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Sunday, March 22, 2026

  

How young galaxies grew magnetic fields faster than expected





Tata Institute of Fundamental Research
Magnetic fields in collapsing clouds 

image: 

Lower panel shows a collapsing plasma cloud with uniform magnetic field (red).Top Right: Compression alone amplifies the field. Bottom Right: Collapse-driven turbulence accelerates dynamo amplification (also generating a horizontal component (blue)), producing magnetic fields stronger than compression alone.

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Credit: Pallavi Bhat, Anvar Shukurov, Muhammed Irshad and Kandaswamy Subramanian. NASA; SOFIA; HAWC+; A. S. Borlaff/NASA; JPL-Caltech; ESA; Hubble.




How fast can a galaxy build ordered magnetic fields spanning thousands of light-years? Existing theories say several billion years, but observations of galaxies in our universe imply shorter timescales.

In a study published in the Physical Review Letters and highlighted in the Physics magazine, scientists propose an explanation that resolves this contradiction. They say that the collapse of plasma clouds during the formation of galaxies could significantly accelerate the growth of these magnetic fields.

Almost all visible matter in our universe is in the form of plasma, which can be stirred by forces related to gravity, temperature gradients and rotation. If these lead to turbulent flow, the dynamo theory predicts that the existing magnetic fields in the plasma are amplified. The dynamo theory is our primary framework for understanding the origin of cosmic magnetic fields.

“However, dynamo theory has its limitations”, says Pallavi, an assistant professor at the International Centre for Theoretical Sciences (ICTS) and an author of the study. “In particular, it struggles to explain observations of young galaxies with robust magnetic fields across thousands of light-years”. 

The new study explores how dynamos might operate differently during galaxy formation. It considers an ionized gas cloud collapsing under gravity - the stage during which galaxies assemble. “When the galaxy is forming, gravity itself can stir the plasma, which can amplify magnetic fields”, says Irshad, a graduate student at ICTS and the lead author of the paper.
Through analytic calculations, the team was able to show that such stirring of plasma that occurs during the collapse can accelerate the formation of magnetic fields. As a result, the observed magnetic fields could be established significantly faster than was earlier thought. 

The reason for this, they say, is how the turbulent flow of plasma is altered during the collapse. One characteristic of turbulent flows are eddies, not unlike the swirls we see in water streams. How fast the magnetic field grows depends on the ‘turnover rate’ of these eddies — how fast they swirl. 

The team found that this turnover rate increases as the cloud collapses, leading to an accelerated ‘super exponential’ growth in magnetic fields, explaining how magnetic fields could have formed faster in the younger galaxies. Through numerical analysis, the team also showed that the field thus formed is stronger than one would expect from the standard dynamo theory.

In their study, the team uses a mathematical framework called ‘supercomoving coordinates’. In cosmology, this is used to absorb the expansion of the universe. “These coordinates essentially make the equations of a collapsing galaxy the same as a static galaxy, making the calculations very straightforward”, says Irshad. “This works well for a uniformly collapsing spherical system, but we would need to extend this study for more realistic cases”. 

There’s still much to learn in this “zeroth-order question you ask about the timescale” too, says Pallavi. For example, there have been efforts to create computational models for the structure formation in the universe. This study can predict how fast the magnetic fields are set up in the universe, enabling scientists to test and refine their models accordingly, she says.

Although magnetic forces are typically much weaker than gravity in shaping cosmic structures, the new study suggests that strong, ordered magnetic fields may have appeared earlier, slowly nudging the evolution of our universe for longer than we thought.

Spin separates giant planets from ‘failed stars’



Clearest evidence yet that giant planets spin faster than their cosmic lookalikes




Northwestern University




For decades, astronomers have struggled to differentiate giant planets from brown dwarfs, a class of objects more massive than planets but too small to ignite nuclear fusion like true stars. 

Through a telescope, these cosmic lookalikes can have the overlapping brightness, temperatures and even atmospheric fingerprints. The striking similarity leaves astronomers unsure if they have observed an oversized planet or an undersized star.

Now, a Northwestern University-led team has uncovered a crucial clue that separates the two: how fast they spin.

In a new study, astrophysicists found the clearest evidence yet that giant planets spin significantly faster than their brown dwarf counterparts. The new results suggest rotation measurements may provide a powerful new diagnostic for classifying these indistinguishable populations and suggest that these two objects evolve differently, perhaps even forming through distinct processes.

The study will be published on Wednesday (March 18) in The Astronomical Journal. It marks the largest survey of spin measurements of directly imaged extrasolar planets and brown dwarfs to date.

“Spin is a fossil record of how a planet formed,” said Northwestern’s Chih-Chun “Dino” Hsu, who led the study. “By measuring how quickly these worlds rotate, we can start to piece together the physical processes that shaped them tens to hundreds of millions of years ago.”

An expert on exoplanets and brown dwarfs, Hsu is a postdoctoral researcher at Northwestern’s Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA), where he is advised by study coauthor Jason Wang. Wang is an assistant professor of physics and astronomy at Northwestern’s Weinberg College of Arts and Sciences and a member of CIERA.

