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Sunday, December 31, 2017

Black hole - Wikipedia

https://en.wikipedia.org/wiki/Black_hole
A black hole is a region of spacetime exhibiting such strong gravitational effects that nothing—not even particles and electromagnetic radiation such as light—can escape from inside it. The theory of general relativity predicts that a sufficiently compact mass can deform spacetime to form a black hole. The boundary of the ...
‎Supermassive black hole · ‎Hawking radiation · ‎Stellar black hole · ‎Gravitational lens

Stephen Hawking's New Black Hole Theory: Scientists ... - Space.com

https://www.space.com › Science & Astronomy
Jan 28, 2014 - Stephen Hawking's New Black Hole Theory: Scientists Remain Unconvinced. ... Famed astrophysicist Stephen Hawking has shaken up the popular science world with his newest study about the basic nature of black holes, but is his idea revolutionary? ... This paradox pits Einstein's theory of ...
Posted by sayanyein at 5:58 PM No comments:

Friday, December 29, 2017

29 dec. 2017 Learning psychology . Id, ego and super-ego - Wikipedia https://en.wikipedia.org/wiki/Id,_ego_and_super-ego

Image result for id ego superego theory
www.simplypsychology.org
According to this Freudian model of the psyche, the id is the set of uncoordinated instinctual trends; the super-ego plays the critical and moralizing role; and the ego is the organized, realistic part that mediates between the desires of the id and the super-ego.

29 dec. 2017 Learning psychology . Id, ego and super-ego - Wikipedia https://en.wikipedia.org/wiki/Id,_ego_and_super-ego.

Id, ego and super-ego - Wikipedia

https://en.wikipedia.org/wiki/Id,_ego_and_super-ego
People also ask

What is the id ego and superego?
The id, ego, and superego are names for the three parts of the human personality which are part of Sigmund Freud's psychoanalytic personality theory. According to Freud, these three parts combine to create the complex behavior of human beings.

Examples of Id Ego and Superego

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What is the ego and the id?
The id is an important part of our personality because as newborns, it allows us to get our basic needs met. Freud believed that the id is based on our pleasure principle. In other words, the id wants whatever feels good at the time, with no consideration for the reality of the situation.Aug 21, 2014

Id, Ego, Superego, and the Unconscious in Psychology 101 at ...

https://allpsych.com/psychology101/ego/
Search for: What is the ego and the id?
What is id ego and superego with examples?
According to Sigmund Freud, personality consists of the id, ego, and superego. These three parts work together to create a complete personality. The superego is the social component and is your conscience. The id is your instinct, while the ego is your conscious decisions.Sep 21, 2014

The Superego: Definition & Examples - Video & Lesson Transcript ...

study.com/academy/lesson/the-superego-definition-examples-quiz.html
Search for: What is id ego and superego with examples?
What are the ID?
An identity document (also called a piece of identification or ID, or colloquially as papers) is any document which may be used to prove a person's identity. If issued in a small, standard credit card size form, it is usually called an identity card (IC, ID card, Citizen Card or Passport Card)

superego
suːpərˈiːɡəʊ/
noun
Psychoanalysis
noun: superego; plural noun: superegos; noun: super-ego; plural noun: super-egos
  1. the part of a person's mind that acts as a self-critical conscience, reflecting social standards learned from parents and teachers.

    "the father is the model for the superego"
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What is the id ego and superego?
What is the ego and the id?
What is id ego and superego with examples?
What are the ID?
Posted by sayanyein at 10:26 PM No comments:

29 dec. 2017 Gravitational collapse From Wikipedia, the free encyclopedia

https://en.wikipedia.org/wiki/Gravitational_collapse
29 dec. 2017,


Contents

  • 1 Star formation
  • 2 Stellar remnants
    • 2.1 White dwarf
    • 2.2 Neutron star
    • 2.3 Black holes
      • 2.3.1 Theoretical minimum radius for a star
  • 3 See also
  • 4 References
  • 5 External links

Star formation

Main article: Star formation
An interstellar cloud of gas will remain in hydrostatic equilibrium as long as the kinetic energy of the gas pressure is in balance with the potential energy of the internal gravitational force.
Mathematically this is expressed using the virial theorem, which states that, to maintain equilibrium, the gravitational potential energy must equal twice the internal thermal energy.[1]
If a pocket of gas is massive enough that the gas pressure is insufficient to support it, the cloud will undergo gravitational collapse.
The mass above which a cloud will undergo such collapse is called the Jeans mass.
This mass depends on the temperature and density of the cloud, but is typically thousands to tens of thousands of solar masses.[2]

29 dec, 2017.


