Thursday, August 17, 2023

Memory

https://youtu.be/VzxI8Xjx1iw

Bernhard Wenzl •

 
  • Working memory is the ability of the brain to maintain a temporary representation of information about the task that an animal is currently engaged in. This sort of dynamic memory is thought to be mediated by the formation of cell assemblies—groups of activated neurons that maintain their activity by constantly stimulating one another.[104]
  • Episodic memory is the ability to remember the details of specific events. This sort of memory can last for a lifetime. Much evidence implicates the hippocampus in playing a crucial role: people with severe damage to the hippocampus sometimes show amnesia, that is, inability to form new long-lasting episodic memories.[105]
  • Semantic memory is the ability to learn facts and relationships. This sort of memory is probably stored largely in the cerebral cortex, mediated by changes in connections between cells that represent specific types of information.[106]
  • Instrumental learning is the ability for rewards and punishments to modify behavior. It is implemented by a network of brain areas centered on the basal ganglia.[107]
  • Motor learning is the ability to refine patterns of body movement by practicing, or more generally by repetition. A number of brain areas are involved, including the premotor cortex, basal ganglia, and especially the cerebellum, which functions as a large memory bank for microadjustments of the parameters of movement.[108]





Tuesday, August 08, 2023

I am Alive and Always Watching

 I just wanted to say that to prevent cancellation of this blog and account I am showing that I am alive and well.

Tuesday, May 10, 2022

Black hole Annoucements on May 12th

Garching bei München, European Southern Observatory, see ESO Media Advisory (15:00 CEST) - Live streaming at ESO Website and ESO YouTube Channel

Mexico City, CONACyT, see CONACyT Media Advisory (08:00 CDT) - Live streaming at CONACyT YouTube Channel

Santiago de Chile, Joint ALMA Observatory, see ALMA Media Advisory (09:00 CLT)

Shanghai, Shanghai Astronomical Observatory, see Shanghai Astronomical Observatory Media Advisory (21:00 CST)

Taipei, Academia Sinica Institute for Astronomy and Astrophysics (21:00 CST), see YouTube Live Streaming.

Tokyo, National Astronomical Observatory of Japan (22:00 JST), see YouTube Live Streaming.

Washington D.C.,  National Press Club, see National Science Foundation Media Advisory (09:00 EDT) - Live streaming at NSF Webpage and NSF Facebook

Madrid (15:00 CEST, see CSIC YouTube streaming)

South Korea (22:00 KST, see YouTube Live Streaming

How to Understand the Black Hole Image

Saturday, December 05, 2020

The Sound of the Perfect Fluid

 

 The sound of the perfect fluid

 


Perfect Fluid

Perfect fluid

From Wikipedia, the free encyclopedia
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The stress–energy tensor of a perfect fluid contains only the diagonal components.

In physics, a perfect fluid is a fluid that can be completely characterized by its rest frame mass density and isotropic pressure p.

Real fluids are "sticky" and contain (and conduct) heat. Perfect fluids are idealized models in which these possibilities are neglected. Specifically, perfect fluids have no shear stresses, viscosity, or heat conduction.

In space-positive metric signature tensor notation, the stress–energy tensor of a perfect fluid can be written in the form

where U is the 4-velocity vector field of the fluid and where is the metric tensor of Minkowski spacetime.

In time-positive metric signature tensor notation, the stress–energy tensor of a perfect fluid can be written in the form

where U is the 4-velocity of the fluid and where is the metric tensor of Minkowski spacetime.

This takes on a particularly simple form in the rest frame

where is the energy density and is the pressure of the fluid.


Perfect fluids admit a Lagrangian formulation, which allows the techniques used in field theory, in particular, quantization, to be applied to fluids. This formulation can be generalized, but unfortunately, heat conduction and anisotropic stresses cannot be treated in these generalized formulations.[why?]

Perfect fluids are used in general relativity to model idealized distributions of matter, such as the interior of a star or an isotropic universe. In the latter case, the equation of state of the perfect fluid may be used in Friedmann–Lemaître–Robertson–Walker equations to describe the evolution of the universe.

In general relativity, the expression for the stress–energy tensor of a perfect fluid is written as

where U is the 4-velocity vector field of the fluid and where is the metric, written with a space-positive signature.

See also

References

External links