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The White House’s favorite source of pro-Trump news is … the White House’s YouTube channel

The White House’s favorite source of pro-Trump news is … the White House’s YouTube channel

The most frequently curated content on the White House Wire, the Trump administration’s attempt to aggregate pro-Trump “real news” from across the right-wing media, doesn’t come from Truth Social, Breitbart, or even Fox News. It comes from YouTube — notably, from the White House’s own channel.

The White House Wire was launched at the end of April on the official WH.gov page, around the time that the Trump comms team began ramping up its war on the mainstream journalists and outlets who covered them critically. At that time, they’d revoked the Associated Press’ credentials after the outlet refused to refer to the Gulf of Mexico as the “Gulf of America.” Two months after its launch, Jim Nielsen, a web developer and founding engineer at the data analytics company Quadratic, ran an analysis on the links that the Trump administration has been selecting to shape their narrative. (Or, as Nielsen put it, “what kind of links they’re considering as ‘real news’”.)

Surprisingly, YouTube was the top linkout, followed by Fox News, The Post Millennial, and Fox Business. Also on the list: social media sites such as X.com (in 6th place) and Trump’s own Truth Social (8th place), and one mainstream outlet (Reuters in 7th place.)

According to an Axios story written during the launch, the Wire was intended to emulate The Drudge Report, both in layout and in purpose: a regularly-updated page of links to a curated selection of media content, along with headlines that were edited in a way that shaped a pro-Trump narrative. “It’s a place for supporters of the president’s agenda to get the real news all in one place in a shareable and readable format,” a White House official told Axios at the time, calling it a “one-stop shop for news” and a potential hub for MAGA influencer content.

Notably, for all the talk about having influencers as major players on the platform, nearly all of the YouTube link outs on the site go directly to the White House’s content. Some of them are livestreams, some of them are taped official remarks, while others are short, slickly edited videos about whatever is on the President’s agenda — perhaps a sign that no matter what influencers might say to praise them, there’s no better message than the one that’s shaped directly by the White House itself.

And even the links that go outside the MAGA media ecosystem have some Trumpian editorializing in the headlines, too. For instance, a New York Post headline on Thursday characterized the passage of the Big Beautiful Bill Act as a “bruising struggle”, reflecting the intraparty revolts and GOP defections throughout the process. On the White House Wire, the link to the Post’s story glossed over it and declared in all caps: “THE ONE, BIG BEAUTIFUL BILL HEADS TO TRUMP’S DESK”. (The White House did not immediately return a request for comment.)

Ever since his 2021 removal from Twitter and Facebook, Trump and his political apparatus have invested heavily in building out their own media infrastructure – from the websites, to the code, to the servers themselves – in order to retain complete control over their messaging without the threat of deplatforming. Truth Social, for instance, is wholly owned by Trump, meaning no other investor or shareholder can remove him for posting controversial content – one of the reasons he declined to return to Twitter after Elon Musk bought the company and rebranded it as X.

Trumpworld has also tried to reduce their reliance on right-wing media outlets over the years, which have not been as reliably loyal as they’d prefer. Fox News, for instance, became the subject of Trump’s hatred after they were the first to declare that he’d lost Arizona in the 2020 presidential election; Breitbart nearly became blacklisted after it was revealed that its chairman Steve Bannon was leaking to reporters during his stint in the White House. Cribbing the Drudge Report’s format is simply part of their pattern: Matt Drudge, the site’s primary curator and a major power player in right-wing media, became a vehement anti-Trumper and frequently uses the Drudge Report to criticise the president.

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#White #Houses #favorite #source #proTrump #news #White #Houses #YouTube #channel


Since LIGO’s Nobel-winning discovery of gravitational waves—ripples in spacetime—the U.S.-based detector has been picking up on hundreds of signals from black hole mergers. And, after a decade of studying gravitational waves, researchers believe a significant fraction of black holes may come from cosmic chain reactions.

