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A renewed bid to protect burrowing owls is advancing: What changed?

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A renewed bid to protect burrowing owls is advancing: What changed?


Western burrowing owls are diminutive, adorable and goofy—and conservation organizations have renewed calls for the state to protect them before it’s too late.

Now, more than 20 years since a formal request was made, California wildlife officials appear to be listening.

The California Department of Fish and Wildlife recently recommended that state wildlife policymakers consider a petition to list the owls as endangered or threatened.

It’s the first of several steps the native underground nesters need to clear to earn protection under the state Endangered Species Act. It doesn’t mean it’s warranted, but that it could be warranted.

So while the species’ fate is in no way settled, the groups pushing for the designation are hopeful. This petition, submitted in March, has already soared farther than one launched just over 20 years ago.

“We’re kind of in an emergency situation here,” said Jeff Miller, a senior conservation advocate for the Center for Biological Diversity, who penned both petitions. “It would be kind of shocking if they don’t get some kind of protections.”

So what changed?

Conservationists say the situation is even more dire for the owl. They were once one of the state’s most common birds, present “pretty much everywhere” there were open, low-elevation grasslands, according to Miller.

But “we are down to very low numbers,” Miller said. As a breeding species, it’s “difficult, if not impossible, to get back once you lose it from a specific locality.”

Around San Francisco Bay, there are about 25 breeding pairs, down from roughly 1,000 pairs in the region’s South Bay area alone roughly 30 years ago, he said.

Miller describes the owls as “eggs on legs” because their round head and body sit atop long, skinny legs. They stand just 10 inches tall, flash bright-yellow eyes and, as their name suggests, live underground. “They can seem kind of goofy,” Miller said.

Goofiness aside, conservationists say, incorrect assumptions about the owls’ behavior have been righted, and political winds have changed—fueling hope that this petition has a chance.

Habitat loss remains a top concern. Developers often eye owl habitat for condos and golf courses.

Sprawl development and control efforts targeting ground squirrels, whose burrows the owls appropriate, have pushed the owls out of the grasslands they dwell in. Renewable energy projects and, in some cases, agriculture have also infringed on their digs.

Pamela Flick, California program director for Defenders of Wildlife, a co-petitioner, said the best available science shows the owls have vanished or are close to vanishing in nearly 30% of their range in the state, calling it “really, truly concerning.”

Other petitioners include the Burrowing Owl Preservation Society, Urban Bird Foundation, Central Valley Bird Club, and San Bernardino Valley and Santa Clara Valley Audubon societies.

When the first petition was submitted in 2003, it was argued that owls in population strongholds such as the Imperial Valley would simply be able to fly to other places in the state and boost dwindling populations.

That turned out to be incorrect. Miller said decades of banding and tracking the owls has shown they typically don’t set up shop and breed elsewhere if banished from an area.

Two key players in the petition’s future are the state Fish and Game Commission and the California Department of Wildlife. The department implements and enforces rules made by the commission, as well as conducts research to inform the commission’s decisions.

Miller said it was a “very different political climate” when his group and others brought the first petition.

Earlier this year, he told The Times that the commission in its early days managed with hunting and fishing as a top priority. Now, he said, there’s greater emphasis on conserving vulnerable species.

There’s another twist too: Rather than push for statewide protection, Miller said, petitioners are focusing on the most imperiled owl populations. Conservationists are seeking endangered status for owls in the Bay Area, as well as central-western and southwestern California. They’re seeking threatened status for those in the Central Valley and southern desert.

Parceling out ranges could also mitigate pushback. Some of the areas where the owls are doing best—such as the Imperial Valley and the southern Central Valley—are in manipulated agricultural land. “We don’t want to be at odds with an economic interest if we don’t need to be,” Miller said.

Ultimately, the decision would rest with the Fish and Game Commission. It could opt to list certain populations, or none, or go statewide. The birds are not listed under the federal Endangered Species Act.

