Marcoccia, Paolo Nardini, Germano Pieroni, Mauro
We analyze the detection prospects for potential Primordial Black Hole Binary (PBHB) populations buried in the Stellar-Origin Black Hole Binary (SOBHB) population inferred by the LVK collaboration. We consider different PBHB population scenarios and several future Gravitational Wave (GW) detectors. To separate the PBHB component from the SOBHB one,...
Buchmüller, Wilfried Domcke, Valerie Schmitz, Kai
Published in
Journal of Cosmology and Astroparticle Physics
Many symmetry breaking patterns in grand unified theories (GUTs) give rise to cosmic strings that eventually decay when pairs of GUT monopoles spontaneously nucleate along the string cores. These strings are known as metastable cosmic strings and have intriguing implications for particle physics and cosmology. In this article, we discuss the curren...
Beltrán Jiménez, Jose Di Dio, Enea Figueruelo, David
Published in
Journal of Cosmology and Astroparticle Physics
Models with pure momentum exchange in the dark sector have been shown to provide a promising scenario to tackle the tension in the clustering inferred from high- and low-redshift probes. A distinctive feature of these models is that only the Euler equation for the dark matter component is modified and the correction is such that the net effect can ...
Durrer, Ruth Kusenko, Alexander
Published in
Journal of Cosmology and Astroparticle Physics
Yukawa interactions can mediate relatively long-range attractive forces between fermions in the early universe. Such a globally attractive interaction creates an instability that can result in the growth of structure in the affected species even during the radiation dominated era. The formation and collapse of fermionic microhalos can create hot fi...
Brax, Philippe van de Bruck, Carsten Di Valentino, Eleonora Giarè, William Trojanowski, Sebastian
We revisit the possibility of using cosmological observations to constrain models that involve interactions between neutrinos and dark matter. We show that small-scale measurements of the cosmic microwave background with a few per cent accuracy are critical to uncover unique signatures from models with tiny couplings that would require a much highe...
Ghanim, Rim
In 2016, POLAR - a polarimeter - was launched on the Tiangong-2 Chinese space lab. It was designed to measure the polarization of the prompt emission of Gamma-Ray Bursts (GRBs). The next-generation GRBs polarimeter, POLAR-2, is set to launch into space in 2026. However, before building the device, performing calibration on the final prototype and u...
Lerendegui-Marco, J. Alcayne, V. Babiano-Suarez, V. Bacak, M. Balibrea-Correa, J. Casanovas, A. Domingo-Pardo, C. de la Fuente, G. Gameiro, B. García-Infantes, F.
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Neutron capture cross-section measurements are fundamental in the study of the slow neutron capture (s-) process of nucleosynthesis and for the development of innovative nuclear technologies. One of the best suited methods to measure radiative neutron capture (n,$\gamma$) cross sections over the full stellar range of interest for all the applicatio...
Perkins, Haille M.L. Ellis, John Fields, Brian D. Hartmann, Dieter H. Liu, Zhenghai McLaughlin, Gail C. Surman, Rebecca Wang, Xilu
Binary neutron star mergers (BNS) produce high-energy emissions from several physically different sources, including a gamma-ray burst (GRB) and its afterglow, a kilonova, and, at late times, a remnant many parsecs in size. Ionizing radiation from these sources can be dangerous for life on Earth-like planets when located too close. Work to date has...
Domcke, Valerie Ema, Yohei Sandner, Stefan
Axion inflation, i.e. an axion-like inflaton coupled to an Abelian gauge field through a Chern-Simons interaction, comes with a rich and testable phenomenology. This is particularly true in the strong backreaction regime, where the gauge field production heavily impacts the axion dynamics. Lattice simulations have recently demonstrated the importan...
Tagliazucchi, Matteo Braglia, Matteo Finelli, Fabio Pieroni, Mauro
Gravitational Waves (GW) sourced by second-order primordial curvature fluctuations are among the favoured models fitting the recent Pulsar Timing Array (PTA) measurement of a Stochastic GW Background (SGWB). We study how spectral distortions (SDs) and anisotropies of the Cosmic Microwave Background (CMB) can constrain such scalar fluctuations. Wher...