A recent paper published in Physical Review Letters describes an analysis of 155 pairs of binary black holes, identified by LIGO and its sisters, Virgo and KAGRA, in Italy and Japan, respectively. According to the study, about 14% of merging black holes may be what’s called “second-generation black holes,” or black holes that form from previous mergers of two smaller black holes. This “hierarchical” backstory is vastly different from the textbook version of how black holes emerge from the explosive death of a star.

“Overall in the universe, black holes are merging all the time,” Cailin Plunkett, the study’s first author and a graduate student at the Massachusetts Institute of Technology, told MIT News. “Now we’re seeing a relatively consistent picture where there’s a decent percentage of black holes that are coming from this repeated pathway.”

Tracking the invisible

Gravitational waves that reach Earth’s detectors typically come from extremely intense events. Over the years, LIGO has picked up some truly perplexing signals. For example, last summer it found the most colossal black hole merger ever—and if that wasn’t wild enough, the black holes that took part in the merger lie within a cosmic “dead zone” for black holes.

This zone refers to a range of black hole masses in which, physically speaking, black holes can’t form through ordinary stellar collapse. From these discoveries, astronomers realized just how little we knew about black holes, which are challenging to investigate directly. In that sense, it was a no-brainer that the ever-growing catalog of LIGO’s gravitational signals would turn up entirely new insights about black holes.

“It is increasingly clear, both from individual events and population analyses, that massive black holes exist in [this] range,” the researchers wrote in the latest paper. “These observations have spurred further investigation into mechanisms that can populate this gap.”

A wobbly imprint

The latest research represents one such investigation. During mergers, the two black holes spiral toward each other along an orbital plane. When one or both black hole spins are misaligned, the orbital plane can wobble, or “precess,” the researchers explained to MIT News. The degree to which the disk wobbles acts as a parameter from which researchers can measure the masses and spins of the merging black holes.

One telling sign of hierarchical mergers is that they’re “lopsided,” meaning one of the pair has a much higher spin and mass than the other. For the study, the team created an analytic model to capture the kind of wobble that would have emerged from second-generation black holes. Around 14% of merging black holes followed this pattern, and the second-generation black holes identified had a very specific range of masses, at around 20 solar masses or 40 solar masses and above.

Of mysterious origins

To be fair, that might not sound like a whole lot. But it demonstrates that a sizeable portion of known black holes indeed follow this pattern. As for why, the team suspects hierarchical mergers emerge from dense stellar environments. Simply, when multiple neighboring stars die and collapse into black holes, the dense environment can make it easier for those black holes to find each other and merge. That could further lead to the formation of second-generation black holes. Theoretically, this could “repeat potentially ad infinitum, by virtue of the fact that you have a ton of stars and black holes in this really dense environment,” Plunkett said.

But an ensuing mystery concerns those black holes in the 40-and-above regime, which coincides with the aforementioned “death zones” for black hole masses. According to stellar evolution theory, black holes born of supernovas shouldn’t leave any black holes above roughly 45 solar masses, explained Plunkett.

“Yet we have seen black holes that are that massive,” she mused. “And the question is: Where did they come from?”

For now, it’s hard to say when we’ll get an answer to that question, if ever. But one thing seems to be clear: black holes are a lot weirder than we could ever imagine.

#Scientists #Black #Holes #Born #Black #HolesBlack holes,Gravitational wave,LIGO">Scientists Say Some Black Holes Are Born From Other Black Holes
                Since LIGO’s Nobel-winning discovery of gravitational waves—ripples in spacetime—the U.S.-based detector has been picking up on hundreds of signals from black hole mergers. And, after a decade of studying gravitational waves, researchers believe a significant fraction of black holes may come from cosmic chain reactions. A recent paper published in Physical Review Letters describes an analysis of 155 pairs of binary black holes, identified by LIGO and its sisters, Virgo and KAGRA, in Italy and Japan, respectively. According to the study, about 14% of merging black holes may be what’s called “second-generation black holes,” or black holes that form from previous mergers of two smaller black holes. This “hierarchical” backstory is vastly different from the textbook version of how black holes emerge from the explosive death of a star. “Overall in the universe, black holes are merging all the time,” Cailin Plunkett, the study’s first author and a graduate student at the Massachusetts Institute of Technology, told MIT News. “Now we’re seeing a relatively consistent picture where there’s a decent percentage of black holes that are coming from this repeated pathway.”

