984 research outputs found
Greek Myth on Etruscan Urns from Perusia: the sacrifice of Iphigenia
The production of cremation urns of Perusia is one of the most important of North Etruria, and many of them were decorated with scenes of myth. The meaning of a myth is strictly related to its social and cultural context. Indeed, the reception of an iconographical theme depends on the specific cultural setting and each society perceives and re-elaborates the same image in different ways. This paper examines the use of the myth of the sacrifice of Iphigenia for the local Etruscan context of the second and first century B.C.E. The representation of that myth enjoyed in Perusia a success that is much greater than in Greek context, revealing the creative approach of the Perusian sculptors and the culture of their patrons
Synergistic Gravity and the Role of Resonances in GRS-Inspired Braneworlds
We consider 5D braneworld models of quasi-localized gravity in which 4D
gravity is reproduced at intermediate scales while the extra dimension opens up
at both the very short and the very long distances, where the geometry is flat.
Our main interest is the interplay between the zero mode of these models,
whenever a normalizable zero mode exists, and the effects of zero energy
graviton resonant modes coming from the contributions of massive KK modes. We
first consider a compactified version of the GRS model and find that
quasi-localized gravity is characterized by a scale for which both the
resonance and the zero mode have significant contribution to 4D gravity. Above
this scale, gravity is primarily mediated by the zero mode, while the resonance
gives only minor corrections. Next, we consider an asymmetric version of the
standard non-compact GRS model, characterized by different cosmological
constants on each AdS side. We show that a resonance is present but the
asymmetry, through the form of the localizing potential, can weaken it,
resulting in a shorter lifetime and, thus, in a shorter distance scale for 4D
gravity. As a third model exhibiting quasi-localization, we consider a version
of the GRS model in which the central positive tension brane has been replaced
by a configuration of a scalar field propagating in the bulk.Comment: 18 pages, 3 figures, added 1 figure, revised version as published in
Class. Quant. Gra
The radion and the perturbative metric in RS1
We calculate the linearized metric perturbations in the five dimensional
two-brane model of Randall and Sundrum. In a carefully chosen gauge, we write
down and decouple Einstein equations for the perturbations and get the final
and simple perturbative metric ansatz. This ansatz turns out to be equal to the
linear expansion of the metric solution of Charmousis et al. \cite{rubakov}. We
show that this ansatz, the metric ansatz of Boos et al. \cite{boos} and the one
of Das and Mitov \cite{das} are not incompatible, as it appears on the surface,
but completely equivalent by an allowed gauge transformation that we give.Comment: 12 pages, no figures, LaTeX, typos fixed, 1 reference adde
Gauss-Bonnet gravity renders negative tension braneworlds unstable
We show that the Gauss-Bonnet correction to Einstein gravity induces a
gravitational tachyon mode, namely an unstable spin 2 fluctuation, in the
Randall-Sundrum I model. We demonstrate that this instability is generically
related to the presence of a negative tension brane in the set-up, with or
without -symmetry across it. Indeed it is shown that the tachyon mode is a
bound state localised on any negative tension brane of co-dimension one,
embedded in anti-de Sitter background. We discuss the possible resolution of
this instability by the inclusion of induced gravity terms on the branes or by
an effective four-dimensional cosmological constant.Comment: published versio
Spontaneous Lorentz Breaking and Massive Gravity
We study a theory where the presence of an extra spin-two field coupled to
gravity gives rise to a phase with spontaneously broken Lorentz symmetry. In
this phase gravity is massive, and the Weak Equivalence Principle is respected.
The newtonian potentials are in general modified, but we identify an
non-perturbative symmetry that protects them. The gravitational waves sector
has a rich phenomenology: sources emit a combination of massless and massive
gravitons that propagate with distinct velocities and also oscillate. Since
their velocities differ from the speed of light, the time of flight difference
between gravitons and photons from a common source could be measured.Comment: 4 page
Massive Gravity on a Brane
At present no theory of a massive graviton is known that is consistent with
experiments at both long and short distances. The problem is that consistency
with long distance experiments requires the graviton mass to be very small.
Such a small graviton mass however implies an ultraviolet cutoff for the theory
at length scales far larger than the millimeter scale at which gravity has
already been measured. In this paper we attempt to construct a model which
avoids this problem. We consider a brane world setup in warped AdS spacetime
and we investigate the consequences of writing a mass term for the graviton on
a the infrared brane where the local cutoff is of order a large (galactic)
distance scale. The advantage of this setup is that the low cutoff for physics
on the infrared brane does not significantly affect the predictivity of the
theory for observers localized on the ultraviolet brane. For such observers the
predictions of this theory agree with general relativity at distances smaller
than the infrared scale but go over to those of a theory of massive gravity at
longer distances. A careful analysis of the graviton two-point function,
however, reveals the presence of a ghost in the low energy spectrum. A mode
decomposition of the higher dimensional theory reveals that the ghost
corresponds to the radion field. We also investigate the theory with a brane
localized mass for the graviton on the ultraviolet brane, and show that the
physics of this case is similar to that of a conventional four dimensional
theory with a massive graviton, but with one important difference: when the
infrared brane decouples and the would-be massive graviton gets heavier than
the regular Kaluza--Klein modes, it becomes unstable and it has a finite width
to decay off the brane into the continuum of Kaluza-Klein states.Comment: 26 pages, LaTeX. v2: extended version with an appendix added about
non Fierz-Pauli mass terms. Few typos corrected. Final version appeared in
PR
Interassay variability of immunometric methods for thyrotropin in an external quality assessment survey: evidence that functional sensitivity is not always adequate for clinical decisions
Cosmological Rescaling through Warped Space
We discuss a scenario where at least part of the homogeneity on a brane world
can be directly related to the hierarchy problem through warped space. We study
the dynamics of an anti-D3-brane moving toward the infrared cut-off of a warped
background. After a region described by the DBI action, the self-energy of the
anti-D3-brane will dominate over the background. Then the world-volume scale of
the anti-D3-brane is no longer comoving with the background geometry. After it
settles down in the infrared end, the world-volume inhomogeneity will appear,
to a Poincare observer, to be stretched by an exponentially large ratio. This
ratio is close to that of the hierarchy problem between the gravitational and
electroweak scales.Comment: 12 pages, 2 figures; v2, PRD version, comments and references adde
Analytical performances achieved by the ‘Aria II’ automatic system in an interlaboratory survey triiodothyronine and thyroxine assays
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