59 research outputs found
Expanding Space: the Root of all Evil?
While it remains the staple of virtually all cosmological teaching, the
concept of expanding space in explaining the increasing separation of galaxies
has recently come under fire as a dangerous idea whose application leads to the
development of confusion and the establishment of misconceptions. In this
paper, we develop a notion of expanding space that is completely valid as a
framework for the description of the evolution of the universe and whose
application allows an intuitive understanding of the influence of universal
expansion. We also demonstrate how arguments against the concept in general
have failed thus far, as they imbue expanding space with physical properties
not consistent with the expectations of general relativity.Comment: 8 pages, accepted for publication in PAS
Cosmological Radar Ranging in an Expanding Universe
While modern cosmology, founded in the language of general relativity, is
almost a century old, the meaning of the expansion of space is still being
debated. In this paper, the question of radar ranging in an expanding universe
is examined, focusing upon light travel times during the ranging; it has
recently been claimed that this proves that space physically expands. We
generalize the problem into considering the return journey of an accelerating
rocketeer, showing that while this agrees with expectations of special
relativity for an empty universe, distinct differences occur when the universe
contains matter. We conclude that this does not require the expansion of space
to be a physical phenomenon, rather that we cannot neglect the influence of
matter, seen through the laws of general relativity, when considering motions
on cosmic scales.Comment: 6 Pages. To appear in MNRA
Halo Mass Functions in Early Dark Energy Cosmologies
We examine the linear density contrast at collapse time, for
large-scale structure in dynamical dark energy cosmologies, including models
with early dark energy. Contrary to previous results, we find that as long as
dark energy is homogeneous on small scales, is insensitive to dark
energy properties for parameter values fitting current data, including the case
of early dark energy. This is significant since using the correct is
crucial for accurate Press-Schechter prediction of the halo mass function.
Previous results have found an apparent failing of the extended Press-Schechter
approach (Sheth-Tormen) for early dark energy. Our calculations demonstrate
that with the correct the accuracy of this approach is restored. We
discuss the significance of this result for the halo mass function and examine
what dark energy physics would be needed to cause significant change in
, and the observational signatures this would leave.Comment: 5 pages, 2 figures. Accepted for MNRAS Letter
Fractal Bubble Cosmology: A concordant cosmological model?
The Fractal Bubble model has been proposed as a viable cosmology that does
not require dark energy to account for cosmic acceleration, but rather
attributes its observational signature to the formation of structure. In this
paper it is demonstrated that, in contrast to previous findings, this model is
not a good fit to cosmological supernovae data; there is significant tension in
the best fit parameters obtained from different samples, whereas LCDM is able
to fit all datasets consistently. Furthermore, the concordance between galaxy
clustering scales and data from the cosmic microwave background is not achieved
with the most recent supernova compilations. The validity of the FB formalism
as a sound cosmological model is further challenged as it is shown that
previous studies of this model achieve concordance by requiring a value for the
present day Hubble constant that is derived from supernovae data containing an
arbitrary distance normalisation.Comment: 6 pages, 3 figures, revised version published in MNRAS letter
The PAndAS view of the andromeda satellite system. I. A Bayesian search for dwarf galaxies using spatial and color-magnitude information
We present a generic algorithm to search for dwarf galaxies in photometric catalogs and apply it to the Pan-Andromeda Archaeological Survey (PAndAS). The algorithm is developed in a Bayesian framework and, contrary to most dwarf galaxy search codes, make
On the origin of the Monoceros Ring - I. Kinematics, proper motions, and the nature of the progenitor
TheMonoceros Ring (MRi) structure is an apparent stellar overdensity that has been postulated to entirely encircle the Galactic plane and has been variously described as being due to lineof- sight effects of the Galactic warp and flare or of extragalactic origin (via accretion). Despite being intensely scrutinized in the literature for more than a decade, no studies to date have been able to definitively uncover its origins. Here we use N-body simulations and a genetic algorithm to explore the parameter space for the initial position, orbital parameters, and, for the first time, the final location of a satellite progenitor. We fit our models to the latest Pan-STARRS data to determine whether an accretion scenario is capable of producing an inplane ring-like structure matching the known parameters of the MRi. Our simulations produce streams that closely match the location, proper motion, and kinematics of the MRi structure. However, we are not able to reproduce the mass estimates from earlier studies based on Pan- STARRS data. Furthermore, in contrast to earlier studies, our best-fitting models are those for progenitors on retrograde orbits. If the MRi was produced by satellite accretion, we find that its progenitor has an initial mass upper limit of ~ 1010M⊙ and the remnant is likely located behind the Galactic bulge, making it difficult to locate observationally. While our models produce realistic MRi-like structures, we cannot definitively conclude that the MRi was produced by the accretion of a satellite galaxy.RRL acknowledges support by the Chilean Ministry of Economy,
Development, and Tourism’s Millennium Science Initiative
through grant IC120009, awarded to the Millennium Institute of
Astrophysics (MAS). RRL also acknowledges support from the
STFC/Newton Fund ST/M007995/1 and the CONICYT/Newton
Fund DPI20140114. BCC acknowledges the support of the
Australian Research Council through Discovery project
DP150100862. AYQH was supported by a National Science
Foundation Graduate Research Fellowship under Grant No.
DGE-1144469. The authors acknowledge the University of Sydney
HPC service at the University of Sydney for providing HPC
resources that have contributed to the research results reported
within this paper
Young accreted globular clusters in the outer halo of M31
We report on observations of two newly discovered globular clusters in the outskirts of M31 made using the Gemini Multi-Object Spectrograph (GMOS) instrument on Gemini North. These objects, PAndAS-7 (PA-7) and PAndAS-8 (PA-8), lie at a galactocentric radius of 87 kpc and are projected, with separation 19 kpc, on to a field halo substructure known as the South-West Cloud. We measure radial velocities for the two clusters which confirm that they are almost certainly physically associated with this feature. Colour-magnitude diagrams reveal strikingly short, exclusively red horizontal branches in both PA-7 and PA-8; both also have photometric [Fe/H]=-1.35±0.15. At this metallicity, the morphology of the horizontal branch is maximally sensitive to age, and we use the distinctive configurations seen in PA-7 and PA-8 to demonstrate that both objects are very likely to be at least 2 Gyr younger than the oldest Milky Way globular clusters. Our observations provide strong evidence for young globular clusters being accreted into the remote outer regions of M31 in a manner entirely consistent with the established picture for the Milky Way, and add credence to the idea that similar processes play a central role in determining the composition of globular cluster systems in large spiral galaxies in general
Argos - III. Stellar populations in the galactic bulge of the milky way
We present the metallicity results from the ARGOS spectroscopic survey of the Galactic bulge. Our aim is to understand the formation of the Galactic bulge: did it form via mergers, as expected from Λ cold dark matter theory, or from disc instabilities,
ARGOS - IV. The kinematics of the Milky Way bulge
We present the kinematic results from our ARGOS spectroscopic survey of the Galactic bulge of the Milky Way. Our aim is to understand the formation of the Galactic bulge. We examine the kinematics of about 17 400 stars in the bulge located within 3.5 kp
Newly discovered globular clusters in NGC 147 and NGC 185 from PAndAS
Using data from the Pan-Andromeda Archaeological Survey (PAndAS), we have discovered four new globular clusters (GCs) associated with the M31 dwarf elliptical (dE) satellites NGC 147 and NGC 185. Three of these are associated with NGC 147 and one with NG
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