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A group of astrophysicists and quantum physicists have achieved a breakthrough in understanding the enigmatic phenomena known as neutron stars “glitches”, reports Space.com. These strange things, which suddenly speed up the rotation of giant dead stars, may be caused by tiny spins of matter inside the bodies of these powerful celestial bodies.
Special research, conducted by scientists from the field of astrophysics and quantum physicsIt provides a new perspective on the behavior of neutron stars. Interestingly, the research used a unique level of the aboveWorld to understand the power of these distant star bodies.
Neutron stars, born from the collapse of large stars, boast extraordinary mass, consisting almost exclusively of neutrons. The team’s research aimed to clarify the events that occur in neutron stars, and provide information into their composition and activity.
Lead author Elena Poli, a researcher at University of Innsbruckemphasized the importance of the research, saying, “Our research establishes a strong link between quantum mechanics and astrophysics and provide new insight into the inner nature of neutron stars.”
Bringing the study of neutron stars “down to earth,” the team used numerical simulations and a representative-an ultracold dipolar atom system to represent neutron stars. The extreme conditions and great distances associated with neutron stars make it impossible to accurately simulate them, but the team successfully simulated neutron star behavior in four use of these ultracold dipolar atoms.
The research suggests that collisions with neutron stars could indicate a more fluid subsurface—something with no viscosity like a water. The strange properties of superfluids, especially a “supersolid” phase, are playing an important role in the emergency.
By injecting the most energetic particles into the ultracold dipolar atoms of Erbium (Er) and Dysprosium (Dy), the team simulated several glitching neutron stars. The results suggest that the larger vortices that carry the gravitational force on the star contribute to the luminosity. observed in neutron stars.
The researchers hope to study in depth the operation of the machine, studying its complexities and its dependence on the quality of the best materials. The study not only expands our understanding of neutron stars but also paves the way for new methods in quantum simulation, which can offer information on other stellar remnants in research centers around the world.
The findings were published in the November issue of the journal Physical Review Letters.
Special research, conducted by scientists from the field of astrophysics and quantum physicsIt provides a new perspective on the behavior of neutron stars. Interestingly, the research used a unique level of the aboveWorld to understand the power of these distant star bodies.
Neutron stars, born from the collapse of large stars, boast extraordinary mass, consisting almost exclusively of neutrons. The team’s research aimed to clarify the events that occur in neutron stars, and provide information into their composition and activity.
Lead author Elena Poli, a researcher at University of Innsbruckemphasized the importance of the research, saying, “Our research establishes a strong link between quantum mechanics and astrophysics and provide new insight into the inner nature of neutron stars.”
Bringing the study of neutron stars “down to earth,” the team used numerical simulations and a representative-an ultracold dipolar atom system to represent neutron stars. The extreme conditions and great distances associated with neutron stars make it impossible to accurately simulate them, but the team successfully simulated neutron star behavior in four use of these ultracold dipolar atoms.
The research suggests that collisions with neutron stars could indicate a more fluid subsurface—something with no viscosity like a water. The strange properties of superfluids, especially a “supersolid” phase, are playing an important role in the emergency.
By injecting the most energetic particles into the ultracold dipolar atoms of Erbium (Er) and Dysprosium (Dy), the team simulated several glitching neutron stars. The results suggest that the larger vortices that carry the gravitational force on the star contribute to the luminosity. observed in neutron stars.
The researchers hope to study in depth the operation of the machine, studying its complexities and its dependence on the quality of the best materials. The study not only expands our understanding of neutron stars but also paves the way for new methods in quantum simulation, which can offer information on other stellar remnants in research centers around the world.
The findings were published in the November issue of the journal Physical Review Letters.