 Tracking the invisible Gravitational waves that reach Earth’s detectors typically come from extremely intense events. Over the years, LIGO has picked up some truly perplexing signals. For example, last summer it found the most colossal black hole merger ever—and if that wasn’t wild enough, the black holes that took part in the merger lie within a cosmic “dead zone” for black holes.

   This zone refers to a range of black hole masses in which, physically speaking, black holes can’t form through ordinary stellar collapse. From these discoveries, astronomers realized just how little we knew about black holes, which are challenging to investigate directly. In that sense, it was a no-brainer that the ever-growing catalog of LIGO’s gravitational signals would turn up entirely new insights about black holes. “It is increasingly clear, both from individual events and population analyses, that massive black holes exist in [this] range,” the researchers wrote in the latest paper. “These observations have spurred further investigation into mechanisms that can populate this gap.”

 A wobbly imprint The latest research represents one such investigation. During mergers, the two black holes spiral toward each other along an orbital plane. When one or both black hole spins are misaligned, the orbital plane can wobble, or “precess,” the researchers explained to MIT News. The degree to which the disk wobbles acts as a parameter from which researchers can measure the masses and spins of the merging black holes. One telling sign of hierarchical mergers is that they’re “lopsided,” meaning one of the pair has a much higher spin and mass than the other. For the study, the team created an analytic model to capture the kind of wobble that would have emerged from second-generation black holes. Around 14% of merging black holes followed this pattern, and the second-generation black holes identified had a very specific range of masses, at around 20 solar masses or 40 solar masses and above. Of mysterious origins To be fair, that might not sound like a whole lot. But it demonstrates that a sizeable portion of known black holes indeed follow this pattern. As for why, the team suspects hierarchical mergers emerge from dense stellar environments. Simply, when multiple neighboring stars die and collapse into black holes, the dense environment can make it easier for those black holes to find each other and merge. That could further lead to the formation of second-generation black holes. Theoretically, this could “repeat potentially ad infinitum, by virtue of the fact that you have a ton of stars and black holes in this really dense environment,” Plunkett said.

 But an ensuing mystery concerns those black holes in the 40-and-above regime, which coincides with the aforementioned “death zones” for black hole masses. According to stellar evolution theory, black holes born of supernovas shouldn’t leave any black holes above roughly 45 solar masses, explained Plunkett. “Yet we have seen black holes that are that massive,” she mused. “And the question is: Where did they come from?” For now, it’s hard to say when we’ll get an answer to that question, if ever. But one thing seems to be clear: black holes are a lot weirder than we could ever imagine.      #Scientists #Black #Holes #Born #Black #HolesBlack holes,Gravitational wave,LIGO

Physical Review Letters describes an analysis of 155 pairs of binary black holes, identified by LIGO and its sisters, Virgo and KAGRA, in Italy and Japan, respectively. According to the study, about 14% of merging black holes may be what’s called “second-generation black holes,” or black holes that form from previous mergers of two smaller black holes. This “hierarchical” backstory is vastly different from the textbook version of how black holes emerge from the explosive death of a star.

“Overall in the universe, black holes are merging all the time,” Cailin Plunkett, the study’s first author and a graduate student at the Massachusetts Institute of Technology, told MIT News. “Now we’re seeing a relatively consistent picture where there’s a decent percentage of black holes that are coming from this repeated pathway.”

Tracking the invisible

Gravitational waves that reach Earth’s detectors typically come from extremely intense events. Over the years, LIGO has picked up some truly perplexing signals. For example, last summer it found the most colossal black hole merger ever—and if that wasn’t wild enough, the black holes that took part in the merger lie within a cosmic “dead zone” for black holes.

This zone refers to a range of black hole masses in which, physically speaking, black holes can’t form through ordinary stellar collapse. From these discoveries, astronomers realized just how little we knew about black holes, which are challenging to investigate directly. In that sense, it was a no-brainer that the ever-growing catalog of LIGO’s gravitational signals would turn up entirely new insights about black holes.

