Scientists Pinpoint First Direct Evidence of Dark Matter, a Mysterious 27% of the Universe's Mass
In a groundbreaking discovery, researchers have claimed to spot the first direct evidence of dark matter, a substance that has long been shrouded in mystery. According to Prof Tomonori Totani, an astrophysicist at the University of Tokyo, gamma rays emanating from the center of our galaxy appear to exhibit the signature of this elusive material.
For decades, scientists have been searching for dark matter, which is thought to make up a staggering 27% of the cosmos. Its very existence was first proposed in the 1930s by Swiss astronomer Fritz Zwicky, who observed that distant galaxies were spinning faster than their mass allowed. Since then, countless theories and hypotheses have emerged, but a definitive proof has remained elusive.
One theory suggests that dark matter is composed of particles known as weakly interacting massive particles (WIMPs), which are heavier than protons but interact with normal matter only minimally. When WIMPs collide, they can annihilate each other, releasing gamma rays in the process. Using data from NASA's Fermi Gamma-ray Space Telescope, Totani spotted a pattern of gamma rays that appears to match the predicted shape of dark matter halos.
However, skeptics remain cautious, citing the need for further verification and ruling out alternative explanations. Prof Justin Read of the University of Surrey notes that the absence of significant signals from other regions of space, such as dwarf galaxies, argues against Totani's claims. Similarly, Prof Kinwah Wu of UCL urges caution, stating that extraordinary evidence is still needed to confirm this groundbreaking discovery.
While more work is required to validate these findings, the implications are profound. If true, this breakthrough would represent a major turning point in our understanding of the universe and the mysterious substance that permeates it.
In a groundbreaking discovery, researchers have claimed to spot the first direct evidence of dark matter, a substance that has long been shrouded in mystery. According to Prof Tomonori Totani, an astrophysicist at the University of Tokyo, gamma rays emanating from the center of our galaxy appear to exhibit the signature of this elusive material.
For decades, scientists have been searching for dark matter, which is thought to make up a staggering 27% of the cosmos. Its very existence was first proposed in the 1930s by Swiss astronomer Fritz Zwicky, who observed that distant galaxies were spinning faster than their mass allowed. Since then, countless theories and hypotheses have emerged, but a definitive proof has remained elusive.
One theory suggests that dark matter is composed of particles known as weakly interacting massive particles (WIMPs), which are heavier than protons but interact with normal matter only minimally. When WIMPs collide, they can annihilate each other, releasing gamma rays in the process. Using data from NASA's Fermi Gamma-ray Space Telescope, Totani spotted a pattern of gamma rays that appears to match the predicted shape of dark matter halos.
However, skeptics remain cautious, citing the need for further verification and ruling out alternative explanations. Prof Justin Read of the University of Surrey notes that the absence of significant signals from other regions of space, such as dwarf galaxies, argues against Totani's claims. Similarly, Prof Kinwah Wu of UCL urges caution, stating that extraordinary evidence is still needed to confirm this groundbreaking discovery.
While more work is required to validate these findings, the implications are profound. If true, this breakthrough would represent a major turning point in our understanding of the universe and the mysterious substance that permeates it.