research is impeccable, with complicated concepts presented in an easily understood manner. I highly recommendNeutron Starsto anyone who wants to learn not only about the history of neutron star research, but also the current race to understand fast radio bursts, magnetars, and colliding neutron ...
Passamonti A and Andersson N 2012 Towards real neutron star seismology: accounting for elasticity and superfluidity Mon. Not. R. Astron. Soc. 419 638A. Passamonti and N. Andersson, Towards real neutron star seismology: accounting for elasticity and superfluidity, MNRAS 419 (2012) 638-655, [...
If new movies aren't appealing to you, Austin has the usual wealth of special screenings, indoors and out. I'm tempted to see Ghostbusters at Blue Starlite tonight or Saturday; they're offering s'mores kits with "real Stay-Puft marshmallows" to enjoy with the film. Alamo Ritz brings ...
With all that starlight removed, the researchers were left with unprecedented, extremely detailed pictures of the shape and evolution of the afterglow over time.The picture that emerged doesn't look like anything we'd see if we looked up into the night sky with just our eyes, Fong told ...
“Perhaps the biggest surprise was how well-behaved the visual signal acted compared to our theoretical expectations,” Metzger noted. “No one had ever seen a neutron star merger up close before. Putting together the complete picture of such an event involves a wide range of physics – general...
Type One says in its website it has planned a “path to commercialization” it calls the “FusionDirect” technology program. The next step is “Starblazer” which is a high-field, turbulence-optimized stellarator the company is developing as a commercial fusion pilot plant design. ...
myfaithfulmetalwatchdogwasputtingmeinahyperbolicorbitthatwouldtakemewithinonemileoftheneutronstar'ssurface.Twenty-fourhourstofall,twenty-fourhourstorise...andduringthattimesomethingwouldtrytokillme.AssomethinghadkilledtheLaskins.Thesametypeofautopilot,withthesameprogram,hadchosentheLaskins’orbit.Ithadnotcaused...
The ref i tted SLy4 ′ force can improve descriptions of f i nite nuclei but slightly reduces the radius ofneutron star of 1.4 solar mass. We found that the extended SLy4 force with a higher-order density dependence canproperly describe properties of both f i nite nuclei and GW170817 ...
内容提示: Draft version February 11, 2022Typeset using L A T E X twocolumn style in AASTeX63Population Properties of Gravitational-Wave Neutron Star–Black Hole MergersJin-Ping Zhu , 1 Shichao Wu , 2,3 Ying Qin , 4 Bing Zhang , 5,6 He Gao , 7 and Zhoujian Cao71 Department of ...
In this work we apply a deep-learning approach to rapidly identify and characterize transient gravitational-wave signals from binary neutron-star mergers in real LIGO data. We show for the first time that artificial neural networks can promptly detect and characterize binary neutron star gravitational...