“It is increasingly clear, both from individual events and population analyses, that massive black holes exist in [this] range,” the researchers wrote in the latest paper. “These observations have spurred further investigation into mechanisms that can populate this gap.”

A wobbly imprint

The latest research represents one such investigation. During mergers, the two black holes spiral toward each other along an orbital plane. When one or both black hole spins are misaligned, the orbital plane can wobble, or “precess,” the researchers explained to MIT News. The degree to which the disk wobbles acts as a parameter from which researchers can measure the masses and spins of the merging black holes.

One telling sign of hierarchical mergers is that they’re “lopsided,” meaning one of the pair has a much higher spin and mass than the other. For the study, the team created an analytic model to capture the kind of wobble that would have emerged from second-generation black holes. Around 14% of merging black holes followed this pattern, and the second-generation black holes identified had a very specific range of masses, at around 20 solar masses or 40 solar masses and above.

Of mysterious origins

To be fair, that might not sound like a whole lot. But it demonstrates that a sizeable portion of known black holes indeed follow this pattern. As for why, the team suspects hierarchical mergers emerge from dense stellar environments. Simply, when multiple neighboring stars die and collapse into black holes, the dense environment can make it easier for those black holes to find each other and merge. That could further lead to the formation of second-generation black holes. Theoretically, this could “repeat potentially ad infinitum, by virtue of the fact that you have a ton of stars and black holes in this really dense environment,” Plunkett said.

But an ensuing mystery concerns those black holes in the 40-and-above regime, which coincides with the aforementioned “death zones” for black hole masses. According to stellar evolution theory, black holes born of supernovas shouldn’t leave any black holes above roughly 45 solar masses, explained Plunkett.

“Yet we have seen black holes that are that massive,” she mused. “And the question is: Where did they come from?”

For now, it’s hard to say when we’ll get an answer to that question, if ever. But one thing seems to be clear: black holes are a lot weirder than we could ever imagine.

#Scientists #Black #Holes #Born #Black #HolesBlack holes,Gravitational wave,LIGO">Scientists Say Some Black Holes Are Born From Other Black HolesScientists Say Some Black Holes Are Born From Other Black Holes
                Since LIGO’s Nobel-winning discovery of gravitational waves—ripples in spacetime—the U.S.-based detector has been picking up on hundreds of signals from black hole mergers. And, after a decade of studying gravitational waves, researchers believe a significant fraction of black holes may come from cosmic chain reactions. A recent paper published in Physical Review Letters describes an analysis of 155 pairs of binary black holes, identified by LIGO and its sisters, Virgo and KAGRA, in Italy and Japan, respectively. According to the study, about 14% of merging black holes may be what’s called “second-generation black holes,” or black holes that form from previous mergers of two smaller black holes. This “hierarchical” backstory is vastly different from the textbook version of how black holes emerge from the explosive death of a star. “Overall in the universe, black holes are merging all the time,” Cailin Plunkett, the study’s first author and a graduate student at the Massachusetts Institute of Technology, told MIT News. “Now we’re seeing a relatively consistent picture where there’s a decent percentage of black holes that are coming from this repeated pathway.”

 Tracking the invisible Gravitational waves that reach Earth’s detectors typically come from extremely intense events. Over the years, LIGO has picked up some truly perplexing signals. For example, last summer it found the most colossal black hole merger ever—and if that wasn’t wild enough, the black holes that took part in the merger lie within a cosmic “dead zone” for black holes.

   This zone refers to a range of black hole masses in which, physically speaking, black holes can’t form through ordinary stellar collapse. From these discoveries, astronomers realized just how little we knew about black holes, which are challenging to investigate directly. In that sense, it was a no-brainer that the ever-growing catalog of LIGO’s gravitational signals would turn up entirely new insights about black holes. “It is increasingly clear, both from individual events and population analyses, that massive black holes exist in [this] range,” the researchers wrote in the latest paper. “These observations have spurred further investigation into mechanisms that can populate this gap.”

