From the Realm of the Nebulae to Populations of Galaxies
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Unveiling dark fifth forces with linear cosmology
Published in Journal of Cosmology and Astroparticle Physics
We initiate the exploration of the cosmology of dark fifth forces: new forces acting solely on Dark Matter. We focus on long range interactions which lead to an effective violation of the Equivalence Principle on cosmological scales today. At the microscopic level, the dark fifth force can be realized by a light scalar with mass smaller than the Hu...
Phases of Pseudo-Nambu-Goldstone Bosons
We study the vacuum dynamics of pseudo-Nambu-Goldstone bosons (pNGBs) for $SO(N+1) \rightarrow SO(N)$ spontaneous and explicit symmetry breaking. We determine the magnitude of explicit symmetry breaking consistent with an EFT description of the effective potential at zero and finite temperatures. We expose and clarify novel additional vacuum transi...
Disk elution method for MICs and MBCs.
Published in Antimicrobial agents and chemotherapy
A MIC macrodilution broth method in which routine antimicrobial susceptibility testing disks were used as a source of antibiotic was compared with the M7A reference method of the National Committee for Clinical Laboratory Standards for accuracy and reproducibility over five test runs. Gentamicin, piperacillin, and oxacillin were tested by using Ame...
Gaia Data Release 3: The extragalactic content
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The Gaia Galactic survey mission is designed and optimized to obtain astrometry, photometry, and spectroscopy of nearly two billion stars in our Galaxy. Yet as an all-sky multi-epoch survey, Gaia also observes several million extragalactic objects down to a magnitude of G~21 mag. Due to the nature of the Gaia onboard selection algorithms, these are...
Gaia Data Release 3: Chemical cartography of the Milky Way
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Gaia DR3 opens a new era of all-sky spectral analysis of stellar populations thanks to the nearly 5.6 million stars observed by the RVS and parametrised by the GSP-spec module. The all-sky Gaia chemical cartography allows a powerful and precise chemo-dynamical view of the Milky Way with unprecedented spatial coverage and statistical robustness. Fir...
Large Scale Limit of the Observed Galaxy Power Spectrum
The large scale limit of the galaxy power spectrum provides a unique window into the early Universe through a possible detection of scale dependent bias produced by primordial non Gaussianities. On such large scales, relativistic effects could become important and be confused for a primordial signal. In this Letter we provide the first consistent e...
Spontaneous baryogenesis from axions with generic couplings
Published in Journal of High Energy Physics
Axion-like particles can source the baryon asymmetry of our Universe through spontaneous baryogenesis. Here we clarify that this is a generic outcome for essentially any coupling of an axion-like particle to the Standard Model, requiring only a non-zero velocity of the classical axion field while baryon or lepton number violating interactions are p...
Constraining the time evolution of the propagation speed of gravitational waves with multimessenger astronomy
Several modified gravity theories predict a possible time variation of the propagation speed of gravitational waves (GW) which could be tested with multimessenger astronomy. For this purpose we derive the relation between the redshift dependence of the propagation speed of GWs and the time delay between the detection of GWs and electromagnetic wave...
Simulation-based inference for stochastic gravitational wave background data analysis
The next generation of space- and ground-based facilities promise to reveal an entirely new picture of the gravitational wave sky: thousands of galactic and extragalactic binary signals, as well as stochastic gravitational wave backgrounds (SGWBs) of unresolved astrophysical and possibly cosmological signals. These will need to be disentangled to a...