A cosmic identity crisis

Typically, astronomers can distinguish planets from stars based on a combination of brightness, temperatures and spectral information. But giant planets and brown dwarfs, which are often called “failed stars,” sit right in the blurry middle of this classification system. The size and mass of the largest planets overlap with the size and mass of the smallest brown dwarfs. And because brown dwarfs lack sustained nuclear fusion, they emit a faint glow like giant planets.

The Northwestern team wondered if the objects’ spins could provide a differentiating factor. Using Northwestern’s institutional access to W.M. Keck Observatory on Maunakea in HawaiÊ»i, the astrophysicists analyzed six giant exoplanets and 25 brown dwarfs.

“We were only able to conduct a spectroscopic survey of this scale because Northwestern is a Keck Observatory partner,” Wang said. “That allowed us to access Keck’s telescopes for many nights to make this survey a reality.”

With high-resolution spectroscopy from the Keck Planet Imager and Characterizer Instrument (KPIC), the team isolated light from the faint objects to measure fine details in their atmospheres. As these distant worlds rotate, features in their spectra broaden, much like the Doppler effect for sound. By analyzing those broadened features, scientists can determine how quickly a planet is spinning.

“With KPIC, we can detect these tiny signals that reveal a planet’s rotation around other nearby stars,” Hsu said.

After measuring the spins of the exoplanets and brown dwarfs, the team combined those new measurements with spin measurements from previous studies. This enabled the team to build a larger curated sample of planets, brown dwarfs and related objects for comparison.

When Hsu and his collaborators compared rotation rates across the full sample, a clear pattern emerged. Giant planets tend to rotate at a larger fraction of their theoretical maximum speed — known as their “breakup velocity,” or the point at which an object would tear itself apart from centrifugal force. By contrast, brown dwarfs rotate more slowly.

A new spin on formation

According to the researchers, this difference likely traces back to the objects’ masses and how their mass compares to that of their host stars. Astronomers have long thought that giant planets form within disks of gas and dust surrounding young stars. During formation, interactions with the disk can influence how much angular momentum — or amount of spin — the planet retains.

Brown dwarfs, on the other hand, can form like stars — through the collapse of gas clouds — or like planets. Interactions between the brown dwarf’s strong magnetic field and the surrounding gas act like a cosmic brake, causing the object to lose angular momentum.

One exoplanet and one brown dwarf in Hsu’s study highlight this difference. A giant planet in the HR 8799 exoplanet system is about seven times the mass of Jupiter and spins unusually fast. But a nearby brown dwarf is roughly three times more massive than the giant exoplanet yet rotates six times slower. 

While both objects lost angular momentum during their formation, the spin of the more massive brown dwarf lost significantly more momentum likely due to its stronger magnetic field. The study also found that brown dwarfs orbiting stars rotate even more slowly than isolated brown dwarfs, drifting through space. This possibly reflects different formation environments.

“Our results suggest that both the planet’s mass and the ratio between the planet’s mass and its star’s mass influence how fast the planet ultimately spins,” Hsu said. “That helps us narrow down the physics of how these systems form.”

Next, the research team plans to expand their studies by examining the spins of free-floating planetary-mass objects — rogue worlds that drift through space without a host star — and by investigating the chemical composition of planetary atmospheres across the population.

“We’re just beginning to explore what planetary spin can tell us,” Hsu said. “With future instruments and larger telescopes, we’ll be able to measure spins for even more worlds and connect rotation, chemistry and formation history across entire planetary systems.”

The study, “Distinct rotational evolution of giant planets and brown dwarf companions,” was supported by NASA, the National Science Foundation and the Heising-Simons Foundation.

Monday, March 16, 2026

New Method Reveals Slower Expansion In Our Cosmic Neighborhood



The velocities of galaxies in groups versus distance. Embedded in the expanding Universe the attractive forces of gravity cluster the groups members together and cosmic expansion tears the outer member galaxies away. This balancing act jointly constrains the mass of the gravitationally-bound group and the Hubble constant being the expanding pull.
 Credit: AIP/ D. Benisty / J. Fohlmeister


March 15, 2026 
By Eurasia Review


Two studies were recently published in Astronomy & Astrophysics by an international team including David Benisty from the Leibniz Institute for Astrophysics Potsdam (AIP). Each paper analyzes observational data for a different nearby galaxy group — the Centaurus A group and the M81 group — to determine both their masses and the value of the Hubble constant.

The Hubble constant describes how fast the Universe expands, expressed as a ratio of the recessional velocity to the distance a galaxy has towards us. The Hubble constant is measured in km/s per Megaparsec, 1 Megaparsec being 3.3 million light years.

From the first light in the early Universe, the so-called cosmic microwave background radiation, a precise measurement for the Hubble constant with the value 68 km/s/Mpc was inferred. Using explosions of stars in receding galaxies to measure their distances, another very precise measurement of the Hubble constant could be established from our late, local Universe. However, the value is 73.

This discrepancy between the expansion rates of the early and the late Universe is known as the Hubble tension. Over the last decades, increasingly precise observations have turned this tension into one of the central challenges in cosmology. It questions our understanding of cosmology and fundamental physics.

