres from the Philosophy Centre.Accommodation may be taken up on Tuesday 23
March, and may be retained until Sunday 28 March, in order to get cheap
airfares.Further details will be
announced in due course on this website.