WIJK BIJ DUURSTEDE (ANP) - Asielzoekers verblijven sinds woensdag in een tijdelijke noodopvang in Wijk bij Duurstede. Ze mogen daar tot eind augustus blijven. Nadat de Utrechtse gemeente eind mei had aangekondigd dat er een opvang zou komen, waren er meerdere ongeregeldheden. Zo werd het gemeentehuis enkele keren vernield.
In een sporthal op het complex Mariënhoeve is plek voor 50 tot 75 asielzoekers.
In een verklaring zegt de waarnemend burgemeester van Wijk bij Duurstede, Petra Doornenbal, dat de noodopvang "verschillende reacties" heeft opgeroepen. "Tegelijkertijd gaat het om mensen die hun huis en land hebben moeten verlaten en hier een veilige plek zoeken. We doen ons best om de opvang goed te organiseren en oog te houden voor de veiligheid en leefbaarheid in de omgeving."
Gnarly, shrivelly celeriac is an unconventional taco filler. But peeled and roasted in Alice Zaslavsky’s recipe, the root vegetable yields an almost carne asada-like flavour
Check out more Alice Zaslavsky recipes
Could it be time to consider the celeriac? If you’re looking for a tasty and left-of-field taco combo for the cooler months that’s full of flavour, low on cost and easily veganised, then it just well might.
Celeriac is firm and fibrous enough to hold its shape under heat, sweet enough to crack some caramelisation, and its centre yields to a creamy and fluffy mashed potato texture when cooked. The flavour is surprisingly meaty, which makes more sense when you consider how the parsley and liquorice notes intensify when caramelised, a bit like a bite of steak with herby sauce, or carne asada with salsa verde.
Continue reading...Forward on the misunderstanding of his role and momentum the four-time champions have put together for a winning World Cup campaign after topping their group
Kai Havertz is recalling the cocktail of feelings that swirled around his head in Budapest three-and-a-half weeks ago. Arsenal could not have lost the Champions League final in more agonising circumstances but the only available option was to straighten up and start smiling. They were due to set off on a bus around Islington for the Premier League trophy parade at 2pm the following day. Was this really the moment to bathe in a million onlookers’ adulation?
“To be honest, it was tough,” says Havertz, whose early goal against Paris Saint-Germain had looked a possible winner for nearly an hour. “After the match, I initially thought we would call the whole thing off. By the next morning, things looked different.”
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Scientists have discovered new evidence that the cosmic structures connecting the universe are much larger than previously predicted—persisting over billions of light years—a finding that challenges a core tenet of cosmology and hints at the possibility of new physics, according to a study published on Wednesday in Nature.
The standard model of cosmology, a well-corroborated framework for understanding the universe that is also known as the Lambda cold dark matter (ΛCDM) model, predicts that the large-scale structure of space looks the same in all areas (homogeneity) and in all directions (isotropy). While there is variation in the distribution of matter on small scales, such as thousands or millions of light years, these distinctions should smooth out into a uniform pattern on the scale of the cosmic web, which is a network of large-scale structures made of dark matter, gas, and galaxies that stretches across the universe.
But in recent years, new observational data has started to hint that galaxies cluster in “preferred directions,” forming distinct structures known as “anisotropies” that are not uniform, even across vast distances. Now, a pair of physicists has discovered that these distinct directions and patterns persist even to the scale of a gigaparsec, which is a unit equal to 3.26 billion light years, possibly signalling “the need for a shift in modern cosmology,” according to their new study.
“The structures observed in the real Universe are significantly larger and more persistent than those formed in state-of-the-art simulations based on the standard model of cosmology,” said authors Francesco Sylos Labini of the Enrico Fermi Research Center in Rome, Italy, and Marco Galoppo of the University of Canterbury in Christchurch, New Zealand, in an email exchange with 404 Media.
“The key advance of our analysis is that it allows this difference to be quantified,” they added. “By measuring the spatial extent and coherence of the observed structures and comparing them directly with theoretical predictions, we found that the discrepancy is statistically highly significant. In other words, the largest structures in the real Universe appear to be substantially larger than expected in standard models of galaxy formation.”
According to existing models, the cosmic web emerged from small density fluctuations in the early universe and gradually developed into large-scale filaments and nodes made of dark matter that gravitationally attract gas, galaxies, and other forms of matter.
Last year, the Dark Energy Spectroscopic Instrument (DESI), a major astronomical survey based in Arizona, released the largest high-resolution 3D map of the universe, which has revolutionized cosmology and allowed scientists to test those theories against observational data.
Labini and Galoppo analyzed the DESI release with statistical tools, including the Angular Distribution of Pairwise Distances (ADPD), which is especially effective for detecting and characterizing large-scale anisotropies in DESI’s dataset.
“The idea was to try to really test whether the idea that isotropies reached very large scales is now supported by data,” said Galoppo in a follow-up call. “Even just five or ten years ago, we didn't really have the data to test on gigaparsec scales. But now, we had a chance, so we decided to take it.”
“What we are able to do is to characterize how large are the largest structures inside this sample” of DESI observations, added Labini in the call.
The results revealed that even in DESI’s super-zoomed-out observations, large-scale structures create preferred directions of galaxy distribution, as opposed to an overall isotropic pattern. This contrasts with expectations derived from the cosmic microwave background, the oldest light in the universe, which suggests that directional correlations should fade rapidly at large scales.
“In the standard model, it's not that there aren’t structures,” said Galoppo in the call. “It is just that they are supposed to be smaller and less persistent than what we found. That's the crux of the matter.”
To that end, DESI is expected to release a new batch of observations within a year, and similar datasets will also be forthcoming from Europe’s Euclid space telescope and the Vera C. Rubin Observatory in Chile in the near term. These new and improved views of the universe will help scientists grapple with just how vast these large-scale structures are, and what that means for our understanding of our cosmic surroundings.
“At present, there is no simple or widely accepted modification of the ΛCDM framework that naturally explains structures of this size while remaining consistent with the observed uniformity of the cosmic microwave background,” Labini and Galoppo wrote over email. “That is precisely why these observations are so interesting: they point to a potentially important gap between theory and observation that deserves further investigation.”
“If future surveys continue to find coherent directional structures on even larger scales, the implications for cosmology would be profound,” they concluded.