 A wobbly imprint The latest research represents one such investigation. During mergers, the two black holes spiral toward each other along an orbital plane. When one or both black hole spins are misaligned, the orbital plane can wobble, or “precess,” the researchers explained to MIT News. The degree to which the disk wobbles acts as a parameter from which researchers can measure the masses and spins of the merging black holes. One telling sign of hierarchical mergers is that they’re “lopsided,” meaning one of the pair has a much higher spin and mass than the other. For the study, the team created an analytic model to capture the kind of wobble that would have emerged from second-generation black holes. Around 14% of merging black holes followed this pattern, and the second-generation black holes identified had a very specific range of masses, at around 20 solar masses or 40 solar masses and above. Of mysterious origins To be fair, that might not sound like a whole lot. But it demonstrates that a sizeable portion of known black holes indeed follow this pattern. As for why, the team suspects hierarchical mergers emerge from dense stellar environments. Simply, when multiple neighboring stars die and collapse into black holes, the dense environment can make it easier for those black holes to find each other and merge. That could further lead to the formation of second-generation black holes. Theoretically, this could “repeat potentially ad infinitum, by virtue of the fact that you have a ton of stars and black holes in this really dense environment,” Plunkett said.

 But an ensuing mystery concerns those black holes in the 40-and-above regime, which coincides with the aforementioned “death zones” for black hole masses. According to stellar evolution theory, black holes born of supernovas shouldn’t leave any black holes above roughly 45 solar masses, explained Plunkett. “Yet we have seen black holes that are that massive,” she mused. “And the question is: Where did they come from?” For now, it’s hard to say when we’ll get an answer to that question, if ever. But one thing seems to be clear: black holes are a lot weirder than we could ever imagine.      #Scientists #Black #Holes #Born #Black #HolesBlack holes,Gravitational wave,LIGO

Since LIGO’s Nobel-winning discovery of gravitational waves—ripples in spacetime—the U.S.-based detector has been picking up on hundreds of signals from black hole mergers. And, after a decade of studying gravitational waves, researchers believe a significant fraction of black holes may come from cosmic chain reactions.

A recent paper published in Physical Review Letters describes an analysis of 155 pairs of binary black holes, identified by LIGO and its sisters, Virgo and KAGRA, in Italy and Japan, respectively. According to the study, about 14% of merging black holes may be what’s called “second-generation black holes,” or black holes that form from previous mergers of two smaller black holes. This “hierarchical” backstory is vastly different from the textbook version of how black holes emerge from the explosive death of a star.

“Overall in the universe, black holes are merging all the time,” Cailin Plunkett, the study’s first author and a graduate student at the Massachusetts Institute of Technology, told MIT News. “Now we’re seeing a relatively consistent picture where there’s a decent percentage of black holes that are coming from this repeated pathway.”

Tracking the invisible

Gravitational waves that reach Earth’s detectors typically come from extremely intense events. Over the years, LIGO has picked up some truly perplexing signals. For example, last summer it found the most colossal black hole merger ever—and if that wasn’t wild enough, the black holes that took part in the merger lie within a cosmic “dead zone” for black holes.

This zone refers to a range of black hole masses in which, physically speaking, black holes can’t form through ordinary stellar collapse. From these discoveries, astronomers realized just how little we knew about black holes, which are challenging to investigate directly. In that sense, it was a no-brainer that the ever-growing catalog of LIGO’s gravitational signals would turn up entirely new insights about black holes.

“It is increasingly clear, both from individual events and population analyses, that massive black holes exist in [this] range,” the researchers wrote in the latest paper. “These observations have spurred further investigation into mechanisms that can populate this gap.”

A wobbly imprint

The latest research represents one such investigation. During mergers, the two black holes spiral toward each other along an orbital plane. When one or both black hole spins are misaligned, the orbital plane can wobble, or “precess,” the researchers explained to MIT News. The degree to which the disk wobbles acts as a parameter from which researchers can measure the masses and spins of the merging black holes.

