24 research outputs found
Cramer's Transactional Interpretation and Causal Loop Problems
Tim Maudlin's argument for the inconsistency of Cramer's Transactional
Interpretation (TI) of quantum theory has been considered in some detail by
Joseph Berkovitz, who has provided a possible solution to this challenge at the
cost of a significant empirical lacuna on the part of TI. The present paper
proposes an alternative solution in which Maudlin's charge of inconsistency is
evaded but at no cost of empirical content on the part of TI. However,
Maudlin's argument is taken as ruling out Cramer's heuristic ``pseudotime''
explanation of the realization of one transaction out of many.Comment: To appear in Synthes
Quantum Haecceity
There is an extensive philosophical literature on the interrelated issues of
identity, individuality, and distinguishability in quantum systems. A key
consideration is whether quantum systems are subject to a strong form of
individuality termed "haecceity" (from the Latin for "this-ness"). I argue that
the traditional, strong form of haecceity does not apply at the quantum level,
but that in order to properly account for the need for symmetrization in
quantum systems, a weaker kind of haecceity must be involved, which I call
"quantum haecceity." In the process, I also question some generally accepted
tenets of the current debate, such as the idea that symmetrization of states
for identical quanta must be postulated and reflects permutation invariance.
Instead, I note that a perturbative Hamiltonian is required for exchange
effects, which suggests that the need for symmetrization arises from specific
physical conditions.Comment: Final accepted version, to appear in Proceedings of the Workshop
"Identity, Individuality and Indistinguishability in Physics and
Mathematics," Philosophical Transactions
The Relativistic Transactional Interpretation: Immune to the Maudlin Challenge
The Transactional Interpretation has been subject at various times to a challenge based on a type of thought experiment first proposed by Maudlin. It has been argued by several authors that such experiments do not in fact constitute a significant problem for the transactional picture. The purpose of this work is to point out that, when the relativistic level of the interpretation is considered, Maudlin-type challenges cannot even be mounted, since the putative 'slow-moving offer wave,' taken as subject to contingent confirmation, does not exist. This is a consequence of the Davies relativistic quantum-mechanical version of the direct-action theory together with the asymmetry between fermionic field sources and bosonic fields. The Maudlin challenge therefore evaporates completely when the relativistic level of the theory is taken into account
Shutters, Boxes, But No Paradoxes: Time Symmetry Puzzles in Quantum Theory
The ``N-Box Experiment'' is a much-discussed thought experiment in quantum
mechanics. It is claimed by some authors that a single particle prepared in a
superposition of N+1 box locations and which is subject to a final
``post-selection'' measurement corresponding to a different superposition can
be said to have occupied ``with certainty'' N boxes during the intervening
time. However, others have argued that under closer inspection, this surprising
claim fails to hold. Aharonov and Vaidman have continued their advocacy of the
claim in question by proposing a variation on the N-box experiment, in which
the boxes are replaced by shutters and the pre- and post-selected particle is
entangled with a photon. These authors argue that the resulting ``N-shutter
experiment'' strengthens their original claim regarding the N-box experiment.
