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Amid Detainees' Release, Putin Flaunts Power and Flouts Western Influence

Aug 22, 2024

3 min

Lynne Hartnett, PhD

On August 1, the United States, Russia, Germany and three other European nations engaged in an historic 24-person East-West prisoner exchange.


The largest such swap since the end of the Cold War, the multi-country deal secured the release of three prominent American detainees: Wall Street Journal correspondent Evan Gershkovich, corporate security executive Paul Whelan and Radio Free Europe/Radio Liberty editor Alsu Kurmasheva. It also freed a dozen Russian opposition leaders, incarcerated in their native country for challenging Vladimir Putin and his authoritarian regime.


Lynne Hartnett, PhD, is the chair of Villanova University’s Department of History and an expert on modern Russia, protest movements and dissidents in exile. Recently, she shared some insights on the Kremlin's decision to release the American and Russian prisoners—as well as the egotism, oppressive tendencies and political posturing that drove their detention.


Q: The arrests and sentencings of Gershkovich, Whelan and Kurmasheva have been described as "outrageous," "a mockery of justice" and reflective of "a total disregard for basic freedoms." What prompted Putin and the Russian government to detain these individuals?


Dr. Hartnett: For Putin, seizing Gershkovich, Whelan and Kurmasheva was a power play. They were pawns for him to use when he deemed it convenient. If they could be used in a prisoner swap, they would be. But if that time never arrived, their incarceration, suffering and even potential deaths were inconsequential to him.


Their arrests were also a signal that, in Russia, Putin's authority is uncontested. These were American citizens, and around the world, a U.S. passport opens doors: It holds power; it provides access; and it affords its holder protection. But the arrests of Gershkovich, Whelan and Kurmasheva were Putin’s attempt to demonstrate the limits of American influence. They were meant as a signal that, in Russia, a U.S. passport becomes meaningless if it serves Putin to make it so.


Q: In recent years, the Russian government has seemingly worked to rehabilitate the reputations of figures like Josef Stalin, who infamously used the Soviet Gulag to stifle opposition and criticism. Is Putin's use of detentions as a political cudgel similar?


DH: The show trials of the Stalinist era are frequently referenced. However, it should be stressed that those were largely intended for domestic consumption. They were used to justify the Communist elites' repression of fellow citizens by broadcasting "evidence" that enemies lurked within.


The trials of Americans like Gershkovich and Brittney Griner [a professional basketball player detained on smuggling charges] were designed to show the world, not just Russians, that Putin's regime would not be cowed—even if the person being tried had fame and a powerful enterprise, like the Wall Street Journal or the WNBA, supporting them.


Q: The New York Times recently ran a piece on the Russian dissidents released, claiming "hopes are high [they] will breathe new life into a fragmented opposition force." What do you anticipate these political players' activism will look like in the coming years, especially in exile?


DH: As in the Imperial and Soviet periods, Russian censorship prevents any news or opinions that are not the government's from coming to light. As Putin has dismantled political opposition in Russia and tightened his grip on any vestiges of civil society in the country, there is little hope that a powerful opposition movement can gain momentum without outside support.


This is where the Russian dissidents living abroad come in. They will ensure that a vision for another type of Russia is articulated.


At the end of the 19th and the beginning of the 20th centuries, political exiles smuggled illegal newspapers and journals into the Russian empire to instill hope in their compatriots, to give them some indication that a nation beyond the autocracy was achievable. This, in my opinion, is the role that Russian dissidents living in exile must have today.


They must provide the vision. They must provide the hope.


While they cannot change the system on their own—they need a movement en masse—the dissidents abroad are needed to demonstrate that a nation without Putin and his repressive regime is possible. This is certainly not an easy venture, and it will require extraordinary sacrifices to be made a reality. However, it may be the Russian people's only hope.


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Lynne Hartnett, PhD

Lynne Hartnett, PhD

Professor and Chair of History | College of Liberal Arts and Sciences

Lynne Hartnett, PhD, is an expert on Russian history, protest movements and refugees and political exile.

