I ricercatori hanno utilizzato il telescopio astronomico di Atacama per creare questa nuova mappa della materia oscura. Le aree arancioni mostrano aree di massa elevata; C’è poco o nessun colore viola. Le caratteristiche tipiche sono larghe centinaia di milioni di anni luce. La barra bianca mostra dove la contaminazione della luce dalla polvere nella nostra galassia, la Via Lattea, misurata dal satellite Planck, oscura la visione profonda. La nuova mappa utilizza la luce del fondo cosmico a microonde (CMB) come retroilluminazione per oscurare tutto ciò che si trova tra noi e il Big Bang. “È come una silhouette, ma invece di avere il nero nell’ombra, hai consistenza e grumi di materia nera, come la luce che attraversa uno schermo di tessuto con molti nodi e protuberanze”, ha detto Suzanne Stocks. , direttore dell’ACT e professore di fisica Henry DeWolf Smith di Princeton. “La famosa immagine blu e gialla della CMB è un’istantanea di come appariva l’universo in una singola epoca, circa 13 miliardi di anni fa, e ora ci fornisce informazioni su tutte le epoche”. Credito: collaborazione ACT
La ricerca dell’Atacama Cosmology Telescope Collaboration ha portato a significativi progressi nella comprensione dell’evoluzione dell’universo.
Per migliaia di anni, gli esseri umani sono stati affascinati dai misteri dell’universo.
A differenza degli antichi filosofi che immaginavano l’origine dell’universo, i cosmologi moderni usano strumenti quantitativi per ottenere informazioni sulla sua evoluzione e struttura. La cosmologia moderna inizia all’inizio del XX secolo con lo sviluppo della teoria della relatività generale da parte di Albert Einstein.
Ora, i ricercatori della collaborazione Atacama Astronomical Telescope (ACT) hanno presentato una serie di documenti. IL[{” attribute=””>Astrophysical Journal featuring a groundbreaking new map of dark matter distributed across a quarter of the sky, extending deep into the cosmos, that confirms Einstein’s theory of how massive structures grow and bend light over the 14-billion-year life span of the universe.
The new map uses light from the cosmic microwave background (CMB) essentially as a backlight to silhouette all the matter between us and the Big Bang.
The Atacama Cosmology Telescope in Northern Chile, supported by the National Science Foundation, operated from 2007-2022. The project is led by Princeton University and the University of Pennsylvania — Director Suzanne Staggs at Princeton, Deputy Director Mark Devlin at Penn — with 160 collaborators at 47 institutions. Credit: Mark Devlin, Deputy Director of the Atacama Cosmology Telescope and the Reese Flower Professor of Astronomy at the University of Pennsylvania
“It’s a bit like silhouetting, but instead of just having black in the silhouette, you have texture and lumps of dark matter, as if the light were streaming through a fabric curtain that had lots of knots and bumps in it,” said Suzanne Staggs, director of ACT and Henry DeWolf Smyth Professor of Physics at Princeton University. “The famous blue and yellow CMB image [from 2003] Un’istantanea di come appariva l’universo in un’epoca, circa 13 miliardi di anni fa, ora ci fornisce informazioni su tutte le epoche.
“È un brivido vedere l’invisibile, l’impalcatura della materia oscura che costituisce le nostre galassie visibili costellate di stelle”, ha affermato Joe Dunkley, professore di fisica e scienze astrofisiche, che ha condotto l’analisi per ACT. “In questa nuova immagine, possiamo vedere direttamente l’invisibile rete cosmica di materia oscura che circonda e collega le galassie”.
“In genere, gli astronomi possono misurare solo la luce, quindi vediamo come le galassie sono distribuite in tutto l’universo; queste osservazioni rivelano la distribuzione della massa, e quindi mostrano principalmente come la materia oscura è distribuita nel nostro universo”, ha detto Princeton Charles A. ha detto David Spergel, un giovane professore di astronomia. .
La ricerca dell’Atacama Astronomical Telescope Collaboration è culminata in una nuova mappa della materia oscura distribuita su un quarto dell’intero cielo, raggiungendo le profondità dell’Universo. I risultati forniscono ulteriore supporto alla teoria della relatività generale di Einstein, che è stata la base del Modello standard della cosmologia per più di un secolo, e forniscono nuovi metodi per escludere la materia oscura. Credito: Lucy Reading-Ikanda, Fondazione Simons
“Abbiamo mappato la distribuzione della materia oscura invisibile attraverso il cielo, ed è esattamente ciò che le nostre teorie prevedono”, ha detto il coautore Blake Sherwin, Ph.D. nel 2013. Un alunno di Princeton e professore di cosmologia all’Università di Cambridge, dove guida un nutrito gruppo di ricercatori dell’ACT. “Questa è una prova sbalorditiva che comprendiamo la storia di come la struttura del nostro universo si è evoluta nel corso di miliardi di anni.[{” attribute=””>Big Bang to today.’