The new studies shed light onto this tension from a more holistic viewpoint in contrast to the approach based on stellar explosions. While the stellar-explosion method aims to directly track the cosmic expansion, the new studies analyze the motion of galaxies in groups embedded in the expanding Universe. The attractive forces of gravity cluster the groups together and cosmic expansion tears the member galaxies apart. This balancing act jointly constrains the mass of the gravitationally-bound group and the Hubble constant being the expanding pull. Surprisingly, David Benisty from AIP and his collaborators obtained a Hubble constant of about 64 km/s/Mpc. The result suggests that at least part of the Hubble tension may arise from the observations and methods we choose to infer the Hubble constant.

The researchers focused on two galaxy groups: The Centaurus A group is one of the nearest galaxy groups beyond the Milky Way’s own Local Group. It was assumed to be dominated by the giant elliptical galaxy Centaurus A and contains dozens of smaller satellite galaxies. The new analysis showed that the Centaurus A group is not centered around Centaurus A, but forms a binary with the M83 galaxy. The team thus determined the first value of the Hubble constant from this group as a binary and a more accurate mass estimate.

The M81 group is already known to have two galaxies, M81 and M82, in its center. Thanks to the extended dataset, the member galaxies around this binary were found to still form a planar structure, as previously established. The study of the turbulent dynamics shows that is yet so neatly ordered: The inner planar region with distances of less than 1 million light years is tilted by about 34 degrees to the larger-scale environment. At 10 million light years distance, the orientation has turned to align with the larger-scale sheet-like structure that also stretches out to the Centaurus A group.

Most intriguingly, the two galaxy groups do not only share a similar surrounding. They also have in common that the masses of the most luminous member galaxies almost entirely constitute the total group mass and that the motions of all galaxies in their vicinity are equally well described by the interplay between the galaxies’ gravitational attraction and the cosmic pull. Hence, in contrast to simulated galaxy groups which are always embedded in an overall dark-matter halo, the observations of both galaxy groups can be well explained without this additional dark mass.

The team will use this method that gives a comprehensive understanding of structures in our cosmic neighborhood and transfer it to a larger cosmic volume. With new observations at larger distances, coming, for instance, from the 4-metre Multi-Object Spectroscopic Telescope (4MOST), the next data releases may not only bring a resolution to the Hubble tension but also yield a more precise census how much of this puzzling dark kind of matter is in our Universe.

This work was carried out in collaboration with David Benisty (AIP Potsdam), Jenny Wagner (Academia Sinica, Institute of Astronomy and Astrophysics, and University of Helsinki), Adrian Faucher (École Polytechnique), David Mota (University of Oslo), and Igor Karachentsev (Special Astrophysical Observatory, Russian Academy of Sciences).

Tuesday, March 10, 2026

The Ultra-High-Energy Neutrino May Have Begun Its Journey In Blazars


Visualization of the ultra-high-energy neutrino event detected by the KM3NeT/ARCA detector in the Mediterranean Sea. The colored tracks show the Cherenkov light produced as secondary particles travel through the water and are recorded by the detector’s optical modules. 

CREDIT: KM3NeT

March 10, 2026 
By Eurasia Review


Three years ago, in the waters of the Mediterranean Sea, the passage of an “ultra-energetic” cosmic neutrino was observed — the most energetic ever detected. The event drew international attention from the scientific community as well as from the media and the public, not least because the origin of this particle — whose energy exceeded that of previously observed neutrinos by more than an order of magnitude — is unknown.


A new paper published in the Journal of Cosmology and Astroparticle Physics (JCAP) by the KM3NeT collaboration, which operates the KM3NeT/ARCA detector off the coast of Sicily, suggests that the source of this particle may be in a population of blazars — active galactic nuclei hosting a supermassive black hole that emit a plasma jet directed toward Earth.

In search of the “culprit”


KM3NeT/ARCA is a neutrino detector immersed in the depths of the sea off the coast of Sicily, and it may come as a surprise that it is still under construction. Nevertheless, on 13 February 2023 it recorded an extraordinary signal: the passage of a neutrino which, at around 220 PeV, far exceeded the energies of all high-energy neutrinos observed up to that point. The event also caught the scientific community off guard: what could have generated a particle with such exceptional characteristics?

To answer this question, the collaboration worked much like forensic investigators deducing who or what left a particular trace at a crime scene: starting from an initial hypothesis, the authors simulated the events that might have occurred and then compared the results with the actual observations.

The authors’ hypothesis — one among several proposed over the past year — is that the ultra-high-energy neutrino may have been produced in a specific class of blazars. “There are several possible explanations for the origin of this particle,” explains Meriem Bendahman, a researcher at INFN Naples and a member of the KM3NeT collaboration, among the authors of the study, which counts hundreds of contributors. “For example, it has been proposed that such neutrinos are generated when ultra-high-energy cosmic rays interact with the cosmic microwave background radiation, the residual light from the early Universe. But there is also the possibility that the neutrino originates from a diffuse flux produced by a population of extreme accelerators, such as blazars.”

A diffuse source

Bendahman explains that there are reasons to believe the observed neutrino did not originate from a single sudden and identified event — such as an explosion or a flare. In similar cases, scientists look for an electromagnetic “counterpart,” that is, a signal in radio, optical, X-ray or gamma-ray emission coming from the same region of the sky in coincidence with the neutrino detection

In the case of the event three years ago, however, no such electromagnetic counterpart was found. “This does not completely rule out the possibility of a point-like source,” Bendahman notes, “but it leads us to consider that our neutrino may come from a diffuse background — that is, from a flux of neutrinos including contributions from many sources.”

