AI chip startup Groq is in talks to raise a fresh $600 million at a near $6 billion valuation, sources tell Bloomberg, although the deal isnāt yet final and terms could change.Ā
Groq raised $640 million at a $2.8 billion valuation in August 2024, making this double the valuation in about a year. Groq previously raised about $1 billion.
The new round is led by Austin-based firm Disruptive, Bloomberg reports. The November round was led by BlackRock, with participation from Neuberger Berman, Type One Ventures, Cisco, KDDI, and Samsung Catalyst Fund.
Groq was founded by Jonathan Ross, who previously worked at Google developing its Tensor Processing Unit chip. The startup emerged from stealth in 2016.
This new raise comes after Groq announced in May an exclusive partnership with Bell Canada to power the telcoās large AI infrastructure project. In April, Groq partnered with Meta to offer AI infrastructure to speed Llama 4 inference. Neither Disruptive nor Groq immediately returned our request for comment.
Correction: This story originally incorrectly reported the date of the last raise.
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![Scientists Say Some Black Holes Are Born From Other Black Holes
Since LIGOās Nobel-winning discovery of gravitational wavesāripples in spacetimeāthe 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 whatās called āsecond-generation black holes,ā or black holes that form from previous mergers of two smaller black holes. This āhierarchicalā backstory is vastly different from the textbook version of how black holes emerge from the explosive death of a star. āOverall in the universe, black holes are merging all the time,ā Cailin Plunkett, the studyās first author and a graduate student at the Massachusetts Institute of Technology, told MIT News. āNow weāre seeing a relatively consistent picture where thereās a decent percentage of black holes that are coming from this repeated pathway.ā
Tracking the invisible Gravitational waves that reach Earthās 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 everāand if that wasnāt wild enough, the black holes that took part in the merger lie within a cosmic ādead zoneā for black holes.
This zone refers to a range of black hole masses in which, physically speaking, black holes canāt 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 LIGOās gravitational signals would turn up entirely new insights about black holes. āIt is increasingly clear, both from individual events and population analyses, that massive black holes exist in [this] range,ā the researchers wrote in the latest paper. āThese observations have spurred further investigation into mechanisms that can populate this gap.ā
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 āprecess,ā 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 theyāre ālopsided,ā 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 ārepeat potentially ad infinitum, by virtue of the fact that you have a ton of stars and black holes in this really dense environment,ā Plunkett said.
But an ensuing mystery concerns those black holes in the 40-and-above regime, which coincides with the aforementioned ādeath zonesā for black hole masses. According to stellar evolution theory, black holes born of supernovas shouldnāt leave any black holes above roughly 45 solar masses, explained Plunkett. āYet we have seen black holes that are that massive,ā she mused. āAnd the question is: Where did they come from?ā For now, itās hard to say when weāll 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 LIGOās Nobel-winning discovery of gravitational wavesāripples in spacetimeāthe 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 whatās called āsecond-generation black holes,ā or black holes that form from previous mergers of two smaller black holes. This āhierarchicalā backstory is vastly different from the textbook version of how black holes emerge from the explosive death of a star. āOverall in the universe, black holes are merging all the time,ā Cailin Plunkett, the studyās first author and a graduate student at the Massachusetts Institute of Technology, told MIT News. āNow weāre seeing a relatively consistent picture where thereās a decent percentage of black holes that are coming from this repeated pathway.ā
Tracking the invisible Gravitational waves that reach Earthās 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 everāand if that wasnāt wild enough, the black holes that took part in the merger lie within a cosmic ādead zoneā for black holes.
This zone refers to a range of black hole masses in which, physically speaking, black holes canāt 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 LIGOās gravitational signals would turn up entirely new insights about black holes. āIt is increasingly clear, both from individual events and population analyses, that massive black holes exist in [this] range,ā the researchers wrote in the latest paper. āThese observations have spurred further investigation into mechanisms that can populate this gap.ā
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 āprecess,ā 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 theyāre ālopsided,ā 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 ārepeat potentially ad infinitum, by virtue of the fact that you have a ton of stars and black holes in this really dense environment,ā Plunkett said.
But an ensuing mystery concerns those black holes in the 40-and-above regime, which coincides with the aforementioned ādeath zonesā for black hole masses. According to stellar evolution theory, black holes born of supernovas shouldnāt leave any black holes above roughly 45 solar masses, explained Plunkett. āYet we have seen black holes that are that massive,ā she mused. āAnd the question is: Where did they come from?ā For now, itās hard to say when weāll 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](https://gizmodo.com/app/uploads/2026/07/black-hole-hierarchial-mergers-1280x853.jpg)
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