One telling sign of hierarchical mergers is that they’re “lopsided,” meaning one of the pair has a much higher spin and mass than the other. For the study, the team created an analytic model to capture the kind of wobble that would have emerged from second-generation black holes. Around 14% of merging black holes followed this pattern, and the second-generation black holes identified had a very specific range of masses, at around 20 solar masses or 40 solar masses and above.

Of mysterious origins

To be fair, that might not sound like a whole lot. But it demonstrates that a sizeable portion of known black holes indeed follow this pattern. As for why, the team suspects hierarchical mergers emerge from dense stellar environments. Simply, when multiple neighboring stars die and collapse into black holes, the dense environment can make it easier for those black holes to find each other and merge. That could further lead to the formation of second-generation black holes. Theoretically, this could “repeat potentially ad infinitum, by virtue of the fact that you have a ton of stars and black holes in this really dense environment,” Plunkett said.

But an ensuing mystery concerns those black holes in the 40-and-above regime, which coincides with the aforementioned “death zones” for black hole masses. According to stellar evolution theory, black holes born of supernovas shouldn’t leave any black holes above roughly 45 solar masses, explained Plunkett.

“Yet we have seen black holes that are that massive,” she mused. “And the question is: Where did they come from?”

For now, it’s hard to say when we’ll get an answer to that question, if ever. But one thing seems to be clear: black holes are a lot weirder than we could ever imagine.

#Scientists #Black #Holes #Born #Black #HolesBlack holes,Gravitational wave,LIGO

Ready for the 2026 World Cup final? You might think you are, but your body is going to have to be prepared to put in some work—especially if your favorite team makes it.

Research shows that watching high-pressure matches can raise your heart rate, increase your stress levels, and put extra strain on your cardiovascular system.

According to a recent study from researchers at Bielefeld University in Germany, fans’ physiological stress increases by about 41 percent during a soccer final compared to a normal day. Heart rate also rose significantly, jumping from 70.9 beats per minute to 78.7 beats per minute—a difference even when compared to other weekends.

Researchers at Bielefeld tracked 229 fans of the German club Arminia Bielefeld for three months. Participants wore smartwatches that continuously recorded heart rate and an estimated stress index based on heart rate variability, allowing researchers to compare the day of the 2025 German Cup final with the days leading up to the match.

The physiological reaction to the soccer final began long before the match began. The researchers saw fans’ stress levels begin to rise in the morning and peak just before kickoff. Even after the final whistle, viewers showed signs of elevated stress.

Where you watch the game also makes a difference. The study found that fans who watched at the stadium had an average heart rate of 94.2 beats per minute compared to 79.4 among those who watched the match on television. After their team’s first goal, those in the stands saw their heart rate climb to an average of up to 108 beats per minute—a much more intense response than that observed in other contexts.

Alcohol consumption appeared to amplify that effect. Participants who reported drinking during the game had a heart rate approximately 5 percent higher than the rest of the fans during the match and nearly 12 percent higher after their team’s first goal. Although the researchers did not assess medical risks, they note that alcohol can increase cardiovascular strain when people are in an emotional state.

During the first few minutes of the match, when the outcome was still uncertain, heart rates reached their highest levels. Once the game seemed to be decided, fans’ heart rates dropped.

However, two goals scored in the final minutes caused them to spike again, even though the chances of a comeback were practically nil. (You can only imagine how fast Argentina fans’ hearts were thumping during this week’s furious comeback against Egypt.) For the authors, this reflects that the body responds not only to the objective chances of winning but also to emotions such as hope, pride, or attachment to the team.

The findings align with the results of previous studies on the physiological impacts of soccer. That incluides a study published in the New England Journal of Medicine after the 2006 World Cup in Germany, found that the risk of suffering an acute cardiovascular event nearly triples during German national team matches among people with preexisting heart conditions.

Subsequent research shows that matches can lead to an increase in stress hormones such as cortisol and found that fans who identify more strongly with their team exhibit more intense biological responses during decisive matches.

This article originally appeared on WIRED en Español and has been translated from Spanish.