“We therefore simulated a population of blazars using an open-source software called AM3, with physically motivated parameters,” Bendahman explains. To build a realistic model of blazars, the researchers fixed many parameters to values already known from other independent observations, such as the magnetic field strength or the size of the emission region.


In the simulations, they mainly varied two key parameters: the baryonic loading, which indicates how much energy is carried by protons compared to electrons (and therefore how many neutrinos can be produced), and the proton spectral index, which determines how the proton energy is distributed and how likely it is to reach extreme energies.

For each combination of these two parameters, they calculated both the diffuse neutrino flux and the corresponding gamma-ray flux, to be compared with observational data.
The comparison with IceCube and Fermi LAT

One of the strengths of Bendahman and colleagues’ work is its integrated approach: in addition to KM3NeT/ARCA data, the authors also considered observations from the IceCube Neutrino Observatory and the Fermi Gamma-ray Space Telescope. They did not rely only on what had been observed, but also — and perhaps especially — on what these instruments had not observed.

The absence of comparable ultra-high-energy events in existing neutrino datasets, including those from IceCube, suggests that such phenomena are extremely rare. Any viable model must therefore also account for this absence. The proposed scenario satisfies this constraint.

Moreover, since neutrino production is generally accompanied by gamma-ray emission, the authors verified that the contribution from blazars does not exceed the extragalactic gamma-ray background measured by Fermi.

In this way, Bendahman and colleagues showed that a population of blazars is a plausible source of the ultra-high-energy neutrino: “We modelled a realistic population of blazars with physically motivated parameters, and we found that this population of blazars could explain the origin of this ultra-high-energy event, while also being consistent with the constraints that we have regarding the gamma-ray and neutrino observations.”

KM3NeT: the best is yet to come


The hypothesis that a population of blazars may lie at the origin of the event remains promising, but it needs to be tested with new data. “We need more observational data,” explains Bendahman. “KM3NeT is still under construction, and we detected this ultra-high-energy neutrino with only a partial configuration. With the full detector and more data, we will be able to perform more powerful statistical analyses and open a new window on the ultra-high-energy neutrino universe.” At the time of the observation, only 21 detection lines of KM3NeT were active, corresponding to about 10% of the final volume of the apparatus.

If confirmed, this KM3NeT collaboration’s interpretation would provide new insights into the ability of blazars to accelerate particles to even more extreme energies than previously hypothesized. “We have never observed such a high-energy neutrino before, and if it turns out to come from cosmic accelerators like blazars,” Bendahman concludes, “it would give us new insight into how these objects can emit particles at energies beyond what we previously expected.”

Sunday, March 08, 2026

IWD

Source: Originally published by Z. Feel free to share widely.

With fierce anger burning in our hearts and an unbreakable resolve, we mourn the assassination of the courageous feminist and leftist leader and fighter Yanar Mohammed, president of the Organization of Women’s Freedom in Iraq, who was struck down by the hand of darkness in Baghdad on the morning of March 2, 2026 — as though they believed a bullet could extinguish the fire of feminist struggle and liberation. Two gunmen on motorcycles opened fire on her in front of her residence in the Al-Shaab district, in a crime whose perpetrators we all know.

The assassination of Yanar is a fully premeditated political crime targeting the feminist and leftist movements and every voice demanding justice and equality. It is a declaration of war against free women and against all who refuse to submit to the power of repression, sectarianism, and savage patriarchy.

Yanar: An Idea That Took Human Form

Yanar embodied a profound idea at the heart of class and social struggle — the idea that women’s liberation is central to any project of justice. The idea that no true equality exists without dismantling the structures of patriarchal violence protected by political, religious, and tribal authority. The idea that socialism without feminism remains incomplete, and that feminism which fails to confront class exploitation remains limited in its impact.

Yanar opened the doors of her organization to dozens of Iraqi women who sought refuge from domestic and social violence, enabling many of them to break free from forced marriage, denial of education, and deprivation of their rights. Her organization was never merely a human rights office issuing reports and statements — it was a frontline of daily life, receiving hundreds of distress calls every year from women living under crushing violence.

They Targeted Her Because She Was Dangerous to Oppression

They targeted her because she exposed violence, uncovered human trafficking networks, and opened the doors of safe houses to those cast aside by society. They targeted her because she said what no one wanted to hear: that the situation of Iraqi women has been deteriorating for decades, and that occupation and political Islam are two faces of the same coin in producing oppression. Yanar saw that the American invasion had turned Iraqi streets into zones without women, and she exposed the false choice between two options with no third alternative — either occupation or political Islam — insisting that choosing between them meant a life neither free nor dignified.

Her organization faced a campaign by the state media labeling them “those who humiliate Iraqi women,” because she openly raised the issue of human trafficking and demanded that the state recognize victims and ensure their protection. This is a familiar pattern: when a crime is exposed, those who expose it are attacked; when killing goes unaddressed, those who demand justice are accused of damaging the national reputation.