Conservation groups expect the commission to vote on whether to accept the petition Oct. 10. If it does, the owls will become a “candidate” species, which affords them the same protections as if they were listed under the state Endangered Species Act while a 12- to 18-month status review moves forward.

2024 Los Angeles Times. Distributed by Tribune Content Agency, LLC.

Citation:
A renewed bid to protect burrowing owls is advancing: What changed? (2024, August 5)
retrieved 5 August 2024
from https://phys.org/news/2024-08-renewed-burrowing-owls-advancing.html

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The Higgs particle could have ended the universe by now—here’s why we’re still here

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The Higgs particle could have ended the universe by now—here’s why we’re still here


The Higgs particle could have ended the universe by now – here's why we're still here
Tarantula nebula—a starforming region—seen by the James Webb Space Telescope. Credit: Nasa, ESA, CSA, STScI, Webb ERO Production Team, CC BY-SA

Although our universe may seem stable, having existed for a whopping 13.7 billion years, several experiments suggest that it is at risk—walking on the edge of a very dangerous cliff. And it’s all down to the instability of a single fundamental particle: the Higgs boson.

In new research by me and my colleagues, just accepted for publication in Physical Letters B, we show that some models of the early universe, those which involve objects called light primordial black holes, are unlikely to be right because they would have triggered the Higgs boson to end the cosmos by now.

The Higgs boson is responsible for the mass and interactions of all the particles we know of. That’s because particle masses are a consequence of elementary particles interacting with a field, dubbed the Higgs field. Because the Higgs boson exists, we know that the field exists.

You can think of this field as a perfectly still water bath that we soak in. It has identical properties across the entire universe. This means we observe the same masses and interactions throughout the cosmos. This uniformity has allowed us to observe and describe the same physics over several millennia (astronomers typically look backwards in time).

But the Higgs field isn’t likely to be in the lowest possible energy state it could be in. That means it could theoretically change its state, dropping to a lower energy state in a certain location. If that happened, however, it would alter the laws of physics dramatically.

Such a change would represent what physicists call a phase transition. This is what happens when water turns into vapor, forming bubbles in the process. A phase transition in the Higgs field would similarly create low-energy bubbles of space with completely different physics in them.

In such a bubble, the mass of electrons would suddenly change, and so would its interactions with other particles. Protons and neutrons—which make up the atomic nucleus and are made of quarks—would suddenly dislocate. Essentially, anybody experiencing such a change would likely no longer be able to report it.

Constant risk

Recent measurements of particle masses from the Large Hadron Collider (LHC) at Cern suggest that such an event might be possible. But don’t panic; this may only occur in a few thousand billion billion years after we retire. For this reason, in the corridors of particle physics departments, it is usually said that the universe is not unstable but rather “meta-stable,” because the world’s end will not happen anytime soon.

To form a bubble, the Higgs field needs a good reason. Due to quantum mechanics, the theory which governs the microcosmos of atoms and particles, the energy of the Higgs is always fluctuating. And it is statistically possible (although unlikely, which is why it takes so much time) that the Higgs forms a bubble from time to time.

However, the story is different in the presence of external energy sources like strong gravitational fields or hot plasma (a form of matter made up of charged particles): the field can borrow this energy to form bubbles more easily.

Therefore, although there is no reason to expect that the Higgs field forms numerous bubbles today, a big question in the context of cosmology is whether the extreme environments shortly after the Big Bang could have triggered such bubbling.

However, when the universe was very hot, although energy was available to help form Higgs bubbles, thermal effects also stabilized the Higgs by modifying its quantum properties. Therefore, this heat could not trigger the end of the universe, which is probably why we are still here.

Primordial black holes

In our new research, we showed there is one source of heat, however, that would constantly cause such bubbling (without the stabilizing thermal effects seen in the early days after the Big Bang). That’s primordial black holes, a type of black hole which emerged in the early universe from the collapse of overly dense regions of spacetime. Unlike normal black holes, which form when stars collapse, primordial ones could be tiny—as light as a gram.