#Watching #Soccer #Final #Body #Scienceworld cup 2026,sports,health,soccer,stress,fandom">What Watching a Soccer Final Does to Your Body, According to ScienceReady for the 2026 World Cup final? You might think you are, but your body is going to have to be prepared to put in some work—especially if your favorite team makes it.Research shows that watching high-pressure matches can raise your heart rate, increase your stress levels, and put extra strain on your cardiovascular system.According to a recent study from researchers at Bielefeld University in Germany, fans’ physiological stress increases by about 41 percent during a soccer final compared to a normal day. Heart rate also rose significantly, jumping from 70.9 beats per minute to 78.7 beats per minute—a difference even when compared to other weekends.Researchers at Bielefeld tracked 229 fans of the German club Arminia Bielefeld for three months. Participants wore smartwatches that continuously recorded heart rate and an estimated stress index based on heart rate variability, allowing researchers to compare the day of the 2025 German Cup final with the days leading up to the match.The physiological reaction to the soccer final began long before the match began. The researchers saw fans’ stress levels begin to rise in the morning and peak just before kickoff. Even after the final whistle, viewers showed signs of elevated stress.Where you watch the game also makes a difference. The study found that fans who watched at the stadium had an average heart rate of 94.2 beats per minute compared to 79.4 among those who watched the match on television. After their team’s first goal, those in the stands saw their heart rate climb to an average of up to 108 beats per minute—a much more intense response than that observed in other contexts.Alcohol consumption appeared to amplify that effect. Participants who reported drinking during the game had a heart rate approximately 5 percent higher than the rest of the fans during the match and nearly 12 percent higher after their team’s first goal. Although the researchers did not assess medical risks, they note that alcohol can increase cardiovascular strain when people are in an emotional state.During the first few minutes of the match, when the outcome was still uncertain, heart rates reached their highest levels. Once the game seemed to be decided, fans’ heart rates dropped.However, two goals scored in the final minutes caused them to spike again, even though the chances of a comeback were practically nil. (You can only imagine how fast Argentina fans’ hearts were thumping during this week’s furious comeback against Egypt.) For the authors, this reflects that the body responds not only to the objective chances of winning but also to emotions such as hope, pride, or attachment to the team.The findings align with the results of previous studies on the physiological impacts of soccer. That incluides a study published in the New England Journal of Medicine after the 2006 World Cup in Germany, found that the risk of suffering an acute cardiovascular event nearly triples during German national team matches among people with preexisting heart conditions.Subsequent research shows that matches can lead to an increase in stress hormones such as cortisol and found that fans who identify more strongly with their team exhibit more intense biological responses during decisive matches.This article originally appeared on WIRED en Español and has been translated from Spanish.#Watching #Soccer #Final #Body #Scienceworld cup 2026,sports,health,soccer,stress,fandom

2026 World Cup final? You might think you are, but your body is going to have to be prepared to put in some work—especially if your favorite team makes it.

Research shows that watching high-pressure matches can raise your heart rate, increase your stress levels, and put extra strain on your cardiovascular system.

According to a recent study from researchers at Bielefeld University in Germany, fans’ physiological stress increases by about 41 percent during a soccer final compared to a normal day. Heart rate also rose significantly, jumping from 70.9 beats per minute to 78.7 beats per minute—a difference even when compared to other weekends.

Researchers at Bielefeld tracked 229 fans of the German club Arminia Bielefeld for three months. Participants wore smartwatches that continuously recorded heart rate and an estimated stress index based on heart rate variability, allowing researchers to compare the day of the 2025 German Cup final with the days leading up to the match.

The physiological reaction to the soccer final began long before the match began. The researchers saw fans’ stress levels begin to rise in the morning and peak just before kickoff. Even after the final whistle, viewers showed signs of elevated stress.

Where you watch the game also makes a difference. The study found that fans who watched at the stadium had an average heart rate of 94.2 beats per minute compared to 79.4 among those who watched the match on television. After their team’s first goal, those in the stands saw their heart rate climb to an average of up to 108 beats per minute—a much more intense response than that observed in other contexts.