They wanted to intimidate activists and drive women back into the cage of silence. They ignored the reality that Yanar’s voice was never a single voice. It was the echo of tens of thousands of women who learned from her that freedom is seized, not granted.

The Climate That Bred the Crime: Power Is Complicit in Blood

The sectarian, nationalist, and patriarchal government of Iraq bears direct political and moral responsibility for the climate that produced this crime. The quota system that entrenched sectarian and ethnic division, shielded militias, and turned a blind eye to hate speech and violence against women is the incubator for targeting defenders of freedom.

This climate does not produce violence by accident — it manufactures it systematically through three intertwined channels: first, the religious pulpit, which reinforces the image of woman as a dependent being requiring a male guardian to govern and decide on her behalf. Second, the patriarchal media, which distorts the image of activists and portrays them as enemies of religion, family, and nation — thereby granting moral justification for killing in the minds of those who carry it out. Third, the culture of impunity that protects militias and makes political assassination a cost-free instrument.

When feminists are incited against and their reputations smeared without accountability, the bullet becomes an extension of that incitement. The killer executes what the culture of hatred produces daily from pulpits, screens, and mosques.

Impunity: Complicity in Blood

We condemn this cowardly crime and demand the killers be identified and publicly held accountable. The Iraqi Interior Minister has ordered the formation of a specialized investigative team to determine the circumstances of the crime — a step we acknowledge in form, though we will not forget that dozens of human rights and women’s rights defenders were killed in Iraq before Yanar without their killers ever being identified. Impunity is not merely a failure of the judicial system; it is a deliberate political message: activists can be killed, and no one will be held responsible.

There is no justice in a homeland where fighters are assassinated while sectarian and patriarchal structures continue to reproduce violence. Protecting activists is a political obligation that tolerates no delay, and cannot be satisfied by forming investigative committees that save face and bury files.

The Idea That Does Not Die

A bullet pierces the body. The idea endures. Yanar Mohammed was born in Baghdad and was known for her defining words: “We women are capable of knowing what is best for us, our families, and our communities.” This simple sentence is, at its core, a complete revolution against every logic of guardianship and exclusion that governs women within a patriarchal sectarian context that claims to protect them while imprisoning them.

The idea Yanar planted — the idea of liberation, full equality for women, and a socialist future — will take deeper root. It will transform into collective action, into a feminist movement more resolute in confronting violence, discrimination, exploitation, and the system that sustains them. Because every fighter who has fallen throughout the history of feminist and human struggle has not extinguished the movement — she has ignited within it a deeper anger and a stronger resolve. A single bullet does not stop a movement. It kindles within it a new conviction: that what she fought for is worth the sacrifice.

Yes to the Women’s Revolution

A revolution that links women’s liberation to the liberation of society from sectarianism, tyranny, and corruption. A revolution that insists no true equality exists as long as the sectarian constitution elevates religious law above civil law, and as long as women in Iraq lose their rights to custody, marriage, divorce, and inheritance through the decrees of clerics rather than through equal civil law. A revolution that affirms that women’s liberation is the measure of society’s progress and development.

Today we stand at a defining moment: either the movement breaks under the weight of shock, or it reorganizes itself and raises its hand higher. We choose the second. We choose organized anger over helpless despair. We choose to continue until the name Yanar Mohammed becomes a reference point for every Iraqi girl learning the meaning of resistance.

They will not silence our voices. We will raise them higher. We will not be afraid. We will not be silent. We will not compromise on the freedom of women.

Yanar did not die. Death claims bodies — but she who planted freedom in the hearts of thousands walks among us every time a woman raises her voice and refuses silence.

[Yanar Mohammed (1960 — March 2, 2026): architect, founder of the Organization of Women’s Freedom in Iraq, editor-in-chief of Al-Musawa newspaper, protector of hundreds of women in safe houses, recipient of the Gruber Foundation Women’s Rights Prize in 2008 and other international awards. She fell to the bullets of darkness — and darkness will never extinguish what she lit.]Email

A Danish leftist-feminist activist and writer of Iraqi origin, Bayan Saleh is a feminist activist, writer, and long-time leftist organizer. She co-founded the Independent Women’s Organization in Erbil in 1991, was active in the Worker-Communist Party of Iraq and the Committee for the Defense of Iraqi Women’s Rights, and represented the committee at the UNHCR in Turkey. Since 2001 she has been a member and candidate of the Danish Red-Green Alliance, and since 2003 she has served on the editorial board of Al-Hiwar Al-Mutamaddin. She coordinates the Center for Women’s Equality, is a member of Amnesty International, and has served in leading positions in the Danish Women’s Council. Bayan has led multiple projects on migrant and refugee women’s rights in Denmark, Kurdistan, and the Middle East, and frequently participates in Scandinavian and international conferences on women’s rights, migration, and equality. Her educational background includes a BSc in Agriculture (University of Mosul, Iraq), diplomas in administration and IT (Denmark), and professional qualifications in psychotherapy and family counseling. She currently works as a family counselor and project manager supporting migrant women in Denmark.

