28-30 March 2023
Mario Royal Kaikan (Chino, Nagano) + Online
Asia/Tokyo timezone

Stochastic Properties of Ultralight Scalar Fields

29 Mar 2023, 09:00
Mario Royal Kaikan (Chino, Nagano) + Online

Mario Royal Kaikan (Chino, Nagano) + Online



Mariangela Lisanti


Ultralight axionlike particles are well-motivated dark matter candidates that are the target of numerous direct detection efforts. In the vicinity of the Solar System, such particles can be treated as oscillating scalar fields. The velocity dispersion of the Milky Way determines a coherence time of about
oscillations, beyond which the amplitude of the axion field fluctuates stochastically. Any analysis of data from an axion direct detection experiment must carefully account for this stochastic behavior to properly interpret the results. This is especially true for experiments sensitive to the gradient of the axion field that are unable to collect data for many coherence times. Indeed, the direction, in addition to the amplitude, of the axion field gradient fluctuates stochastically. I will present a stochastic treatment for the gradient of the axion field, which can be applied to any axion signal, regardless of coherence time. Additionally, I will show that ignoring the stochastic behavior of the gradient of the axion field can potentially result in failure to discover a true axion signal.

Presentation Materials