CHANDRASEKHAR LIMIT வார்த்தையின் சொல்லிலக்கணம்
Named after S. Chandrasekhar, who calculated it.
«CHANDRASEKHAR LIMIT» தொடர்புடைய ஆங்கிலம் புத்தகங்கள்
பின்வரும் புத்தக விவரத்தொகுப்புத் தேர்ந்தெடுப்பில்
Chandrasekhar limit இன் பயன்பாட்டைக் கண்டறியுங்கள்.
Chandrasekhar limit தொடர்பான புத்தகங்கள் மற்றும் ஆங்கிலம் இலக்கியத்தில் அதன் பயன்பாட்டுச் சூழலை வழங்குவதற்கு அதிலிருந்து பெறப்பட்ட சுருக்கமான சாரங்களைத் தொடர்புபடுத்துகின்றன.
1
Three Steps to the Universe: From the Sun to Black Holes to ...
This maximum mass, now known as the Chandrasekhar limit, is about 1.4 solar
masses. If the mass is larger than the Chandrasekhar limit, the pressure is never
strong enough to resist gravity. A white dwarf can have a mass below the ...
David Garfinkle, Richard Garfinkle, 2009
Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online.
Frederic P. Miller, Agnes F. Vandome, McBrewster John, 2010
The Chandrasekhar limit is an upper bound on the mass of bodies made from
electron-degenerate matter, a dense form of matter which consists of nuclei
immersed in a gas of electrons. The limit is the maximum nonrotating mass which
can ...
4
An Introduction to the Study of Stellar Structure
In chapters i-iv, Chandrasekhar presents the "classical" background necessary to his argument: the laws of thermodynamics (from Carathéodory's rigorous axiomatic standpoint), adiabatic and polytropic laws, and the work of Ritter, Emden, ...
5
In Quest of the Universe
The Chandrasekhar Limit Even though electron degeneracy supports the white
dwarf against collapsing completely, there is a limit to the amount of pressure that
degenerate electrons can withstand. In 1930, a 19-year-old student on his way ...
6
Articles on Astrophysics, Including:
Chandrasekhar Limit, ...
Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online.
7
In Quest of the Stars and Galaxies
Chandrasekhar limit The limit to the mass of a white dwarf star, above which it
cannot be supported by electron degeneracy and cannot exist as a white dwarf.
More than 1000 stars have been identified as white dwarfs, but none is bright ...
Edison State College Fort Myers Florida Theo Koupelis, Theo Koupelis, 2010
8
Theory of Neutron Star Magnetospheres
Consequently adding mass to a white dwarf can in principle push it over the
Chandrasekhar limit and allow it to collapse to the neutron star stage. If the
maximum neutron star mass were less than the maximum white dwarf mass, a
collapsing ...
9
A Brief History of Time:
(This mass is now known as the Chandrasekhar limit.) A similar discovery was
made about the same time by the Russian scientist Lev Davidovich Landau. This
had serious implications for the ultimate fate of massive stars. If a star's mass is ...
10
Encyclopedia of Space and Astronomy
Early in his career he demonstrated that there was an upper limit (now called the
Chandrasekhar limit) to the mass of a white dwarf star. In 1937 Chandrasekhar
immigrated from India to the United States, where he joined the faculty of the ...
«CHANDRASEKHAR LIMIT» வார்த்தையைக் கொண்டுள்ள புதிய உருப்படிகள்
பின்வரும் செய்தி உருப்படிகளின் சூழலில்
Chandrasekhar limit என்ற வார்த்தையைப் பயன்படுத்துவது பற்றியும் எப்படிப் பயன்படுத்துவது என்பதைப் பற்றியும் தேசிய மற்றும் பன்னாட்டு அச்சகங்கள் என்ன பேசியிருக்கின்றன என்பதைக் கண்டறியுங்கள்.
What killed the white dwarfs? (Aside from the giant explosion)
Theoretically, there's a maximum mass the white dwarf can have before it becomes unstable: the Chandrasekhar limit, roughly 1.4 times the ... «Ars Technica, மே 15»
Indian physicists crack puzzle of exploding stars
The results suggest that the standard Chandrasekhar limit for white dwarf stars can be violated through an alternative theory of gravity, ... «Calcutta Telegraph, ஏப்ரல் 15»
Astronomers discover supernova subset which could allow for more …
This point is known as the Chandrasekhar limit, which occurs when the white dwarf achieves a mass the equivalent to 1.4 times that of our Sun, ... «Gizmag, மார்ச் 15»
Dyson Spheres and Swarms around White Dwarfs avoid two out of …
... very carefully, its luminosity could be sustained at 0.0004 solar for aeons before it ran into the Chandrasekhar Limit at 1.44 solar masses. «Next Big Future, மார்ச் 15»
Astronomers detect star leaving the Milky Way at record speeds
This is known as the Chandrasekhar limit, and very soon after the star explodes in spectacular thermonuclear fashion. It is hoped that further ... «Gizmag, மார்ச் 15»
Speeding star accelerated by exploding companion
"Usually a white dwarf has to grow and reach a specific mass called the Chandrasekhar limit, which is about 1.4 times the mass of the Sun, ... «ABC Science Online, மார்ச் 15»
White Dwarfs in Death Spiral Poised for a Spectacular Supernova
The Chandrasekhar limit is the greatest mass that a white dwarf star can have and support itself against gravitational collapse. It has a value of ... «The Daily Galaxy, பிப்ரவரி 15»
Asteroids or planets might trigger a supernova
White dwarfs explode when their mass exceeds a threshold known as the Chandrasekhar limit, which is about 1.4 times the mass of the sun. «Science News, பிப்ரவரி 15»
Cataclysmic Dawn
... not violent enough to expel more gas than is falling in, mass will accumulate onto the white dwarf star until it passes its Chandrasekhar limit. «Space Fellowship, ஜனவரி 15»
Indian Nobel Laureates
Chandrasekhar was awarded for his theory on white dwarf stars' limitation named after him as “Chandrasekhar limit”. 6. Dr Amartya Sen. «Zee News, டிசம்பர் 14»
இல் உள்ள வார்த்தைகளில் மறைக்கப்பட்டிருக்கும் எல்லாவற்றையும் கண்டறியுங்கள் 