It is argued in this paper that the apparently surprising features of this
variation are no more robust than those of the N-box experiment and that it is
not accurate to say that the particle is ``with certainty'' in all N shutters
at any given time.Comment: Presentation improved; to appear in International Studies in
Philosophy of Scienc
The Relativistic Transactional Interpretation: Immune to the Maudlin Challenge
The Transactional Interpretation has been subject at various times to a challenge based on a type of thought experiment first proposed by Maudlin. It has been argued by several authors that such experiments do not in fact constitute a significant problem for the transactional picture. The purpose of this work is to point out that, when the relativistic level of the interpretation is considered, Maudlin-type challenges cannot even be mounted, since the putative 'slow-moving offer wave,' taken as subject to contingent confirmation, does not exist. This is a consequence of the Davies relativistic quantum-mechanical version of the direct-action theory together with the asymmetry between fermionic field sources and bosonic fields. The Maudlin challenge therefore evaporates completely when the relativistic level of the theory is taken into account
Quantum Nonlocality: Not Eliminated by the Heisenberg Picture
It is argued that the Heisenberg picture of standard quantum mechanics does
not save Einstein locality as claimed in Deutsch and Hayden (2000). In
particular, the EPR-type correlations that DH obtain by comparing two qubits in
a local manner are shown to exist before that comparison. In view of this
result, the local comparison argument would appear to ineffective in supporting
their locality claim.Comment: Final version; to appear in Foundations of Physic
The Possibilist Transactional Interpretation and Relativity
A recent ontological variant of Cramer's Transactional Interpretation, called
"Possibilist Transactional Interpretation" or PTI, is extended to the
relativistic domain. The present interpretation clarifies the concept of
'absorption,' which plays a crucial role in TI (and in PTI). In particular, in
the relativistic domain, coupling amplitudes between fields are interpreted as
amplitudes for the generation of confirmation waves (CW) by a potential
absorber in response to offer waves (OW), whereas in the nonrelativistic
context CW are taken as generated with certainty. It is pointed out that
solving the measurement problem requires venturing into the relativistic domain
in which emissions and absorptions take place; nonrelativistic quantum
mechanics only applies to quanta considered as 'already in existence' (i.e.,
'free quanta'), and therefore cannot fully account for the phenomenon of
measurement, in which quanta are tied to sources and sinks.Comment: Final version with some minor corrections as published in Foundations
of Physics. This paper has significant overlap with Chapter 6 of my book on
the Transactional Interpretation, forthcoming from Cambridge University
Press:
http://www.cambridge.org/us/knowledge/isbn/item6860644/?site_locale=en_US
(Additional preview material is available at rekastner.wordpress.com)
Comments welcom
de Broglie waves as the "Bridge of Becoming" between quantum theory and relativity
It is hypothesized that de Broglie's 'matter waves' provide a dynamical basis
for Minkowski spacetime in an antisubstantivalist or relational account. The
relativity of simultaneity is seen as an effect of the de Broglie oscillation
together with a basic relativity postulate, while the dispersion relation from
finite rest mass gives rise to the differentiation of spatial and temporal
axes. Thus spacetime is seen as not fundamental, but rather as emergent from
the quantum level. A result by Solov'ev which demonstrates that time is not an
applicable concept at the quantum level is adduced in support of this claim.
Finally, it is noted that de Broglie waves can be seen as the "bridge of
becoming" discussed by Elitzur and Dolev (2005).Comment: Forthcoming in Foundations of Science; reference added to recent work
of Dolc
Inside-Out Evacuation of Transitional Protoplanetary Disks by the Magneto-Rotational Instability
How do T Tauri disks accrete? The magneto-rotational instability (MRI)
supplies one means, but protoplanetary disk gas is typically too poorly ionized
to be magnetically active. Here we show that the MRI can, in fact, explain
observed accretion rates for the sub-class of T Tauri disks known as
transitional systems. Transitional disks are swept clean of dust inside rim
radii of ~10 AU. Stellar coronal X-rays ionize material in the disk rim,
activating the MRI there. Gas flows from the rim to the star, at a rate limited
by the depth to which X-rays ionize the rim wall. The wider the rim, the larger
the surface area that the rim wall exposes to X-rays, and the greater the
accretion rate. Interior to the rim, the MRI continues to transport gas; the
MRI is sustained even at the disk midplane by super-keV X-rays that Compton
scatter down from the disk surface. Accretion is therefore steady inside the
rim. Blown out by radiation pressure, dust largely fails to accrete with gas.
Contrary to what is usually assumed, ambipolar diffusion, not Ohmic
dissipation, limits how much gas is MRI-active. We infer values for the
transport parameter alpha on the order of 0.01 for GM Aur, TW Hyd, and DM Tau.
Because the MRI can only afflict a finite radial column of gas at the rim, disk
properties inside the rim are insensitive to those outside. Thus our picture
provides one robust setting for planet-disk interaction: a protoplanet interior
to the rim will interact with gas whose density, temperature, and transport
properties are definite and decoupled from uncertain initial conditions. Our
study also supplies half the answer to how disks dissipate: the inner disk
drains from the inside out by the MRI, while the outer disk photoevaporates by
stellar ultraviolet radiation.Comment: Accepted to Nature Physics June 7, 2007. The manuscript for
publication is embargoed per Nature policy. This arxiv.org version contains
more technical details and discussion, and is distributed with permission
from the editors. 10 pages, 4 figure