Stellar remnants


NGC 6745 produces material densities sufficiently extreme to trigger star formation through gravitational collapse
At what is called the death of the star (when a star has burned out its fuel supply), it will undergo a contraction that can be halted only if it reaches a new state of equilibrium.
Depending on the mass during its lifetime, these stellar remnants can take one of three forms:
  • White dwarfs, in which gravity is opposed by electron degeneracy pressure[3]
  • Neutron stars, in which gravity is opposed by neutron degeneracy pressure and short-range repulsive neutron–neutron interactions mediated by the strong force
  • Black hole, in which there is no force strong enough to resist gravitational collapse

White dwarf

Main article: White dwarf
The collapse of the stellar core to a white dwarf takes place over tens of thousands of years, while the star blows off its outer envelope to form a planetary nebula.
If it has a companion star, a white dwarf-sized object can accrete matter from the companion star until it reaches the Chandrasekhar limit (about one and a half times the mass of our Sun) at which point gravitational collapse takes over again.
While it might seem that the white dwarf might collapse to the next stage (neutron star), they instead undergo runaway carbon fusion, blowing completely apart in a Type Ia supernova.

Neutron star

Main article: Neutron star
Neutron stars are formed by gravitational collapse of the cores of larger stars, and are the remnant of other types of supernova. They are so compact that a Newtonian description is inadequate for an accurate treatment, which requires the use of Einstein's general relativity.

Black holes

Main article: Black hole

Logarithmic plot of mass against mean density (with solar values as origin) showing possible kinds of stellar equilibrium state. For a configuration in the shaded region, beyond the black hole limit line, no equilibrium is possible, so runaway collapse will be inevitable.
According to Einstein's theory, for even larger stars, above the Landau-Oppenheimer-Volkoff limit, also known as the Tolman–Oppenheimer–Volkoff limit (roughly double the mass of our Sun) no known form of cold matter can provide the force needed to oppose gravity in a new dynamical equilibrium. Hence, the collapse continues with nothing to stop it.

Simulated view from outside black hole with thin accretion disc, by J. A. Marck[4]
Once a body collapses to within its Schwarzschild radius it forms what is called a black hole, meaning a space-time region from which not even light can escape.
It follows from a theorem of Roger Penrose[5] that the subsequent formation of some kind of singularity is inevitable.
Nevertheless, according to Penrose's cosmic censorship hypothesis, the singularity will be confined within the event horizon bounding the black hole, so the space-time region outside will still have a well behaved geometry, with strong but finite curvature, that is expected[6] to evolve towards a rather simple form describable by the historic Schwarzschild metric in the spherical limit and by the more recently discovered Kerr metric if angular momentum is present.
On the other hand, the nature of the kind of singularity to be expected inside a black hole remains rather controversial.
According to some theories, at a later stage, the collapsing object will reach the maximum possible energy density for a certain volume of space or the Planck density (as there is nothing that can stop it).
This is when the known laws of gravity cease to be valid.[7]There are competing theories as to what occurs at this point, but it can no longer really be considered gravitational collapse at that stage.[8]

Theoretical minimum radius for a star

The radii of larger mass neutron stars (about 2.0 solar mass) are estimated to be about 12-km, or approximately 2.0 times their equivalent Schwarzschild radius.
It might be thought that a sufficiently massive neutron star could exist within its Schwarzschild radius (1.0 SR) and appear like a black hole without having all the mass compressed to a singularity at the center; however, this is probably incorrect.
Within the event horizon, matter would have to move outward faster than the speed of light in order to remain stable and avoid collapsing to the center.
No physical force therefore can prevent a star smaller than 1.0 SR from collapsing to a singularity (at least within the currently accepted framework of general relativity; this doesn’t hold for the Einstein–Yang–Mills–Dirac system). A model for nonspherical collapse in general relativity with emission of matter and gravitational waves has been presented.[9]

See also

  • Big Crunch
  • Stellar evolution
  • Thermal runaway

References



  • Kwok, Sun (2006). Physics and chemistry of the interstellar medium. University Science Books. pp. 435–437. ISBN 1-891389-46-7.

    1. Bedran, ML et al.(1996)."Model for nonspherical collapse and formation of black holes by emission of neutrinos, strings and gravitational waves", Phys. Rev. D 54(6),3826.

    External links

    • Gravitational collapse on arxiv.org
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  • Prialnik, Dina (2000). An Introduction to the Theory of Stellar Structure and Evolution. Cambridge University Press. pp. 198–199. ISBN 0-521-65937-X.

