1,073 research outputs found
Constructing Collaborative Success for Network Learning: The Story of the Discovery Community Self-Assessment Tool
Ā· Despite conversations about the importance of community collaboration, foundations continue to struggle with how to best frame and support collaborative success.
Ā· Existing tools to assess collaboration may not fit with either a foundationās values or a specific program strategy.
Ā· From a foundation perspective, developing a community self-assessment tool reinforced the idea that collaborative functioning is crucial and deserves attention.
Ā· This article shares a story of the development and initial use of the Discovery Community Self-Assessment Tool as a process of social construction critical to collective action and a possible indicator of network learning
Tackling non-linearities with the effective field theory of dark energy and modified gravity
We present the extension of the effective field theory framework to the
mildly non-linear scales. The effective field theory approach has been
successfully applied to the late time cosmic acceleration phenomenon and it has
been shown to be a powerful method to obtain predictions about cosmological
observables on linear scales. However, mildly non-linear scales need to be
consistently considered when testing gravity theories because a large part of
the data comes from those scales. Thus, non-linear corrections to predictions
on observables coming from the linear analysis can help in discriminating among
different gravity theories. We proceed firstly by identifying the necessary
operators which need to be included in the effective field theory Lagrangian in
order to go beyond the linear order in perturbations and then we construct the
corresponding non-linear action. Moreover, we present the complete recipe to
map any single field dark energy and modified gravity models into the
non-linear effective field theory framework by considering a general action in
the Arnowitt-Deser-Misner formalism. In order to illustrate this recipe we
proceed to map the beyond-Horndeski theory and low-energy Horava gravity into
the effective field theory formalism. As a final step we derived the 4th order
action in term of the curvature perturbation. This allowed us to identify the
non-linear contributions coming from the linear order perturbations which at
the next order act like source terms. Moreover, we confirm that the stability
requirements, ensuring the positivity of the kinetic term and the speed of
propagation for scalar mode, are automatically satisfied once the viability of
the theory is demanded at linear level. The approach we present here will allow
to construct, in a model independent way, all the relevant predictions on
observables at mildly non-linear scales.Comment: 19 pages. Sec IV and Appendix B added. Matches JCAP versio
An Extended action for the effective field theory of dark energy: a stability analysis and a complete guide to the mapping at the basis of EFTCAMB
We present a generalization of the effective field theory (EFT) formalism for
dark energy and modified gravity models to include operators with higher order
spatial derivatives. This allows the extension of the EFT framework to a wider
class of gravity theories such as Horava gravity. We present the corresponding
extended action, both in the EFT and the Arnowitt-Deser-Misner (ADM) formalism,
and proceed to work out a convenient mapping between the two, providing a self
contained and general procedure to translate a given model of gravity into the
EFT language at the basis of the Einstein-Boltzmann solver EFTCAMB. Putting
this mapping at work, we illustrate, for several interesting models of dark
energy and modified gravity, how to express them in the ADM notation and then
map them into the EFT formalism. We also provide for the first time, the full
mapping of GLPV models into the EFT framework. We next perform a thorough
analysis of the physical stability of the generalized EFT action, in absence of
matter components. We work out viability conditions that correspond to the
absence of ghosts and modes that propagate with a negative speed of sound in
the scalar and tensor sector, as well as the absence of tachyonic modes in the
scalar sector. Finally, we extend and generalize the phenomenological basis in
terms of -functions introduced to parametrize Horndeski models, to
cover all theories with higher order spatial derivatives included in our
extended action. We elaborate on the impact of the additional functions on
physical quantities, such as the kinetic term and the speeds of propagation for
scalar and tensor modes.Comment: 36 pages, matches published version, typos correcte
A de Sitter limit analysis for dark energy and modified gravity models
The effective field theory of dark energy and modified gravity is supposed to
well describe, at low energies, the behaviour of the gravity modifications due
to one extra scalar degree of freedom. The usual curvature perturbation is very
useful when studying the conditions for the avoidance of ghost instabilities as
well as the positivity of the squared speeds of propagation for both the scalar
and tensor modes, or the St\"uckelberg field performs perfectly when
investigating the evolution of linear perturbations. We show that the viable
parameters space identified by requiring no-ghost instabilities and positive
squared speeds of propagation does not change by performing a field
redefinition, while the requirement of the avoidance of tachyonic instability
might instead be different. Therefore, we find interesting to associate to the
general modified gravity theory described in the effective field theory
framework, a perturbation field which will inherit the whole properties of the
theory. In the present paper we address the following questions: 1) how can we
define such a field? and 2) what is the mass of such a field as the background
approaches a final de Sitter state? We define a gauge invariant quantity which
identifies the density of the dark energy perturbation field valid for any
background. We derive the mass associated to the gauge invariant dark energy
field on a de Sitter background, which we retain to be still a good
approximation also at very low redshift (). On this background we
also investigate the value of the speed of propagation and we find that there
exist classes of theories which admit a non-vanishing speed of propagation,
even among the Horndeski model, for which in literature it has previously been
found a zero speed. We finally apply our results to specific well known models.Comment: 22 page
The role of the tachyonic instability in Horndeski gravity
The tachyonic instability is associated with the unboundedness of the
Hamiltonian from below and results in an unstable low- regime. In the
cosmological exploration of modified gravity, it is seldom taken into account,
with more focus given to the popular no-ghost and no-gradient conditions. The
latter though are intrinsically high- statements. Here we combine all three
conditions into a full set of requirements that we show to guarantee stability
on the whole range of cosmological scales. We then explore the impact of the
different conditions on the parameter space of scalar-tensor gravity, with
particular emphasis on the no-tachyon one. We focus on Horndeski gravity and
also consider separately the two subclasses of and Generalized Brans
Dicke theories. We identify several interesting features, for instance in the
parameter space of designer on a CDM background, shedding light on
previous findings. When looking at the phenomenological functions and
, associated to the weak lensing and clustering potential respectively, we
find that in the case of Generalized Brans Dicke the no-tachyon condition
clearly cuts models with . This effect is less prevalent in
the Horndeski case due to the larger amount of free functions in the theory.Comment: 9 pages, 4 figures - accepted version by JCA
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