PRESS RELEASE 2024

SUBMARINE CONNECTIONS WITH SARDINIA: THE TERABIT PROJECT GOES LIVE AND STRENGHTENS CANDIDACY FOR ET

Sparkle Bluemed Golfo Aranci

The TeRABIT project enters the execution phase for the network component with the exclusive acquisition of a portion of Sparkle’s BlueMed submarine cable. This will allow to extend GARR-T, the new generation of GARR network, to Sardinia, thus connecting it to the rest of the research network on the national territory.

The TeRABIT project, funded by the NRRP with INFN and OGS as proposers and CINECA and GARR as partners, is creating a digital research infrastructure that integrates a high-performance network with HPC resources and distributed computing to make it available to the entire scientific community.

Thanks to the current acquisition and the use of cutting-edge technologies, it will be possible to exploit the optical spectrum of the BlueMed submarine cable system. This means that there will be more lanes in the fiber, managed by GARR, exclusively for research data traffic. This innovation represents the first step towards achieving dual high-speed fiber optic connectivity in Sardinia, ensuring not only rapid data transmission to the research and university world but also greater redundancy and reliability extending globally.

From a technological point of view, this is a unique result so far in the national panorama, as explained by Massimo Carboni, Chief Technical Officer of GARR: “Thanks to the open cable technology, which offers the possibility to freely manage a wide range of spectrum rather than individual optical signals, this new digital fiber optic bridge will eliminate the distance of the island creating a seamless integration between the GARR-T infrastructure in the peninsula and that of Sardinia, effectively opening a unified optical network throughout the national territory. Today’s is the first stone of the expansion of GARR-T, which will be completed by 2025 and will provide connectivity up to 400 Gbps”.

“We are proud to present this first concrete result today,” commented Mauro Campanella, scientific coordinator of the TeRABIT project. “We are creating a broad-spectrum infrastructure, perfectly harmonized with other ongoing interventions financed by the NRRP. Once operational, the new connection will bring Sardinia’s infrastructure and researchers closer to TeRABIT’s HPC computing systems and to the resources of ICSC, the National Research Center in HPC, Big Data, and Quantum Computing being installed throughout the national territory.”

The new network connection will support the needs of several research infrastructures and laboratories in Sardinia and will strengthen the candidacy of the Sos Enattos area to host the Einstein Telescope, the future infrastructure to be built in Europe dedicated to gravitational waves, a third-generation detector 10 times more sensitive than those currently existing.

Once the expansion is completed, the GARR-T network will guarantee an increase of 5,000 km of fiber optic, reaching a total capacity of approximately 40 Tbps throughout Italy.

BUBBLES OF ULTRACOLD ATOMS TO UNDERSTAND THE QUANTUM VACUUM AND THE UNIVERSE

Bolle 2023

The ultracold atoms lab of the Pitaevskii Center for Bose-Einstein Condensation in Trento reports for the first time the observation of phenomena related to the stability of our universe. The results arise from the collaboration among the National Institute of Optics of Cnr, the Physics Department of the University of Trento, Tifpa-Infn and the University of Newcastle and it has been published in Nature Physics.

In which kind of vacuum is our universe? Modern physics describes our universe as an intricate outcome of the interactions between particles and fields (the electromagnetic one, for example). From a general point of view, our universe could be in a not so stable configuration, known as false vacuum, which has an energy higher than the absolute minimum. So, in principle it could decay to the lowest energy state, the true vacuum, triggered by quantum or thermal fluctuations.

False vacuum decay could take place on very different time scales, depending on the system parameters and it manifests with the appearance of bubbles of true vacuum, similarly to the formation of liquid drops in a gas cooled below the condensation point. This process is strongly related to cosmological phenomena and the research community has dedicated great effort to understand in which kind of vacuum our universe is. Several research groups have developed sophisticated theories to describe this process, and, in the absence of a direct access to the conditions of the Big Bang, table top experimental platforms for testing and simulating these models have been devised.

