Probing Dark Energy via Neutrino & Supernova Observatories
Lawrence J. Hall, Hitoshi Murayama, Michele Papucci, Gilad Perez
Abstract
A novel method for extracting cosmological evolution parameters is proposed, using a probe other than light: future observations of the diffuse anti-neutrino flux emitted from core-collapse supernovae (SNe), combined with the SN rate extracted from future SN surveys. The relic SN neutrino differential flux can be extracted by using future neutrino detectors such as Gadolinium-enriched, megaton, water detectors or 100-kiloton detectors of liquid Argon or liquid scintillator. The core-collapse SN rate can be reconstructed from direct observation of SN explosions using future precision observatories. Our method, by itself, cannot compete with the accuracy of the optical-based measurements but may serve as an important consistency check as well as a source of complementary information. The proposal does not require construction of a dedicated experiment, but rather relies on future experiments proposed for other purposes.
Create a lesson
Related papers
First-principle predictions of fragmentation functions via quantum computing
Juan J. Gálvez-Viruet, Felipe J. Llanes-Estrada, Nicolas M. Arenaza et al.
High energy thermal photons from chirally imbalanced QGP
Sourav Duari, Nilanjan Chaudhuri, Pradip Roy et al.
Spin-dependent fermion potentials from mixed tensor couplings of massive spin-1 and spin-2 bosons
D. Khadka, V. V. Flambaum
Building a Better Beta: Nucleation and Timescales in Cosmological Phase Transitions
William Searle, Csaba Balázs
Quantum Steering Geometry at High Energy Particle Colliders
Juan J. Mejia Alvarez, Andrew J. Wildridge, Angelo Arisi et al.
Quantum-statistical effects of bosonic warm dark matter in microscopic interacting dark sectors
Zhijian Zhang