84 citations · 167 across the 16 of their papers we have counts for
17 papers
Search for Compact Binary Coalescences with Sub-solar Mass Components in Data from the Second Part of LIGO-Virgo-KAGRA's Fourth Observing Run
The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1816
We report on a gravitational wave search for compact binary coalescences with secondary mass between 0.2 M and 1 M and primary mass between 0.2 M and 10 M, restricting the componen…
A Hint of a Low-Energy Excess in Cosmic-Ray Fluorine
M. J. Boschini, S. Della Torre, M. Gervasi +11
Since its launch, the Alpha Magnetic Spectrometer-02 (AMS-02) has delivered outstanding quality measurements of the spectra of cosmic-ray (CR) species, , , and nu…
The HelMod Monte Carlo Model for the Propagation of Cosmic Rays in Heliosphere
Matteo J. Boschini, Stefano Della Torre, Massimo Gervasi +6
The heliospheric modulation model HelMod solve the transport-equation for the Galactic Cosmic Rays propagation through the heliosphere down to Earth. It is based on a 2-D Monte Car…
Precision measurement of the (e + e) flux in primary cosmic rays from 0.5 GeV to 1 TeV with the Alpha Magnetic Spectrometer on the International Space Station
Manuela Vecchi
We present a precise measurement of the combined electron plus positron flux from 0.5 GeV to 1 TeV, based on the analysis of the data collected by the Alpha Magnetic Spectrometer d…
Precision Measurement of the Proton Flux in Primary Cosmic Rays from 1 GV to 1.8 TV with the Alpha Magnetic Spectrometer on the International Space Station
Cristina Consolandi
A precision measurement of the proton flux in primary cosmic rays with rigidity from 1 GV to 1.8 TV is presented based on 300 million events. The results show that the proton flux…
Results on Solar Physics from AMS-02
S. Della Torre, AMS-02 Collaboration
AMS-02 is a wide acceptance high-energy physics experiment installed on the International Space Station in May 2011 and operating continuously since then. Using the largest number…
Cosmic Rays Propagation with HelMod: Difference between forward-in-time and backward-in-time approaches
S. Della Torre, P. Bobik, M. J. Boschini +9
The cosmic rays modulation inside the heliosphere is well described by a transport equation introduced by Parker in 1965. To solve this equation several approaches were followed in…
Pulsar Wind Nebulae as a source of the observed electron and positron excess at high energy: the case of Vela-X
S. Della Torre, M. Gervasi, P. G. Rancoita +2
We investigate, in terms of production from pulsars and their nebulae, the cosmic ray positron and electron fluxes above GeV, observed by the AMS-02 experiment up to 1 TeV…
Possible Contribution to Electron and Positron Fluxes from Pulsars and their Nebulae
S Della Torre, M Gervasi, PG Rancoita +2
The AMS-02 experiment confirms the excess of positrons in cosmic rays (CRs) for energy above 10 GeV with respect to the secondary production of positrons in the interstellar medium…
On the Contribution of Pulsars to the Positron Fraction in Cosmic Rays
S. Della Torre, M. Gervasi, P. G. Rancoita +2
Several cosmic ray experiments have measured the positron fraction up to few hundred GeV. Their data have revealed an excess of positrons above 10 GeV that is not consistent with t…
Latitudinal Dependence of Cosmic Rays Modulation at 1 AU and Interplanetary-Magnetic-Field Polar Correction
P. Bobik, G. Boella, M. J. Boschini +9
The cosmic rays differential intensity inside the heliosphere, for energy below 30 GeV/nuc, depends on solar activity and interplanetary magnetic field polarity. This variation, te…
Heliosphere Dimension and Cosmic Ray Modulation
P. Bobik, M. J. Boschini, C. Consolandi +8
The differential intensities of Cosmic Rays at Earth were calculated using a 2D stochastic Montecarlo diffusion code and compared with observation data. We evaluated the effect of…
Systematic Investigation of Solar Modulation of Galactic Protons for Solar Cycle 23 using a Monte Carlo Approach with Particle Drift Effects and Latitudinal Dependence
P. Bobik, G. Boella, M. J. Boschini +8
A propagation model of galactic cosmic protons through the Heliosphere was implemented using a 2-D Monte Carlo approach to determine the differential intensities of protons during…
Antiproton modulation in the Heliosphere and AMS-02 antiproton over proton ratio prediction
P. Bobik, M. J. Boschini, C. Consolandi +6
We implemented a quasi time-dependent 2D stochastic model of solar modulation describing the transport of cosmic rays (CR) in the heliosphere. Our code can modulate the Local Inter…
Proton and antiproton modulation in the heliosphere for different solar conditions and AMS-02 measurements prediction
P. Bobik, M. J. Boschini, C. Consolandi +6
Galactic Cosmic Rays (GCRs) are mainly protons confined in the galactic magnetic field to form an isotropic flux inside the galaxy. Before reaching the Earth orbit they enter the H…
Electron and Positron solar modulation and prediction for AMS-02
P. Bobik, M. J. Boschini, C. Consolandi +6
The solar modulation, a combination of diffusion, convection, magnetic drift and energy loss inside the heliosphere is usually seen as a depletion in the Galactic cosmic ray (CR) f…
Proton Modulation in the Heliosphere for Different Solar Conditions and Prediction for AMS-02
P. Bobik, G. Boella, M. J. Boschini +9
Spectra of Galactic Cosmic Rays (GCRs) measured at the Earth are the combination of several processes: sources production and acceleration, propagation in the interstellar medium a…