The Gran Sasso Science Institute, located in L’Aquila, Italy, is an international doctoral school and research center focused on Astroparticle Physics, Mathematics, Computer Science, and Social Sciences. GSSI is in L’Aquila, Italy and it currently hosts around 150 PhD students, 40% of whom are international. The GSSI astroparticle research covers several areas, including gravitational-wave (GW), high-energy astrophysics, cosmic-ray (CR) searches and theory, dark matter searches, and neutrino physics. It is one of Europe’s leading centers for multi-messenger research. GSSI scientists are highly engaged in observations, data analysis and the development of modeling of extreme transients to interpret multi-messenger observations. They are at the forefront of activities related to the Virgo detector, as well as in the design and scientific development of next-generation observatories, such as the Einstein Telescope. GSSI also leads the Lunar Gravitational Wave Antenna project and contributes to the LISA mission. Additionally, researchers access major ground- and space-based observatories to detect electromagnetic counterparts of GW events.
Main contact for TNA call: Marica Branchesi
Available expertise
The GSSI is engaged in the study of the physics governing the emission of multi-messenger from compact objects such as neutron stars, black holes (from stellar to supermassive), and white dwarfs. Within the ACME project we provide expertise on:
- on analyzing gravitational wave observations from LIGO, Virgo, and KAGRA and studying the formation, evolution, and demographics of compact objects;
- on observations and modeling electromagnetic signals (optical, X, gamma, VHE) from astrophysical transients’ counterparts of gravitational-wave sources, such as gamma-ray bursts, kilonovae, and supernovae;
- on modeling the gravitational wave signals of inspirals and post-mergers produced by binary black holes for testing General Relativity;
- on modeling the signals emitted by coalescing neutron star systems to study the properties of matter at super-nuclear densities, and on characterizing compact objects in General Relativity and in extended gravity theories;
- on Virgo, the Einstein Telescope (ET) e il Lunar Gravitational Wave Antenna (LGWA), technological, data analysis and science case development;
The other field of research for which GSSI provides expertise is on high-energy cosmic radiation: cosmic rays (CR), neutrinos, and gamma rays. In particular:
- physics behind the mechanisms responsible for the acceleration and propagation of astrophysical particles and, in general, the dynamics of particle-plasma interactions in astrophysical environments;
- observations of CR and gamma rays both from space (DAMPE experiment) and from Earth (Auger experiment),
- development of new detectors for space-based detection of CR, neutrinos, and gamma rays (HERD, NUSES, Crystal Eye experiments).
Available tools and software
galaxyRate
galaxyRate is an open-source code to estimates the merger rate density of binary compact objects and the properties of their host galaxies based on observational scaling relations. Link: https://gitlab.com/Filippo.santoliquido/galaxy_rate_open
cosmoRate
cosmoRate is an open-source code designed to evaluate the property distributions of compact object mergers across the history of the Universe. Link: https://gitlab.com/Filippo.santoliquido/cosmo_rate_public
ARGdf
ARGdf is a few-body code integrator for stellar interactions, collisions, and triples with PN approximations. Code is developed by GGSI but is not public yet. Relevant publications: 10.1051/0004-6361/202038795, 10.1038/s42005-020-0310-x, 10.3847/2041-8213/abdfcd...
SIMPROP
SIMPROP is a Monte Carlo simulation code for modeling the propagation of ultra-high-energy cosmic rays Link: https://github.com/carmeloevoli/SimProp-Sirente
Nbody6++GPU
Nbody6++GPUis a direct N-body code that enables an accurate simulation of star clusters in a one-to-one fashion, taking into account stellar dynamics and stellar evolution of single and binary stars. Link: https://github.com/nbody6ppgpu/Nbody6PPGPU-beijing...
RAVEN
RAVEN (Rapid Association and Visualization Engine) is a software toolkit developed for fast and automated multi-messenger coincidence analysis between gravitational-wave (GW) candidates and high-energy astrophysical transients such as gamma-ray bursts (GRBs). Designed...
NITRATES
NITRATES (NITRogen Analysis Tool for Rapid Event Search) is a data analysis pipeline designed to identify high-energy electromagnetic counterparts to gravitational-wave (GW) events using time-tagged data from the Swift Burst Alert Telescope (BAT). It focuses on...
BAT-GLIMPSE
BAT-GLIMPSE (Gamma-ray Localization using Imaging and Mosaic techniques for Pointing and Slew Epochs) is a real-time data analysis pipeline developed for the Swift Burst Alert Telescope (BAT). Its primary purpose is to detect and localize high-energy transients, such...
MAGGPY
MAGGPY is a Python-based simulation tool designed to model the joint population of gravitational-wave (GW) sources—specifically binary neutron star (BNS) and neutron star–black hole (NSBH) mergers—and short gamma-ray bursts (GRBs). It enables realistic connections...
B-pop
B-pop is a modular, Python-based software package designed to generate realistic populations of binary compact objects—such as binary neutron stars (BNS), neutron star–black hole binaries (NSBH), and binary black holes (BBH)—for use in gravitational-wave (GW)...
GWFish
GWFish is a flexible, open-source software package designed to perform Fisher matrix–based forecasts for gravitational-wave (GW) detector networks. Its primary purpose is to evaluate the expected performance of current and future GW observatories in estimating source...
HERMES
Computational framework for the line of sight integration which creates sky maps in the HEALPix-compatibile format of various galactic radiative processes.…
Tutorials are provided on the following topics:
- Scientific Programming in Modern C++
- Numerical Algorithms in Scientific Applications
- N-body methods to model collisional astrophysical systems (star clusters and galactic nuclei), and semi-analytic approaches to model CBC formation in dense environments.
- GWFish tutorials
- cosmoRate tutorials
Tutorials are available at this link.
Involved scientists