11 research outputs found
Uniqueness of the Fock quantization of the Gowdy model
After its reduction by a gauge-fixing procedure, the family of linearly
polarized Gowdy cosmologies admit a scalar field description whose
evolution is governed by a Klein-Gordon type equation in a flat background in
1+1 dimensions with the spatial topology of , though in the presence of a
time-dependent potential. The model is still subject to a homogeneous
constraint, which generates -translations. Recently, a Fock quantization
of this scalar field was introduced and shown to be unique under the
requirements of unitarity of the dynamics and invariance under the gauge group
of -translations. In this work, we extend and complete this uniqueness
result by considering other possible scalar field descriptions, resulting from
reasonable field reparameterizations of the induced metric of the reduced
model. In the reduced phase space, these alternate descriptions can be obtained
by means of a time-dependent scaling of the field, the inverse scaling of its
canonical momentum, and the possible addition of a time-dependent, linear
contribution of the field to this momentum. Demanding again unitarity of the
field dynamics and invariance under the gauge group, we prove that the
alternate canonical pairs of fieldlike variables admit a Fock representation if
and only if the scaling of the field is constant in time. In this case, there
exists essentially a unique Fock representation, provided by the quantization
constructed by Corichi, Cortez, and Mena Marugan. In particular, our analysis
shows that the scalar field description proposed by Pierri does not admit a
Fock quantization with the above unitarity and invariance properties.Comment: 14 page
Quantum unitary dynamics in cosmological spacetimes
We address the question of unitary implementation of the dynamics for scalar
fields in cosmological scenarios. Together with invariance under spatial
isometries, the requirement of a unitary evolution singles out a rescaling of
the scalar field and a unitary equivalence class of Fock representations for
the associated canonical commutation relations. Moreover, this criterion
provides as well a privileged quantization for the unscaled field, even though
the associated dynamics is not unitarily implementable in that case. We discuss
the relation between the initial data that determine the Fock representations
in the rescaled and unscaled descriptions, and clarify that the S-matrix is
well defined in both cases. In our discussion, we also comment on a recently
proposed generalized notion of unitary implementation of the dynamics, making
clear the difference with the standard unitarity criterion and showing that the
two approaches are not equivalent.Comment: 18 page
Quantum Gowdy model: A uniqueness result
Modulo a homogeneous degree of freedom and a global constraint, the linearly
polarised Gowdy cosmologies are equivalent to a free scalar field
propagating in a fixed nonstationary background. Recently, a new field
parameterisation was proposed for the metric of the Gowdy spacetimes such that
the associated scalar field evolves in a flat background in 1+1 dimensions with
the spatial topology of , although subject to a time dependent potential.
Introducing a suitable Fock quantisation for this scalar field, a quantum
theory was constructed for the Gowdy model in which the dynamics is implemented
as a unitary transformation. A question that was left open is whether one might
adopt a different, nonequivalent Fock representation by selecting a distinct
complex structure. The present work proves that the chosen Fock quantisation is
in fact unique (up to unitary equivalence) if one demands unitary
implementation of the dynamics and invariance under the group of constant
translations. These translations are precisely those generated by the global
constraint that remains on the Gowdy model. It is also shown that the proof of
uniqueness in the choice of complex structure can be applied to more general
field dynamics than that corresponding to the Gowdy cosmologies.Comment: 28 pages, minor changes, version accepted for publication in
Classical and Quantum Gravit
Massless scalar field in de Sitter spacetime: unitary quantum time evolution
We prove that, under the standard conformal scaling, a massless field in de
Sitter spacetime admits an O(4)-invariant Fock quantization such that time
evolution is unitarily implemented. This result disproves previous claims in
the literature. We discuss the relationship between this quantization with
unitary dynamics and the family of O(4)-invariant Hadamard states given by
Allen and Folacci, as well as with the Bunch-Davies vacuum.Comment: 23 pages. Typos corrected, matches published versio
Uniqueness of the Fock quantization of fields with unitary dynamics in nonstationary spacetimes