The existence of such light black holes is a prediction of many theoretical models that describe the evolution of the cosmos shortly after the Big Bang. This includes some models of inflation, suggesting the universe blew up hugely in size after the Big Bang.

However, proving this existence comes with a big caveat: Stephen Hawking demonstrated in the 1970s that, because of quantum mechanics, black holes evaporate slowly by emitting radiation through their event horizon (a point at which not even light can escape).

Hawking showed that black holes behave like heat sources in the universe, with a temperature inversely proportional to their mass. This means that light black holes are much hotter and evaporate more quickly than massive ones. In particular, if primordial black holes lighter than a few thousand billion grams formed in the early universe (10 billion times smaller than the moon’s mass), as many models suggest, they would have evaporated by now.

In the presence of the Higgs field, such objects would behave like impurities in a fizzy drink—helping the liquid form gas bubbles by contributing to its energy via the effect of gravity (due to the mass of the black hole) and the ambient temperature (due to its Hawking radiation).

When primordial black holes evaporate, they heat the universe locally. They would evolve in the middle of hot spots that could be much hotter than the surrounding universe, but still colder than their typical Hawking temperature. What we showed, using a combination of analytical calculations and numerical simulations, is that, because of the existence of these hot spots, they would constantly cause the Higgs field to bubble.

But we are still here. This means that such objects are highly unlikely to ever have existed. In fact, we should rule out all of the cosmological scenarios predicting their existence.

That’s of course unless we discover some evidence of their past existence in ancient radiation or gravitational waves. If we do, that may be even more exciting. That would indicate that there’s something we don’t know about the Higgs; something that protects it from bubbling in the presence of evaporating primordial black holes. This may, in fact, be brand new particles or forces.

Either way, it is clear that we still have a lot to discover about the universe on the smallest and biggest scales.

More information:
Louis Hamaide et al, Primordial Black Holes Are True Vacuum Nurseries, arXiv (2023). DOI: 10.48550/arxiv.2311.01869

Journal information:
arXiv


Provided by
The Conversation


This article is republished from The Conversation under a Creative Commons license. Read the original article.The Conversation

Citation:
The Higgs particle could have ended the universe by now—here’s why we’re still here (2024, August 5)
retrieved 5 August 2024
from https://phys.org/news/2024-08-higgs-particle-universe.html

This document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no
part may be reproduced without the written permission. The content is provided for information purposes only.





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Researchers identify global hotspots for flows of ‘dirty money’, with Dubai and Hong Kong emerging as focal points

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Researchers identify global hotspots for flows of ‘dirty money’, with Dubai and Hong Kong emerging as focal points


money
Credit: Unsplash/CC0 Public Domain

New research from the University of Sussex, published August 5 has identified a large-scale shift from the UK to what researchers are terming the “Dubai-Kong axis” as a new hotspot for illicit financial flows (IFFs)—money tied to corruption, organized crime and sanctions evasion.

Researchers at the University’s School of Global Studies and Center for the Study of Corruption have revealed significant shifts in the pattern of global IFFs. The research reveals how different types of “dirty money,” funds obtained through activities such as drug trafficking, corruption, fraud, or other criminal enterprises, flows around the world.

Led by Dr. Daniel Haberly, researchers conducted a detailed analysis of multiple datasets over the course of four years. Their new study highlights the intricate links between politics, regulation, and the location of secretive shell companies and bank accounts used by a variety of actors to evade US sanctions, and to enable corruption and different types of criminal activities.

Among their findings is a seemingly large-scale shift in the global epicenter of dirty money networks to Dubai and Hong Kong. The UK has historically been at the center of the global financial system, including for many types of illicit financial flows, and the financial activities of actors in US-sanctioned countries. Meanwhile Panama has long been a preferred financial hub for organized criminal groups.

This now looks to be changing, however, and the Sussex researchers have coined the term “Dubai-Kong axis” to refer to the now leading as well interconnected role of Dubai and Hong Kong in global networks of dirty money.