When Centering and Silencing Women No Longer Work

Pam Bondi, International Women’s Day, and the Tools of Patriarchy


The March 8, 2026, celebration of International Women’s Day feels loaded. A celebration born of the early twentieth-century women’s labor movement to bolster gender equality and reproductive rights while stopping violence and abuse against women feels hollow and in need of a massive resurgence, given current US politics. With the dissolution of women’s reproductive autonomy, the rise of pronatalism, the silencing of women harmed by sexual assault, and the ultimate silencing of women through state-sanctioned murder, it is an understatement to say we are living in dark times. Simultaneously, however, we are seeing women push back against their mistreatment; women harmed in this current environment refuse to stay silent and are swiftly and publicly speaking out against the injustices put upon them.

In the timeline of public harms against women, the most recent point (as of this writing) can be broadly located on the Epstein files and, more specifically, on Attorney General Pam Bondi’s disastrous management of the files and her cruel disregard for the women named in them. On February 11, 2026, Bondi testified at a House Judiciary Committee hearing, where she repeatedly refused to answer questions about the Epstein files, a performance widely interpreted as demonstrating fealty to her boss, President Trump.

Bait-and-switch: The Epstein Files

This was neither Bondi’s first muddled foray into the Epstein files nor her first time harming the women—many of them minors at the time of their assaults—named in the files. Releasing the Epstein files was long a rallying cry of the Republican party during the Biden presidency, centered on the notion that prominent Democrats would be named and, thus, irreparably damaged. Indeed, Trump was a repeated, vocal advocate of releasing the files. In September 2025, Bondi promised to share a “mountain of evidence,” and she released several binders, labeled The Epstein Files, Phase 1, exclusively to conservative influencers. Presumably, the intent was to curry favor with friendly journalists and pundits while also setting up prominent Democrats for humiliation. This almost immediately backfired because there was nothing of consequence in these binders; all the information in them was already publicly available. Bondi’s Phase 1 was such a debacle that other members of the Trump inner circle criticized her for it, illustrating the competitiveness of Trump’s sycophants to reach top favor.

Over the next several months, the White House, and particularly Bondi, faced unrelenting scrutiny about the files. Given how many hundreds of times the word “Trump” is named in the files, the efforts to pivot the national narrative to any other story were mostly unsuccessful. Largely bowing to press pressure, in January 2026, Trump’s Department of Justice released approximately 3.5 million additional files, and once again, it was a disaster for the White House and Bondi. Although several new names surfaced and many public figures faced increased scrutiny, the release failed to redact the names of many victim-survivors even as many attackers’ names were redacted, resulting in a whole new level of harm for the victim-survivors and impunity for attackers, who remained nameless and therefore, protected.

Bondi bamboozles the House Judiciary Committee

All of this resulted in the February testimony, when Bondi repeatedly lashed out at various members of the panel. When asked if she would apologize to the victim-survivors present in the chamber, she demurred; when pressed further, she accused the panel of theatrics; and, perhaps most egregiously, she attempted to pivot to the stock market as evidence of the Trump administration’s success, demanding that the panel owed an apology to Trump for its horrid behavior. Bondi played her hand openly, stating, “I’m going to answer the question the way I want to answer the question,” signalling to everyone her partisan contempt for the committee’s members, her disregard for Epstein’s victim-survivors, and her loyalty to Trump.

Although it may seem surprising that a woman could be so baldly insensitive to survivors of sexual assault, Bondi’s audience of one—Trump—puts her insensitivity in a larger context. Bondi is very clearly following the playbook of her boss and his mentor, Roy Cohn: Attack aggressively, never admit wrongdoing, and always claim victory. While Bondi may very well have been uncomfortable in the same physical space as Epstein’s victim-survivors, she most likely believed that as long as she was loyal to her boss, she would remain shielded from any actual retribution. We cannot assume that women will have empathy or compassion for other women just because they are women; Bondi is part of the larger patriarchal culture and therefore subject to its tenets, particularly the cruelty towards anyone deemed threatening to it.

Bondi’s disastrous performance at the hearing is an opportunity to look at the Epstein saga in a new way and may be an opportunity to reimagine International Women’s Day and the treatment of women more broadly. If we peel back the curtain of patriarchy, what we see is not a terrifying monster but rather a fearful ideology running out of gas.

To maintain dominance, those working within the context of patriarchy must lash out at anything deemed threatening. Although this is frightening and often quite harmful, we can look at it in a new way: Whatever the patriarchy and its agents deem threatening must possess some degree of agency and the capacity for power, especially to create systemic change.

The women in the gallery, sitting and standing behind Bondi, were there to represent all victim-survivors of sexual assault. Their silence in this space spoke volumes: They were present, undeterred, and not backing down. Having been harmed and marginalized for years, they are now resolutely standing strong until justice is served.

One of Epstein’s bravest victim-survivors, Virginia Giuffre, took a great risk speaking out against Epstein and his companion Ghislaine Maxwell’s abuse. Giuffre publicly named (then) Prince Andrew, leading directly to the stripping of his royal title. As of this writing, Andrew Mountbatten-Windsor is once again under investigation for crimes while in public office; pointedly, his brother, King Charles, has sought to distance himself from him, and while Mountbatten-Windsor has had his royal title and its associated trappings removed, he remains eighth in the line of succession. Giuffre worked to advocate for victims of sexual assault. After her death by suicide in 2025, her family took up her fight, and they continue to push for a law that would eliminate the statute of limitations for sexual assault.