 Today the first observation of this decay is reported in a study published on Nature Physics and with Alessandro Zenesini (Pitaevskii BEC Center, Istituto nazionale di ottica del Consiglio nazionale delle ricerche e Dipartimento di Fisica dell’Università di Trento, Tifpa Trento Institute for Fundamental Physics and Applications, INFN as first author. Researchers prepared a cloud of sodium atoms in an initial state which looks like a false vacuum. They then measured the time it takes to the system to decay to the real vacuum, under different experimental conditions. After a first comparison with numerical simulations of the system, the authors joined the theory group of Ian Moss, well known cosmologist which has also collaborated with Stephen Hawking, to verify that the most reliable theory of false vacuum decay is compatible with the observations.

Once again, ultracold atoms prove to be an ideal platform for quantum simulation both of the extremely small and the extremely large. “We used the magnetic properties of atoms to create artificial false and true vacuum in an ultra-stable and controllable environment. This exquisite control of the degenerate atomic cloud allows us to study false vacuum decay in different experimental conditions and to compare our results with theoretical predictions.” reports Alessandro Zenesini, Cnr-Ino researcher who collaborated for this research with Giacomo Lamporesi and Alessio Recati from the same institute. 

“False vacuum decay theories were developed more than fifty years ago having in mind processes typical of high-energy and subnuclear physics and cosmology.” says Gabriele Ferrari (UniTrento). “The results are a first step toward the validation of theories which were only on paper, and pave the road to new lines of experimental research on the different aspects of the birth and dynamics of the true vacuum bubble, with also effects on biochemistry and quantum computation.”

This research was funded by Provincia Autonoma di Trento, INFN, MUR, Q@TN, UK Quantum Technologies programme and European Union.

 

 

GREEN LIGHT FROM THE EUROPEAN SPACE AGENCY FOR THE LISA AND ENVISION MISSIONS

eLISA 2arms gws 3 pink

The Scientific Programme Committee (SPC) of the European Space Agency (ESA) today adopted the LISA and EnVision missions. These are respectively the most important space observatory for gravitational waves and a probe that will study the many mysteries still hidden on the planet Venus. The two missions see strong Italian participation with the Italian Space Agency (AS), the National Institute for Nuclear Physics and the University of Trento. The study phase of the two projects has therefore been completed and ESA is now committed to implementing the missions: LISA will be launched in the mid-2030s while EnVision's departure to Venus is currently scheduled for 2031.

 

 

 

EHT UNVEILS NEW IMAGES OF M87*

M87* nel 2018

The scientific collaboration Event Horizon Telescope (EHT), which published the first “photo” of a black hole in 2019, has published new images of M87*, the supermassive black hole at the centre of the Messier 87 galaxy. This time, the images were created from observations taken in April 2018, one year after the data that led to the image released in 2019. Thanks to the contribution of a new telescope, the Greenland Telescope, and to a clearly improved data acquisition rate in all EHT network telescopes, the 2018 observations offer a vision of the source that is independent from the first observations in 2017. The new images were made by an international research group, in which researchers of the National Institute for Astrophysics (INAF), INFN, the University of Naples Federico II and the University of Cagliari participate. They were recently published in the Astronomy & Astrophysics journal. The images reveal a luminous ring, of the same dimensions as the one observed in 2017, which surrounds a deep central depression, the shadow of the black hole, as predicted by general relativity. What is different is the position of the brightest peak of the ring, which has moved by approximately 30° compared to the images from 2017. This is in line with our theoretical understanding of the variability of turbulent material around black holes.

 

EHT Collaboration press release

Paper on Astronomy & Astrophysics


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DESIGN E REALIZZAZIONE
Coordinamento Grafico Uff. Comunicazione F. Cuicchio
Powered by Multimedia Service
REDAZIONE CONTENUTI
Coordinamento Uff. Comunicazione E. Cossi
Realizzazione testi Ufficio Comunicazione

LNF-INFN Servizi di Calcolo
SERVIZIO SISTEMA INFORMATIVO TECNOLOGIE E PORTALE WEB