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GRAPES

Galactic cosmic RAy Propagation: an Extensive Study

Total Cost €

EC-Contrib. €

Partnership

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Outcomes and
results

GRAPES project word cloud

Explore the words cloud of the GRAPES project. It provides you a very rough idea of what is the project "GRAPES" about.

experimental theoretical exceedingly appealing innovative crs map forefront cr medium energy cta neutrino originate transport physics tight posed conventional homogeneous sky live origin establishing anisotropic knee linear consistent once internationally questions pending pursued mechanism time grapes spectrum describe first observational modeling motivated revealing description diffusion categorized astroparticle researcher anisotropy journey interact gamma fine numerical perfect winds roadmap view sensitivity identification cosmic environment attacking interstellar galaxy observations profound km3net discovery accurate techniques ism galactic propagation models communities unprecedented sources physical where tackled connect fact er complexity simplified compelling rays extra spectra enormous earth self structures simulation

Project "GRAPES" data sheet

The following table provides information about the project.

Coordinator	GRAN SASSO SCIENCE INSTITUTE Organization address address: VIA FRANCESCO CRISPI 7 city: L'AQUILA postcode: 67100 website: n.a. contact info title: n.a. name: n.a. surname: n.a. function: n.a. email: n.a. telephone: n.a. fax: n.a.
Coordinator Country	Italy [IT]
Project website	https://carmeloevoli.github.io/pages/grapes.html
Total cost	180˙277 €
EC max contribution	180˙277 € (100%)
Programme	1. H2020-EU.1.3.2. (Nurturing excellence by means of cross-border and cross-sector mobility)
Code Call	H2020-MSCA-IF-2016
Funding Scheme	MSCA-IF-EF-ST
Starting year	2017
Duration (year-month-day)	from 2017-10-01 to 2019-09-30

Partnership

Take a look of project's partnership.

#	participants	country	role	EC contrib. [€]
1	GRAN SASSO SCIENCE INSTITUTE GRAN SASSO SCIENCE INSTITUTE Organization address address: VIA FRANCESCO CRISPI 7 city: L'AQUILA postcode: 67100 website: n.a. contact info title: n.a. name: n.a. surname: n.a. function: n.a. email: n.a. telephone: n.a. fax: n.a.	IT (L'AQUILA)	coordinator	180˙277.00

Map

Project objective

Where do Cosmic Rays (CRs) originate? How do CRs interact with the environment during their journey to Earth? GRAPES aims at revealing the origin of galactic CRs, 100 years after their discovery, by achieving the most accurate description of CR propagation in the interstellar medium (ISM). More specifically: 1) What is the mechanism of propagation in the Galaxy? Measurements show fine structures in the observed CR spectra, but we have exceedingly simplified transport models. In view of the challenges that recent observations posed to conventional homogeneous CR diffusion models, we will develop the first self-consistent simulation of interstellar CR propagation, including non-linear processes, anisotropic diffusion and galactic winds. 2) Where do CR become extra-galactic? Understanding propagation at the end of the galactic CR spectrum is compelling towards the identification of galactic sources. We will provide an innovative approach able to describe at once the CR spectrum and anisotropy up to the knee energy attacking the pending theoretical and observational challenges. These questions are profound, challenging and appealing and can be efficiently pursued only through a new advance in the complex numerical modeling of galactic CR transport and by establishing a tight collaboration between communities involved in CR physics. We live in exciting years, since for the first time experimental techniques allow (or are going to allow) forefront questions to be tackled with the necessary sensitivity. The enormous discovery potential is further witnessed by the fact that the two most advanced experimental projects categorized by the European Astroparticle priority roadmap are specifically tailored to map the high-energy gamma (CTA) and neutrino (KM3NeT) sky with unprecedented level of detail. It is then the perfect time for a motivated and internationally experienced researcher (ER) to connect theoretical modeling and observations at a high level of physical complexity.

Publications

List of publications.
year	authors and title	journal	last update
2019	Carmelo Evoli, Roberto Aloisio, Pasquale Blasi Galactic cosmic rays after the AMS-02 observations published pages: , ISSN: 2470-0010, DOI: 10.1103/physrevd.99.103023	Physical Review D 99/10	2020-03-06
2020	Carlo Mascaretti, Pasquale Blasi, Carmelo Evoli Atmospheric neutrinos and the knee of the cosmic ray spectrum published pages: 22-29, ISSN: 0927-6505, DOI: 10.1016/j.astropartphys.2019.06.002	Astroparticle Physics 114	2020-03-06
2019	Giorgio Galanti, Fabrizio Tavecchio, Marco Roncadelli, Carmelo Evoli Blazar VHE spectral alterations induced by photonâ€“ALP oscillations published pages: 123-132, ISSN: 0035-8711, DOI: 10.1093/mnras/stz1144	Monthly Notices of the Royal Astronomical Society 487/1	2020-03-06
2019	Stefano Gabici, Carmelo Evoli, Daniele Gaggero, Paolo Lipari, Philipp Mertsch, Elena Orlando, Andrew Strong, Andrea Vittino The origin of Galactic cosmic rays: Challenges to the standard paradigm published pages: 1930022, ISSN: 0218-2718, DOI: 10.1142/s0218271819300222	International Journal of Modern Physics D	2020-03-06
2018	Carmelo Evoli, Pasquale Blasi, Giovanni Morlino, Roberto Aloisio Origin of the Cosmic Ray Galactic Halo Driven by Advected Turbulence and Self-Generated Waves published pages: , ISSN: 0031-9007, DOI: 10.1103/PhysRevLett.121.021102	Physical Review Letters 121/2	2020-03-06
2018	Carmelo Evoli, Daniele Gaggero, Andrea Vittino, Mattia Di Mauro, Dario Grasso, Mario Nicola Mazziotta Cosmic-ray propagation with DRAGON2: II. Nuclear interactions with the interstellar gas published pages: 006-006, ISSN: 1475-7516, DOI: 10.1088/1475-7516/2018/07/006	Journal of Cosmology and Astroparticle Physics 2018/07	2020-03-06
2018	Carmelo Evoli, Tim Linden, Giovanni Morlino Self-generated cosmic-ray confinement in TeV halos: Implications for TeV Î³ -ray emission and the positron excess published pages: , ISSN: 2470-0029, DOI: 10.1103/physrevd.98.063017	Physical Review D 98/6	2020-03-06

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