Methods and stability tests associated with the sterile neutrino search using improved high-energy νμ event reconstruction in IceCube
Physical Review D American Physical Society (APS) 110:9 (2024) 092009
Exploration of mass splitting and muon/tau mixing parameters for an eV-scale sterile neutrino with IceCube
Physics Letters B Elsevier 858 (2024) 139077
Percolating cosmic string networks from kination
Phys. Rev. D 110 (2024) 8, 083537
Abstract:
We describe a new mechanism, whose ingredients are realized in string compactifications, for the formation of cosmic (super)string networks. Oscillating string loops grow when their tension μ decreases with time. If 2H+μ'/μ<0, where H
is the Hubble parameter and μ' denotes the time derivative of the tension, loops grow faster than the scale factor and an initial population of isolated small loops (for example, produced by nucleation) can grow, percolate, and form a network. This condition is satisfied for fundamental strings in the background of a kinating volume modulus rolling toward the asymptotic large volume region of moduli space. Such long kination epochs are motivated in string cosmology by both the electroweak hierarchy problem and the need to solve the overshoot problem. The tension of such a network today is set by the final vacuum; for phenomenologically appealing large volume scenario vacua, this would lead to a fundamental string network with Gμ∼10^(-10).
is the Hubble parameter and μ' denotes the time derivative of the tension, loops grow faster than the scale factor and an initial population of isolated small loops (for example, produced by nucleation) can grow, percolate, and form a network. This condition is satisfied for fundamental strings in the background of a kinating volume modulus rolling toward the asymptotic large volume region of moduli space. Such long kination epochs are motivated in string cosmology by both the electroweak hierarchy problem and the need to solve the overshoot problem. The tension of such a network today is set by the final vacuum; for phenomenologically appealing large volume scenario vacua, this would lead to a fundamental string network with Gμ∼10^(-10).
Percolating cosmic string networks from kination
Physical Review D: Particles, Fields, Gravitation and Cosmology American Physical Society 110 (2024) 083537
Abstract:
We describe a new mechanism, whose ingredients are realised in string compactifications, for the formation of cosmic (super)string networks. Oscillating string loops grow when their tension µ decreases with time. If 2H + ˙µ/µ < 0, where H is the Hubble parameter, loops grow faster than the scale factor and an initial population of isolated small loops (for example, produced by nucleation) can grow, percolate and form a network. This condition is satisfied for fundamental strings in the background of a kinating volume modulus rolling towards the asymptotic large volume region of moduli space. Such long kination epochs are motivated in string cosmology by both the electroweak hierarchy problem and the need to solve the overshoot problem. The tension of such a network today is set by the final vacuum; for phenomenologically appealing Large Volume Scenario (LVS) vacua, this would lead to a fundamental string network with Gµ ∼ 10−10.Discovering neutrino tridents at the Large Hadron Collider
Physical Review D American Physical Society 110:7 (2024) 72018