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High-energy and ultra-high-energy neutrinos: A Snowmass white paper
Astrophysical neutrinos are excellent probes of astroparticle physics and high-energy
physics. With energies far beyond solar, supernovae, atmospheric, and accelerator …
physics. With energies far beyond solar, supernovae, atmospheric, and accelerator …
No νs is good news
A bstract The baryon acoustic oscillation (BAO) analysis from the first year of data from the
Dark Energy Spectroscopic Instrument (DESI), when combined with data from the cosmic …
Dark Energy Spectroscopic Instrument (DESI), when combined with data from the cosmic …
Snowmass white paper: beyond the standard model effects on neutrino flavor: Submitted to the proceedings of the US community study on the future of particle …
Neutrinos are one of the most promising messengers for signals of new physics Beyond the
Standard Model (BSM). On the theoretical side, their elusive nature, combined with their …
Standard Model (BSM). On the theoretical side, their elusive nature, combined with their …
Looking forward to lepton-flavor-violating ALPs
A bstract We assess the status of past and future experiments on lepton flavor violating (LFV)
muon and tau decays into a light, invisible, axion-like particle (ALP), a. We propose a new …
muon and tau decays into a light, invisible, axion-like particle (ALP), a. We propose a new …
Critical look at the cosmological neutrino mass bound
Cosmological neutrino mass bounds are becoming increasingly stringent. The latest limit
within Λ CDM from Planck 2018+ ACT lensing+ DESI is∑ m ν< 0.072 eV at 95% CL, very …
within Λ CDM from Planck 2018+ ACT lensing+ DESI is∑ m ν< 0.072 eV at 95% CL, very …
Updated neutrino mass constraints from galaxy clustering and CMB lensing-galaxy cross-correlation measurements
We revisit cosmological constraints on the sum of the neutrino masses Σ m ν from a
combination of full-shape BOSS galaxy clustering [P (k)] data and measurements of the …
combination of full-shape BOSS galaxy clustering [P (k)] data and measurements of the …
Updating neutrino mass constraints with background measurements
Low-redshift probes, such as baryon acoustic oscillations (BAO) and supernovae Ia
luminosity distances, have been shown to be crucial for improving the bounds on the total …
luminosity distances, have been shown to be crucial for improving the bounds on the total …
Tau neutrinos in the next decade: from GeV to EeV
Tau neutrinos are the least studied particle in the standard model. This whitepaper
discusses the current and expected upcoming status of tau neutrino physics with attention to …
discusses the current and expected upcoming status of tau neutrino physics with attention to …
Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations
The recent DESI Baryon Acoustic Oscillation measurements have led to tight upper limits on
the neutrino mass sum, potentially in tension with oscillation constraints requiring $\sum m …
the neutrino mass sum, potentially in tension with oscillation constraints requiring $\sum m …
Precision CMB constraints on eV-scale bosons coupled to neutrinos
The cosmic microwave background (CMB) has proven to be an invaluable tool for studying
the properties and interactions of neutrinos, providing insight not only into the sum of …
the properties and interactions of neutrinos, providing insight not only into the sum of …