Protest MovementsPolitical ExileHistory of RevolutionRussiaRussian History

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Is there any sort of precedent for this event in the museum’s history? Dr. Cooke: Nothing on this scale has ever happened to the Louvre since its founding as a museum during the Revolution. The closest equivalent is the 1911 theft of the Mona Lisa by a former employee who claimed it should be returned to Italy. However, that was one painting, the heist was not committed by organized crime, and the Mona Lisa did not have the renown it enjoys today. The impact of the theft was thus lower, although it did cause major outrage and a sweeping law-enforcement response at the time. Ironically, that theft is often credited with making da Vinci’s painting the global icon it continues to be. Q: What has the reaction to this event been among the French people? DC: It’s harder to get a sense of reactions across French society, because so much of the aftermath has focused on the intellectual milieux’s opinions. And in those realms, it has immediately become a political football. Individuals positioning themselves as anti-elite or anti-status quo, such as Jordan Bardella of the National Rally party, have called the theft a “humiliation,” immediately tying it to French national prestige. Former President François Hollande has conversely and vainly called for the event to be de-polemicized, citing national solidarity. This is happening because the Louvre is one of the most visible manifestations of French soft power—the most-visited museum anywhere on Earth. As such, anything attacking its integrity becomes an attack on the nation, and how individual French citizens feel about the theft is closely tied to their broader view of the nation. Q: Several of the items stolen from the Louvre once belonged to Empress Eugénie. Could you share a bit of information on her story? DC: Eugénie de Montijo was a Spanish aristocrat who married the Emperor of the French, who ruled as Napoleon III between 1852 and 1870. 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4 min

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Spectral analysis indicated GX13+1 was at that very moment undergoing a luminous super-Eddington phase, meaning the neutron star was shining so brightly that the radiation pressure from its surface overcame gravity, leading to a powerful ejection of any infalling material (hence the slow cosmic wind). Further comparison to previous data implied that such phases may be part of a cycle, and could “change the way we think about the behavior of these systems,” according to Joey Neilsen, PhD, associate professor of Physics at Villanova University. Dr. Neilsen played a prominent role as a co-investigator and one of the corresponding authors of the project, along with colleagues at the University of Durham (United Kingdom), Osaka University (Japan), and the University of Teacher Education Fukuoka (Japan). Overall, the collaboration featured researchers from dozens of institutions across the world. GX13+1 is a binary system consisting of a neutron star orbiting a K5 III companion star—a cooler giant star nearing the end of its life. Neutron stars are small, incredibly dense cores of supergiant stars that have undergone supernovae explosions. They are so dense, Dr. Neilsen says, that one teaspoon of its material would weigh about the same as Mount Everest. Because of this, they yield an incredibly strong gravitational field. When these highly compact neutron stars orbit companion stars, they can pull in, or accrete, material from that companion. That inflowing material forms a visible rotating disk of gas and dust called an accretion disk, which is extremely hot and shines brightly in X-rays. It’s so bright that sometimes it can actually drive matter away from the neutron star. “Imagine putting a giant lightbulb in a lake,” Dr. Neilsen said. “If it’s bright enough, it will start to boil that lake and then you would get steam, which flows away like a wind. It’s the same concept; the light can heat up and exert pressure on the accretion disk, launching a wind.” The original purpose of the study was to use XRISM to observe an accretion disk wind, with GX13+1 targeted specifically because its disk is persistently bright, it reliably produces winds, and it has been well studied using Chandra— NASA’s flagship X-ray observatory—and other telescopes for comparison. XRISM can measure the X-ray energies from these systems a factor of 10 more precisely than Chandra, allowing researchers to both demonstrate the capabilities of the new instrument and study the motion of outflowing gas around the neutron star. This can provide new insights into accretion processes. “It's like comparing a blurry image to a much sharper one,” Dr. Neilsen said. “The atomic physics hasn't changed, but you can see it much more clearly.” The researchers uncovered an exciting surprise when the higher-resolution spectrum showed much deeper absorption lines than expected. They determined that the wind was nearly opaque to X-rays and slow at “only” 1.4 million miles per hour—surprisingly leisurely for such a bright source. Based on the data, the team was able to infer that GX13+1 must have been even brighter than usual and undergoing a super-Eddington phase. So much material was ejected that it made GX13+1 appear fainter to the instrument. “There's a theoretical maximum luminosity that you can get out of an accreting object, called the Eddington limit. At that point, the radiation pressure from the light of the infalling gas is so large that it can actually hold the matter away,” Dr. Neilsen said, equating it to standing at the bottom of a waterfall and shining light so brightly that the waterfall stops. “What we saw was that GX13+1 had to have been near, or maybe even above, the Eddington limit.” The team compared their XRISM data from this super-Eddington phase to a set of previous observations without the resolution to measure the absorption lines directly. They found several older observations with faint, unusually shaped X-ray spectra similar to the one seen by XRISM. “XRISM explained these periods with funny-shaped spectra as not just anomalies, but the result of this phenomenally strong accretion disk wind in all its glory,” Dr. Neilsen said. “If we hadn’t caught this exact period with XRISM, we would never have understood those earlier data.” The connection suggests that this system spends roughly 10 percent of its time in a super-Eddington phase, which means super-Eddington accretion may be more common than previously understood—perhaps even following cycles—in neutron star or black hole binary systems. “Temporary super-Eddington phases might actually be a thing that accreting systems do, not just something unique to this system,” Dr. Neilsen said. “And if neutron stars and black holes are doing it, what about supermassive black holes? Perhaps this could pave the way for a deeper understanding of all these systems.”

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