The legal response to sexual assault is further evidence of how fundamentally women are silenced. Murder, for comparison, has no statute of limitations; it is considered such a serious offense that there are no legal time limits on bringing those who commit murder to justice, for the sake of the victim, their loved ones, and society at large. By contrast, the statute of limitations for charges of sexual assault, including the sexual assault of minors, varies by state. This poses two threats to women and girls. First, statutes of limitation send the message to all that sexual assault is legally less offensive than murder. Second, because sexual assault statutes vary by state, victim-survivors are responsible not just for their healing, but also for being aware of the vagaries of a legal system that provides them with variable rights, depending on when and where they were assaulted. This makes the conflation of sexual assault and trafficking even more harmful for those involved. In her death, Giuffre will force us to consider how we conceptualize sexual assault, including, especially, how seriously we expect our legal system to take it.

These women maneuver their vulnerability as a strength, as a way to push back against and introduce new ways to fight for women’s rights. This should serve as a crystal clear warning to Bondi, Maxwell, and Epstein’s friends.

The double-edge of patriarchal power

In Bondi’s embrace of Trump and of his deny-and-deflect ethos, she should be wary that those tools of patriarchy can be turned against her. Trump has a long history of destroying relationships with individuals who no longer serve him; while Bondi is loyal to him, what makes her think he will be loyal to her? Trump’s very public attack on Marjorie Taylor Greene is evidence enough that his loyalty is fickle, at best. When (not if) Trump dumps Bondi, the tools of patriarchy will no longer work to her advantage.

Ghislaine Maxwell, who is arguably paying Epstein’s moral and ethical debts via her prison sentence, may also be harmed further by the tools of patriarchy. Maxwell is believed to possess a great deal of information, including but not limited to Epstein’s lengthy client list, that could harm many public individuals (including Trump). When Maxwell was compelled to speak with Deputy Attorney General Todd Blanche, she was moved to a minimum-security prison in exchange. When compelled a second time, Maxwell requested clemency and, when denied, invoked her Fifth Amendment rights against self-incrimination. Thus far, Maxwell’s attempts to game the legal system are not working. Her silence also speaks volumes, especially as a warning to Trump and his administration: Let me go or continue to fight this losing battle.

What if, instead, Maxwell embraced the bravery and vulnerability of her and her former partner’s victim-survivors? She might then have the courage to speak a truth that remains unspoken. Will powerful people—Democrat and Republican alike—be taken down? Perhaps. But her continued silence is evidence that, as a nation, many remain indifferent to Maxwell’s invocation of her Fifth Amendment rights as a bargaining chip for her own self-protection.

The corporate media regularly repeat the point that being named in the Epstein files and being close to Epstein are not evidence of wrongdoing (where “wrongdoing” is limited to the sexual assault and trafficking of minors). However, it stands to reason that those who turned to Epstein for financial advice, or who socialized with him because they were in the same geographic, class, and social circles, must have, to some degree, been aware of his actions. Too many sly comments, public photographs, and email chains have been shared for those implicated to be able to deny, at the very least, any superficial awareness. This means that their own personal, professional, and financial goals were more important than the lives and well-being of dozens of young women. Many of these powerful individuals—men and women—had platforms from which they could have spoken, reached out to law enforcement, pulled some strings—and they chose not to. They chose to look away or to maneuver a plausible deniability for their own selfish gains.

Reimagining International Women’s Day

This March, I strongly urge us to celebrate women in new and different ways. The history of International Women’s Day has ebbed and flowed since it was first celebrated in February 1909, including several years when it was mostly forgotten. This trajectory is not unlike how our society has viewed women over the generations: Capable of work, of autonomy, and of peace until any of those get in the way. Celebrating women can be a superficial balm to calm people’s nerves in highly stressful times, or it can be an opportunity to reflect more deeply on what our society values and how we might explore and enrich those values in new and different ways.

Let us take this auspicious day to center and amplify women. Yes, let us celebrate women’s labor, let us continue to fight for women’s reproductive autonomy, let us continue to fight violence against women—and let us also acknowledge that the very fact that we still have to fight for these basic rights is a travesty. In addition, let us fight the very ideology of patriarchy by highlighting women’s unique strengths. Let us give more oxygen to the women who speak up and speak out in the face of injustice, and who do so with vulnerability as an act of bravery. I have no doubt that women will prevail and bring down patriarchy. The question, though, is how long it will take and at what cost? If we work to do things differently, maybe we can make that time shorter and that cost less disastrous.

Editor’s note: The Judgment of Gender: How Women Are Centered and Silenced in Pop Culture, by Allison T. Butler, will be published by The Censored Press, later this month.

First published on https://www.projectcensored.org/centering-silencing-women-pam-bondi/

Allison Butler is a Senior Lecturer, Director of Undergraduate Advising, and the Director of the Media Literacy Certificate Program in the Department of Communication at the University of Massachusetts Amherst in Amherst, MA. She is the co-author of The Media and Me: A Guide to Critical Media Literacy for Young PeopleRead other articles by Allison.

