Estimating the carbon footprint of the GRAND project, a multi-decade astrophysics experiment
Clarisse Aujoux,
Kumiko Kotera and
Odile Blanchard ()
Additional contact information
Clarisse Aujoux: IAP - Institut d'Astrophysique de Paris - INSU - CNRS - Institut national des sciences de l'Univers - SU - Sorbonne Université - CNRS - Centre National de la Recherche Scientifique
Kumiko Kotera: VUB - Vrije Universiteit Brussel [Bruxelles], IAP - Institut d'Astrophysique de Paris - INSU - CNRS - Institut national des sciences de l'Univers - SU - Sorbonne Université - CNRS - Centre National de la Recherche Scientifique
Odile Blanchard: GAEL - Laboratoire d'Economie Appliquée de Grenoble - CNRS - Centre National de la Recherche Scientifique - INRAE - Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement - UGA - Université Grenoble Alpes - Grenoble INP - Institut polytechnique de Grenoble - Grenoble Institute of Technology - UGA - Université Grenoble Alpes
Post-Print from HAL
Abstract:
We present a pioneering estimate of the global yearly greenhouse gas emissions of a large-scale Astrophysics experiment over several decades: the Giant Array for Neutrino Detection (GRAND). The project aims at detecting ultra-high energy neutrinos with a 200,000 radio antenna array over 200,000 km as of the 2030s. With a fully transparent methodology based on open source data, we calculate the emissions related to three unavoidable sources: travel, digital technologies and hardware equipment. We find that these emission sources have a different impact depending on the stages of the experiment. Digital technologies and travel prevail for the small-scale prototyping phase (GRANDProto300), whereas hardware equipment (material production and transportation) and data transfer/storage largely outweigh the other emission sources in the large-scale phase (GRAND200k). In the mid-scale phase (GRAND10k), the three sources contribute equally. This study highlights the considerable carbon footprint of a large-scale astrophysics experiment, but also shows that there is room for improvement. We discuss various lines of actions that could be implemented. The GRAND project being still in its prototyping stage, our results provide guidance to the future collaborative practices and instrumental design in order to reduce its carbon footprint.
Keywords: Greenhouse gas emission; Carbon footprint; Climate change; Large-scale astrophysics experiment; Radio-detection (search for similar items in EconPapers)
Date: 2021-09
New Economics Papers: this item is included in nep-ene, nep-env, nep-exp and nep-ppm
Note: View the original document on HAL open archive server: https://hal.science/hal-03228304v1
References: View references in EconPapers View complete reference list from CitEc
Citations:
Published in Astroparticle Physics, 2021, 131 (September), ⟨10.1016/j.astropartphys.2021.102587⟩
Downloads: (external link)
https://hal.science/hal-03228304v1/document (application/pdf)
Related works:
This item may be available elsewhere in EconPapers: Search for items with the same title.
Export reference: BibTeX
RIS (EndNote, ProCite, RefMan)
HTML/Text
Persistent link: https://EconPapers.repec.org/RePEc:hal:journl:hal-03228304
DOI: 10.1016/j.astropartphys.2021.102587
Access Statistics for this paper
More papers in Post-Print from HAL
Bibliographic data for series maintained by CCSD ().