AION: An Atom Interferometer Observatory and Network

Authors:

L Badurina, E Bentine, D Blas, K Bongs, D Bortoletto, T Bowcock, K Bridges, W Bowden, O Buchmueller, C Burrage, J Coleman, G Elertas, J Ellis, C Foot, V Gibson, Mg Haehnelt, T Harte, S Hedges, R Hobson, M Holynski, T Jones, M Langlois, S Lellouch, M Lewicki, R Maiolino, P Majewski, S Malik, J March-Russell, C McCabe, D Newbold, B Sauer, U Schneider, I Shipsey, Y Singh, Ma Uchida, T Valenzuela, M van der Grinten, V Vaskonen, J Vossebeld, D Weatherill, I Wilmut

Abstract:

We outline the experimental concept and key scientific capabilities of AION (Atom Interferometer Observatory and Network), a proposed UK-based experimental programme using cold strontium atoms to search for ultra-light dark matter, to explore gravitational waves in the mid-frequency range between the peak sensitivities of the LISA and LIGO/Virgo/ KAGRA/INDIGO/Einstein Telescope/Cosmic Explorer experiments, and to probe other frontiers in fundamental physics. AION would complement other planned searches for dark matter, as well as probe mergers involving intermediate mass black holes and explore early universe cosmology. AION would share many technical features with the MAGIS experimental programme in the US, and synergies would flow from operating AION in a network with this experiment, as well as with other atom interferometer experiments such as MIGA, ZAIGA and ELGAR. Operating AION in a network with other gravitational wave detectors such as LIGO, Virgo and LISA would also offer many synergies.

Cloud computing and the Square Kilometer Array

Authors:

JC Tseng, Newman R

Clustering properties of the CatWISE2020 quasar catalogue and their impact on the cosmic dipole anomaly

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP)

Abstract:

The cosmic dipole anomaly -- the observation of a significant mismatch between the dipole observed in the matter distribution and that expected given the kinematic interpretation of the cosmic microwave background dipole -- poses a serious challenge to the Cosmological Principle upon which the standard model of cosmology rests. Measurements of the dipole in a given sample crucially depend on having control over other large-scale power so as to avoid biases, in particular those potentially caused by correlations among multipoles during fitting, and those by local source clustering. Currently, the most powerful catalogue that exhibits the cosmic dipole anomaly is the sample of 1.6 million mid-infrared quasars derived from CatWISE2020. We therefore analyse clustering properties of this catalogue by performing an inference analysis of large-scale multipoles in real space, and by computing its angular power spectrum on small scales to test for convergence with LCDM. After accounting for the known trend of the quasar number counts with ecliptic latitude, we find that any other large-scale power is consistent with noise, find no evidence for the presence of an octupole ( ) in the data, and quantify the clustering dipole's proportion to be marginal. Our results therefore reaffirm the anomalously high dipole in the distribution of quasars.

Colloquium: The Cosmic Dipole Anomaly

Reviews of Modern Physics American Physical Society

Authors:

Sebastian Von Hausegger, Roya mohayaee, nathan secrest, rameez, Subir Sarkar

Abstract:

The Cosmological Principle, which states that the Universe is homogeneous and isotropic (when averaged on large scales), is the foundational assumption of Friedmann-Lemaitre-Robertson-Walker (FLRW) cosmologies such as the current standard Lambda-Cold-Dark-Matter (ΛCDM) model. This simplification yields an exact solution to the Einstein field equations that relates space and time through a single time-dependent scale factor, which defines cosmological observables such as the Hubble parameter and the cosmological redshift. The validity of the Cosmological Principle, which underpins modern cosmology, can now be rigorously tested with the advent of large, nearly all-sky catalogs of radio galaxies and quasars. Surprisingly, the dipole anisotropy in the large-scale distribution of matter is found to be inconsistent with the expectation from kinematic aberration and Doppler boosting effects in a perturbed FLRW universe, which is the standard interpretation of the observed dipole in the cosmic microwave background (CMB). Although the matter dipole agrees in direction with that of the CMB dipole, it is anomalously larger, demonstrating that either the rest frames in which matter and radiation appear isotropic are not the same, or that there is an unexpected intrinsic anisotropy in at least one of them. This discrepancy now exceeds 5σ in significance. We review these recent findings, as well as the potential biases, systematic issues, and alternate interpretations that have been suggested to help alleviate the tension. We conclude that the cosmic dipole anomaly poses a serious challenge to FLRW cosmology, and the standard ΛCDM model in particular, as an adequate description of our Universe.

Combined CDF and D0 Upper Limits on Standard Model Higgs Boson Production with up to 8.2 fb$^-1$ of Data

Authors:

T Aaltonen, others