 

Source: Originally published by Z. Feel free to share widely.

On International Working Women’s Day in 2025, Cilia Flores, the wife of Venezuelan President Nicolás Maduro, read a poem she wrote highlighting the historic role played by Latin American women in the fight against imperialism. 

We’re not flowers the wind can pluck,
we’re roots of rebel and loyal land,
we’re grandmothers, mothers, daughters, granddaughters;
we are woman. 
Our blood pulses with the Manuelas,
Luisas, Josefas, Juanas, Cecilias,
Apacuanas, Bartolinas, Eulalias,
Martas, Anas Marías, Barbaritas
and so many others who legacy inspires,
commits, and strengthens us
to continue walking and traveling our path.
And in our hands and chests
a light is on that nobody will ever turn off:
love, peace and liberty. 

Cilia Flores, International Working Women’s Day 2025

One year later, she languishes in a cell in New York City, having been dragged out of her room and kidnapped by U.S. forces on the January 3 attack on Venezuela. The first images after her abduction showed her face bruised. We later learned she had broken ribs, 23 stitches in her forehead, and deteriorating health inside U.S. custody.

Flores is no ordinary first lady. She first rose to prominence in 1992 as a defense lawyer for a group of Venezuelan military officers who rose up against the government of Carlos Andrés Pérez, which had massacred thousands of people in the Caracazo of 1989–nationwide riots following the imposition of neoliberal austerity measures. Key among those officers was Hugo Chávez, the founder of the Bolivarian Revolution.

In 1993, Cilia founded the Bolivarian Circle of Human Rights and aligned herself with Chávez’s revolutionary movement. In 2000, having helped Chávez win consecutive presidential elections, she was elected to the legislature. By 2006, she became the president of the National Assembly, the first woman in Venezuela’s history to occupy the post. Flores held important positions in the United Socialist Party of Venezuela and became the country’s Solicitor General in 2012, a post she left to run Nicolás Maduro’s presidential campaign after President Chávez’s passing. 

Cilia married Nicolás, her longtime partner, following the election. Feeling that the title of “first lady” could not capture her importance to the Bolivarian Revolution, her husband dubbed her the primera combatiente, or first combatant. 

After working behind the scenes as a key advisor to President Maduro, she ran for election to the National Assembly and won in 2015, 2020, and 2025.

Today, she faces charges of conspiracy to import cocaine, along with possession of machine guns and destructive devices. The charges are absurd. 

In the early 1990s, back when Venezuela was a key ally of the United States, over 50% of the world’s cocaine was trafficked through the country. By 2025, as Venezuela was considered an “unusual and extraordinary threat” to the United States, that number was down to 5%. Trump’s rhetoric of Venezuela flooding the U.S. with cocaine, and his constant conflation of cocaine with fentanyl (which is neither trafficked through nor produced in Venezuela), has no basis in reality.

Now that the Trump administration controls Venezuela’s oil trade, the rhetoric on drugs has flipped. Following a visit to Venezuela, the head of U.S. Southern Command touted a new counternarcotics cooperation agreement. Was the abduction of Nicolás and Cilia sufficient to end whatever alleged narcotics operation the Venezuelan government was accused of running? It’s more likely that such operations never existed in the first place. The allegations of drug trafficking served not only to discredit the Venezuelan government and its leaders but also paved the way for the January 3 attack. 

Cilia Flores is one of the most prominent political prisoners in the world, yet most women’s rights organizations have not said a word in her defense. She is a sitting member of Venezuela’s National Assembly and played an instrumental role in the movement that greatly expanded democratic, economic, and social rights in the country. 

Cilia stands with Palestine. In a November 2023 conference in Turkey, she said, “We are witnessing a genocide… We see the victims in Gaza. We see the death of children, women, the elderly, and civilians. We see civilian victims coming out of their destroyed homes, but unable to leave the city because they are in an open-air prison.” 

Cilia brought feminism to the Bolivarian Revolution. On International Working Women’s Day in 2023, she helped launch a social mission aimed at protecting women from the worst of the economic war. At the time, she said, “Venezuelan women have shown they are the vanguard. Women make up more than half the population, but we are also mothers of the other half, so we form a whole. And in this war that Venezuela has endured, we achieved victory and are standing firm thanks to the participation of Venezuelan women, who did not just stay home taking care of children, building their families, but also took to the streets to defend the nation. Our women are patriots… and in the next scenario, whatever it may be, we will be victorious because women will be at the forefront of any battle.” 

Little did she know that the next scenario would be a prison cell in the United States.  Out of solidarity with Cilia, with Venezuelan women in general, we must make it our cause to fight for her freedom. 

Recalling her beautiful poem above, today our blood pulses with Cilia.

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Medea Benjamin is the co-founder of CODEPINK and the co-founder of the human rights group Global Exchange. She has been an advocate for social justice for more than 40 years. She is the author of ten books, including Drone Warfare: Killing by Remote Control; Kingdom of the Unjust: Behind the US-Saudi Connection; and Inside Iran: The Real History and Politics of the Islamic Republic of Iran. Her articles appear regularly in outlets such as Znet, The Guardian, The Huffington Post, CommonDreams, Alternet and The Hill.






































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