The Fock quantization of fields propagating in cosmological spacetimes is not uniquely determined because of several reasons. Apart from the ambiguity in the choice of the quantum representation of the canonical commutation relations, there also exists certain freedom in the choice of field: one can scale it arbitrarily absorbing background functions, which are spatially homogeneous but depend on time. Each nontrivial scaling turns out into a different dynamics and, in general, into an inequivalent quantum field theory. In this work we analyze this freedom at the quantum level for a scalar field in a nonstationary, homogeneous spacetime whose spatial sections have S3 topology. A scaling of the configuration variable is introduced as part of a linear, time dependent canonical transformation in phase space. In this context, we prove in full detail a uniqueness result about the Fock quantization requiring that the dynamics be unitary and the spatial symmetries of the field equations have a natural unitary implementation. The main conclusion is that, with those requirements, only one particular canonical transformation is allowed, and thus only one choice of field-momentum pair (up to irrelevant constant scalings). This complements another previous uniqueness result for scalar fields with a time varying mass on S3, which selects a specific equivalence class of Fock representations of the canonical commutation relations under the conditions of a unitary evolution and the invariance of the vacuum under the background symmetries. In total, the combination of these two different statements of uniqueness picks up a unique Fock quantization for the system. We also extend our proof of uniqueness to other compact topologies and spacetime dimensions
Black holes, gravitational waves and fundamental physics: a roadmap
The grand challenges of contemporary fundamental physics—dark matter, dark energy, vacuum energy, inflation and early universe cosmology, singularities and the hierarchy problem—all involve gravity as a key component. And of all gravitational phenomena, black holes stand out in their elegant simplicity, while harbouring some of the most remarkable predictions of General Relativity: event horizons, singularities and ergoregions.
The hitherto invisible landscape of the gravitational Universe is being unveiled before our eyes: the historical direct detection of gravitational waves by the LIGO-Virgo collaboration marks the dawn of a new era of scientific exploration. Gravitational-wave astronomy will allow us to test models of black hole formation, growth and evolution, as well as models of gravitational-wave generation and propagation. It will provide evidence for event horizons and ergoregions, test the theory of General Relativity itself, and may reveal the existence of new fundamental fields. The synthesis of these results has the potential to radically reshape our understanding of the cosmos and of the laws of Nature.
The purpose of this work is to present a concise, yet comprehensive overview of the state of the art in the relevant fields of research, summarize important open problems, and lay out a roadmap for future progress. This write-up is an initiative taken within the framework of the European Action on 'Black holes, Gravitational waves and Fundamental Physics'
Metodos matematicos em quantizacao canonica de espacos de fase nao triviais
This thesis is devoted to several aspects of the problem of canonical quantization of non-trivial phase spaces, both in finite and infinite dimensions. We will consider quantum representations of the type of the coordinate Schrodinger representation. In part I we discuss general aspects of the problem of quantization of non-linear finite dimensional phase spaces. Besides reviewing concepts that will be generalized in parts II and III, we discuss and criticize a particular quantization of the torus proposed by Gotay. We argue that algebraic relations among classical observables should be taken into account at the quantum level. Part II is devoted to measure theoretical methods in the canonical quantization of scalar field theories. We review the theory of cyclic representations of the Weyl relations and the quantization of the free scalar field with non-zero mass. We study the support of the free field measures, using a sequence of variables which test the field behaviour at large distances, thus allowing to distinguish between the typical quantum fields associated with different values of the mass. Part III is devoted to mathematical methods in the canonical quantization of gauge theories of connections. The use of projective methods together with the formalism of groupoids allows a systematization of the construction of the space of quantum connections introduced by Baez, clarifying the relation between this space and the quantum configuration space introduced by Ashtekar and Isham. We also study properties of the Ashtekar-Lewandowski measure in. We show that this measure is ergodic with respect to the action of the group of diffeomorphisms. We also prove that a typical quantum connection restricted to an analytic curve leads to a parallel transport discontinuous at every point of the curveAvailable from Fundacao para a Ciencia e a Tecnologia, Servico de Informacao e Documentacao, Av. D. Carlos I, 126, 1249-074 Lisboa, Portugal / FCT - Fundação para o Ciência e a TecnologiaSIGLEPTPortuga