Key findings from the paper include:

  1. Shift in location of financial networks: Financial networks in countries under U.S. sanctions are moving from major Western financial centers, and above all London, to non-Western hubs, and above all Hong Kong and Dubai—referred to as the “Dubai-Kong axis.” This is due to these cities’ growing importance as financial centers that have strong connections across Asia, the Middle East, and the former USSR, but also maintain strong ties to the West, especially through their historical colonial links to the UK and London.
  2. Legacy of the British Empire: The UK’s direct involvement in many illicit financial activities seems to have decreased. However, its global network of former colonies including Hong Kong and Dubai, as well as territories that it still controls like the British Virgin Islands and Gibraltar, are more important than ever in illicit financial networks.
  3. Organized criminal networks move away from Panama: Evidence suggests that Dubai and Hong Kong are becoming more important in organized criminal financial networks, while Panama’s role has decreased since the Panama Papers were released.
  4. U.S. and China have significant regulatory deficiencies: Offshore jurisdictions still have significant regulatory gaps, but the most important issues are now in the world’s largest economies. Evidence suggests that the U.S. may have surpassed Switzerland as the international banking center of choice for corrupt transactions, with relatively weak anti-money laundering and counter-terrorism measures and significant financial secrecy.

Dr. Haberly commented, “These results tell us that networks of illicit financial activity can adapt quickly to changing regulatory environments, but in a way that is strongly shaped by established global financial connections and the political priorities of those cracking down on them.

“The Dubai-Kong axis has become the location of choice for actors under the highest pressure from the US and its allies, but other types of illicit financial activity have remained centered on the UK and its Overseas Territories or are even moving to the US itself due to its own regulatory lapses at home.

“We see that greater regulation and law enforcement can have an effect, which is good news for policymakers who want to stop their financial centers from being complicit in illicit financial flows. However, regulatory effectiveness hinges on political will, including the willingness of the world’s most powerful countries to put their own affairs in order at home.”

Professor Elizabeth David-Barrett, GI ACE Principal Investigator, noted, “This research provides a solid evidence base on which policymakers can act. The emergence of the Dubai-Kong axis has been the subject of anecdote and speculation until now, and this thorough analysis of global datasets means that we can now much more reliably track the relative rise and fall of centers of dirty money.”

Citation:
Researchers identify global hotspots for flows of ‘dirty money’, with Dubai and Hong Kong emerging as focal points (2024, August 5)
retrieved 5 August 2024
from https://phys.org/news/2024-08-global-hotspots-dirty-money-dubai.html

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Wheat waste: A phosphorus crisis?

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Wheat waste: A phosphorus crisis?


Wheat waste: A phosphorus crisis?
The predicted demands for N and P for the different components of the photosynthetic machinery (i.e. light capture, electron transport and CO2 assimilation). N limitation (green) and P limitation (blue) are predicted to affect different components of photosynthesis. Credit: Food and Energy Security (2024). DOI: 10.1002/fes3.564

Experiments published in Food and Energy Security by scientists at Queen Mary University of London and Royal Botanic Gardens suggest that we are globally wasting huge amounts of phosphorus.

By studying pot-grown wheat plants, they show that wheat uses nitrogen and phosphorus fertilizers at a ratio of 21 atoms of nitrogen to one atom of phosphorus, and any nitrogen or phosphorus outside this ratio is wasted. These findings indicate that significantly reducing phosphorus input would not affect crop yields but would protect biodiversity, cut costs, conserve this vital resource, and improve ecosystem health.

Wheat is a crucial global food crop, providing 20% of human nutrition. Research on pot-grown wheat plants suggests they require nitrogen and phosphorus in a 21:1 ratio. Excess nitrogen or phosphorus is wasted as it does not boost wheat yield. This pattern likely applies to all crops.

Currently, global fertilizer use has N:P ratios of around 2.1:1 to 4.3:1, far exceeding the optimal level. This waste accumulates in soils and water bodies, harming the environment and increasing costs for farmers and consumers.

Unlike nitrogen, phosphorus is a finite resource essential for feeding a growing population. If these findings hold across agriculture, dramatically cutting phosphorus input can benefit farmers, the environment, and society without compromising yields.