Alcohol consumption appeared to amplify that effect. Participants who reported drinking during the game had a heart rate approximately 5 percent higher than the rest of the fans during the match and nearly 12 percent higher after their team’s first goal. Although the researchers did not assess medical risks, they note that alcohol can increase cardiovascular strain when people are in an emotional state.

During the first few minutes of the match, when the outcome was still uncertain, heart rates reached their highest levels. Once the game seemed to be decided, fans’ heart rates dropped.

However, two goals scored in the final minutes caused them to spike again, even though the chances of a comeback were practically nil. (You can only imagine how fast Argentina fans’ hearts were thumping during this week’s furious comeback against Egypt.) For the authors, this reflects that the body responds not only to the objective chances of winning but also to emotions such as hope, pride, or attachment to the team.

The findings align with the results of previous studies on the physiological impacts of soccer. That incluides a study published in the New England Journal of Medicine after the 2006 World Cup in Germany, found that the risk of suffering an acute cardiovascular event nearly triples during German national team matches among people with preexisting heart conditions.

Subsequent research shows that matches can lead to an increase in stress hormones such as cortisol and found that fans who identify more strongly with their team exhibit more intense biological responses during decisive matches.

This article originally appeared on WIRED en Español and has been translated from Spanish.

#Watching #Soccer #Final #Body #Scienceworld cup 2026,sports,health,soccer,stress,fandom">What Watching a Soccer Final Does to Your Body, According to Science

Ready for the 2026 World Cup final? You might think you are, but your body is going to have to be prepared to put in some work—especially if your favorite team makes it.

Research shows that watching high-pressure matches can raise your heart rate, increase your stress levels, and put extra strain on your cardiovascular system.

According to a recent study from researchers at Bielefeld University in Germany, fans’ physiological stress increases by about 41 percent during a soccer final compared to a normal day. Heart rate also rose significantly, jumping from 70.9 beats per minute to 78.7 beats per minute—a difference even when compared to other weekends.

Researchers at Bielefeld tracked 229 fans of the German club Arminia Bielefeld for three months. Participants wore smartwatches that continuously recorded heart rate and an estimated stress index based on heart rate variability, allowing researchers to compare the day of the 2025 German Cup final with the days leading up to the match.

The physiological reaction to the soccer final began long before the match began. The researchers saw fans’ stress levels begin to rise in the morning and peak just before kickoff. Even after the final whistle, viewers showed signs of elevated stress.

Where you watch the game also makes a difference. The study found that fans who watched at the stadium had an average heart rate of 94.2 beats per minute compared to 79.4 among those who watched the match on television. After their team’s first goal, those in the stands saw their heart rate climb to an average of up to 108 beats per minute—a much more intense response than that observed in other contexts.

Alcohol consumption appeared to amplify that effect. Participants who reported drinking during the game had a heart rate approximately 5 percent higher than the rest of the fans during the match and nearly 12 percent higher after their team’s first goal. Although the researchers did not assess medical risks, they note that alcohol can increase cardiovascular strain when people are in an emotional state.

During the first few minutes of the match, when the outcome was still uncertain, heart rates reached their highest levels. Once the game seemed to be decided, fans’ heart rates dropped.

However, two goals scored in the final minutes caused them to spike again, even though the chances of a comeback were practically nil. (You can only imagine how fast Argentina fans’ hearts were thumping during this week’s furious comeback against Egypt.) For the authors, this reflects that the body responds not only to the objective chances of winning but also to emotions such as hope, pride, or attachment to the team.

The findings align with the results of previous studies on the physiological impacts of soccer. That incluides a study published in the New England Journal of Medicine after the 2006 World Cup in Germany, found that the risk of suffering an acute cardiovascular event nearly triples during German national team matches among people with preexisting heart conditions.

Subsequent research shows that matches can lead to an increase in stress hormones such as cortisol and found that fans who identify more strongly with their team exhibit more intense biological responses during decisive matches.

This article originally appeared on WIRED en Español and has been translated from Spanish.

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