He added: “Remarkably, 80% of the mass in the universe is invisible. By mapping the dark matter distribution across the sky to the largest distances, our ACT lensing measurements allow us to clearly see this invisible world.”
“When we proposed this experiment in 2003, we had no idea the full extent of information that could be extracted from our telescope,” said Mark Devlin, the Reese Flower Professor of Astronomy at the University of Pennsylvania and the deputy director of ACT, who was a Princeton postdoc from 1994-1995. “We owe this to the cleverness of the theorists, the many people who built new instruments to make our telescope more sensitive, and the new analysis techniques our team came up with.” This includes a sophisticated new model of ACT’s instrument noise by Princeton graduate student Zach Atkins.
Research by the Atacama Cosmology Telescope collaboration has culminated in a groundbreaking new map of dark matter distributed across a quarter of the entire sky, reaching deep into the cosmos. Findings provide further support to Einstein’s theory of general relativity, which has been the foundation of the standard model of cosmology for more than a century, and offer new methods to demystify dark matter. Credit: Image courtesy of Debra Kellner
Despite making up most of the universe, dark matter has been hard to detect because it doesn’t interact with light or other forms of electromagnetic radiation. As far as we know, dark matter only interacts with gravity.
To track it down, the more than 160 collaborators who have built and gathered data from the National Science Foundation’s Atacama Cosmology Telescope in the high Chilean Andes observed light emanating following the dawn of the universe’s formation, the Big Bang — when the universe was only 380,000 years old. Cosmologists often refer to this diffuse CMB light that fills our entire universe as the “baby picture of the universe.”
The team tracked how the gravitational pull of massive dark matter structures can warp the CMB on its 14-billion-year journey to us, just as antique, lumpy windows bend and distort what we can see through them.
“We’ve made a new mass map using distortions of light left over from the Big Bang,” said Mathew Madhavacheril, a 2016-2018 Princeton postdoc who is the lead author of one of the papers and an assistant professor in physics and astronomy at the University of Pennsylvania. “Remarkably, it provides measurements that show that both the ‘lumpiness’ of the universe, and the rate at which it is growing after 14 billion years of evolution, are just what you’d expect from our standard model of cosmology based on Einstein’s theory of gravity.”
Sherwin added, “Our results also provide new insights into an ongoing debate some have called ‘The Crisis in Cosmology.’” This “crisis” stems from recent measurements that use a different background light, one emitted from stars in galaxies rather than the CMB. These have produced results that suggest the dark matter was not lumpy enough under the standard model of cosmology and led to concerns that the model may be broken. However, the ACT team’s latest results precisely assessed that the vast lumps seen in this image are the exact right size.
“While earlier studies pointed to cracks in the standard cosmological model, our findings provide new reassurance that our fundamental theory of the universe holds true,” said Frank Qu, lead author of one of the papers and a Cambridge graduate student as well as a former Princeton visiting researcher.
“The CMB is famous already for its unparalleled measurements of the primordial state of the universe, so these lensing maps, describing its subsequent evolution, are almost an embarrassment of riches,” said Staggs, whose team built the detectors that gathered this data over the past five years. “We now have a second, very primordial map of the universe. Instead of a ‘crisis,’ I think we have an extraordinary opportunity to use these different data sets together. Our map includes all of the dark matter, going back to the Big Bang, and the other maps are looking back about 9 billion years, giving us a layer that is much closer to us. We can compare the two to learn about the growth of structures in the universe. I think is going to turn out to be really interesting. That the two approaches are getting different measurements is fascinating.”
ACT, which operated for 15 years, was decommissioned in September 2022. Nevertheless, more papers presenting results from the final set of observations are expected to be submitted soon, and the Simons Observatory will conduct future observations at the same site, with a new telescope slated to begin operations in 2024. This new instrument will be capable of mapping the sky almost 10 times faster than ACT.
Of the co-authors on the ACT team’s series of papers, 56 are or have been Princeton researchers. More than 20 scientists who were junior researchers on ACT while at Princeton are now faculty or staff scientists themselves. Lyman Page, Princeton’s James S. McDonnell Distinguished University Professor in Physics, was the former principal investigator of ACT.
This research will be presented at “Future Science with CMB x LSS,” a conference running from April 10-14 at Yukawa Institute for Theoretical Physics, Kyoto University. The pre-print articles highlighted here will appear on the open-access arXiv.org. They have been submitted to the Astrophysical Journal. This work was supported by the U.S. National Science Foundation (AST-0408698, AST-0965625 and AST-1440226 for the ACT project, as well as awards PHY-0355328, PHY-0855887 and PHY-1214379), Princeton University, the University of Pennsylvania, and a Canada Foundation for Innovation award. Team members at the University of Cambridge were supported by the European Research Council.