Professor Andrew Leitch from Queen Mary University of London said, “Rising fertilizer consumption is driving up food prices. Our research shows we’re using far too much nitrogen relative to phosphorus, leading to waste, pollution, and higher costs.”

Professor Mark Trimmer from Queen Mary University of London added, “Fertilizer runoff is devastating our environment. Reducing phosphorus inputs can significantly improve biodiversity and ecosystem health without affecting crop production.”

Dr. Ilia Leitch at Royal Botanic Gardens Kew commented, “Forty-five percent of flowering plant species are threatened. Excess fertilizer is a major factor. Our study can help farmers reduce fertilizer use, saving money and the environment.”

More information:
S. S. Marques da Silva et al, Nitrogen and phosphorus interactions at a 21 nitrogen:1 phosphorus Redfield‐like ratio impact growth and seed yield in wheat (Triticum aestivum L.), Food and Energy Security (2024). DOI: 10.1002/fes3.564

Citation:
Wheat waste: A phosphorus crisis? (2024, August 5)
retrieved 5 August 2024
from https://phys.org/news/2024-08-wheat-phosphorus-crisis.html

This document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no
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New model refutes leading theory on how Earth’s continents formed

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New model refutes leading theory on how Earth’s continents formed


New model refutes leading theory on how Earth's continents formed
𝑃−𝑋𝐻2𝑂 phase diagrams showing the effect of variably hydrated EAT compositions on the melts’ fO2 (∆FMQ) and H2O contents. Credit: Nature Geoscience (2024). DOI: 10.1038/s41561-024-01489-z

The formation of Earth’s continents billions of years ago set the stage for life to thrive. But scientists disagree over how those land masses formed and if it was through geological processes we still see today.

A recent paper from the University of Illinois Chicago’s David Hernández Uribe in Nature Geoscience adds new information to that debate, poking holes in the leading theory of continent formation. Hernández Uribe used computer models to study the formation of magmas, which is thought to hold clues to the origin of continents.

Magma is the molten substance that, when it cools, forms rocks and minerals. Hernández Uribe looked for magmas that match the compositional signature of rare mineral deposits called zircons that date back to the Archean period of 2.5 to 4 billion years ago, when scientists believed that continents first formed.

Last year, scientists from China and Australia published a paper arguing that Archean zircons could only be formed by subduction—when two tectonic plates collide underwater, pushing land mass to the surface. That process still happens today, causing earthquakes and volcanic eruptions and reshaping the coasts of continents.

But Hernández Uribe, assistant professor of earth and environmental sciences, found that subduction was not necessary to create Archean zircons. Instead, he found that the minerals could form through high pressure and temperatures associated with the melting of the Earth’s thick primordial crust.






“Using my calculations and models, you can get the same signatures for zircons and even provide a better match through the partial melting of the bottom of the crust,” Hernández Uribe said. “So based on these results, we still do not have enough evidence to say which process formed the continents.”

The results also raise uncertainty about when plate tectonics started on Earth. If Earth’s first continents formed by subduction, that meant that continents started moving between 3.6 to 4 billion years ago—as little as 500 million years into the planet’s existence. But the alternative theory of melting crust forming the first continents means that subduction and tectonics could have started much later.

“Our planet is the only planet in the solar system that has active plate tectonics as we know it,” Hernández Uribe said. “And this relates to the origin of life, because how the first continents moved controlled the weather, it controlled the chemistry of the oceans, and all that is related to life.”

More information:
David Hernández-Uribe, Generation of Archaean oxidizing and wet magmas from mafic crustal overthickening, Nature Geoscience (2024). DOI: 10.1038/s41561-024-01489-z

Citation:
New model refutes leading theory on how Earth’s continents formed (2024, August 5)
retrieved 5 August 2024
from https://phys.org/news/2024-08-refutes-theory-earth-continents.html

This document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no
part may be reproduced without the written permission. The content is provided for information purposes only.





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