A new experiment called PTOLEMY (Princeton Tritium Observatory for Light, Early-Universe, Massive-Neutrino Yield) is under development at the Princeton Plasma Physics Laboratory with the goal of challenging one of the most fundamental predictions of the Big Bang – the present-day existence of relic neutrinos produced less than one second after the Big Bang. Using a gigantic graphene surface to hold 100 grams of a single-atomic layer of tritium, low noise antennas that sense the radio waves of individual electrons undergoing cyclotron motion, and a massive array of cryogenic sensors that sit at the transition between normal and superconducting states, the PTOLEMY project has the potential to challenge one of the most fundamental predictions...
The standard Big Bang cosmology predicts the existence of an, as yet undetected, relic neutrino back...
International audienceThe hot dense environment of the early universe is known to have produced larg...
This is a report on the status and prospects of the quantification of neutrino properties through th...
The direct detection of relic neutrinos from the Big Bang was proposed in a paper by Steven Weinberg...
The direct detection of relic neutrinos from the Big Bang was proposed in a paper by Steven Weinberg...
The PTOLEMY project aims to develop a scalable design for a Cosmic Neutrino Background (CNB) detecto...
We propose to achieve the proof-of-principle of the PTOLEMY project to directly detect the Cosmic Ne...
The PTOLEMY project aims to develop a scalable design for a Cosmic Neutrino Background (CNB) detecto...
Future direct observations of the Cosmic Neutrino Background (CvB) have the potential to explore a n...
abstract: We study the physics potential of the detection of the Cosmic Neutrino Back- ground via ne...
The cosmic neutrino background (CNB) can be composed of both active and hypothetical sterileneutrino...
When the Dark Matter mass is below the eV-scale, its cosmological occupation number exceeds the ones...
We explore the potential of measurements of cosmological effects, such as neutrino spectral distorti...
Neutrino oscillations have shown that these weakly interacting particles have a non-zero mass. Despi...
The cosmological background of neutrinos thermally produced in the big bang has been definitively (a...
The standard Big Bang cosmology predicts the existence of an, as yet undetected, relic neutrino back...
International audienceThe hot dense environment of the early universe is known to have produced larg...
This is a report on the status and prospects of the quantification of neutrino properties through th...
The direct detection of relic neutrinos from the Big Bang was proposed in a paper by Steven Weinberg...
The direct detection of relic neutrinos from the Big Bang was proposed in a paper by Steven Weinberg...
The PTOLEMY project aims to develop a scalable design for a Cosmic Neutrino Background (CNB) detecto...
We propose to achieve the proof-of-principle of the PTOLEMY project to directly detect the Cosmic Ne...
The PTOLEMY project aims to develop a scalable design for a Cosmic Neutrino Background (CNB) detecto...
Future direct observations of the Cosmic Neutrino Background (CvB) have the potential to explore a n...
abstract: We study the physics potential of the detection of the Cosmic Neutrino Back- ground via ne...
The cosmic neutrino background (CNB) can be composed of both active and hypothetical sterileneutrino...
When the Dark Matter mass is below the eV-scale, its cosmological occupation number exceeds the ones...
We explore the potential of measurements of cosmological effects, such as neutrino spectral distorti...
Neutrino oscillations have shown that these weakly interacting particles have a non-zero mass. Despi...
The cosmological background of neutrinos thermally produced in the big bang has been definitively (a...
The standard Big Bang cosmology predicts the existence of an, as yet undetected, relic neutrino back...
International audienceThe hot dense environment of the early universe is known to have produced larg...
This is a report on the status and prospects of the quantification of neutrino properties through th...