  • And theoretically Black dwarfs - but: "...no black dwarfs are expected to exist in the universe yet"

  • Class. Quantum Grav. 13 (1996)p393

  • "Gravitational collapse and space-time singularities", R. Penrose, Phys. Rev. Let. 14 (1965) p 57

  • B. Carter, "Axisymmetric black hole has only two degrees of freedom", Phys. Rev. Let. 26 (1971) p331

  • "Black Holes - Planck Unit? WIP". Physics Forums. Archived from the original on 2008-08-02.

  • Brill, Dieter (19 January 2012). "Black Hole Horizons and How They Begin". Astronomical Review.


  • Posted by sayanyein at 3:19 AM No comments:

    Learning Eng. slangs. 29 dec. 2017

    Learning Eng. slangs.29 dec. 2017

     booze
    buːz/Submit
    informal
    noun
    1.
    alcoholic drink.
    "I wonder where he's hidden his booze"
    synonyms: alcohol, alcoholic drink, liquor, intoxicating liquor, drink, strong drink, spirits, intoxicants; More
    verb
    1.
    drink alcohol, especially in large quantities.
    "I expect he's boozing"
    synonyms: drink, have a drink, drink alcohol, indulge, tipple, imbibe, swill; More
    Feedback
    Translations and more def
    Posted by sayanyein at 1:46 AM No comments:

    Thursday, December 28, 2017

    adhd 28 dec. 2017

    Image result for adhd meaning
    attention deficit hyperactivity disorder
    ADHD, or attention deficit hyperactivity disorder, is a medical condition that affects how well someone can sit still, focus, and pay attention. People with ADHD have differences in the parts of their brains that control attention and activity. This means that they may have trouble focusing on some tasks and subjects.
    ADHD - KidsHealth
    m.kidshealth.org › teens › adhd
    Feedback
    About t
    Posted by sayanyein at 2:33 AM No comments:

    Wednesday, December 27, 2017

    ဥာဏ္ေကာင္းသူမ််ားေရာ ဂါမ်ားလွ၏ 28dec. 2017.

    VIDEOSARTICLESPLAYLISTSEXPERTSPODCASTEDGE

    Why Highly Intelligent People Suffer More Mental and Physical Disorders

    December 12, 2017 by TEODORA ZAREVA

    People with high IQ are considered to have an advantage in many domains. They are predicted to have higher educational attainment, better jobs, and a higher income level. Yet, it turns out that a high IQ is also associated with various mental and immunological diseases like depression, bipolar disorder, anxiety, ADHD as well as allergies, asthma, and immune disorders. Why is that? A new paper published in the journal Intelligence reviews the literature and explores the mechanisms that possibly underlie this connection.

    The study authors compared data taken from 3,715 members of the American Mensa Society (people who have scored in the top 2% of intelligent tests) to data from national surveys in order to examine the prevalence of several disorders in those with higher intelligence compared to the average population.

    The results showed that highly intelligent people are 20% more likely to be diagnosed with autism spectrum disorder (ASD), 80% more likely to be diagnosed with ADHD, 83% more likely to be diagnosed with anxiety, and 182% more likely to develop at least one mood disorder.

    When it comes to physiological diseases, people with high cognitive abilities are 213% more likely to have environmental allergies, 108% more likely to have asthma, and 84% more likely to have an autoimmune disease.

    Credit: Journal of Intelligence / High intelligence: A risk factor for psychological and physiological overexcitabilities

    The researchers turned to the field of psychoneuroimmunology (PNI) to look for some of the answers. PNI examines how the chronic stress accumulated as a response to environmental factors influences the communication between the brain and the immune system. 

    The researchers point out that highly intelligent people have tendencies for “intellectual overexcitabilites” and a hyper-reactivity of the central nervous system. On the one hand, this gives people with high IQ heightened awareness that helps their creative and artistic work. In fact, the field of cognitive ability recognizes one aspect of highly intelligent people to be “a broader and deeper capacity to comprehend their surroundings.” 

    This hyper-reactivity, however, can also lead to deeper depressions and poor mental health. This turns out to be particularly true for poets, novelists and people with high verbal intelligence. Their intense emotional response to the environment increases tendencies for rumination and worry, both of which predict depression and anxiety disorders. 

    Heightened psychological responses can affect immunity, write the researchers. People with overexcitabilites may have strong reactions to seemingly harmless external stimuli like an annoying clothing tag or a sound. This reaction may turn into low level chronic stress and launch an inappropriate immune response.

    When the body believes it is in danger (regardless of whether it is an objectively real one like a toxin or an imagined one like an annoying sound), it launches a cascade of physiological responses that include a myriad of hormones, neurotransmitters and signaling molecules. When these processes are chronically activated, they can alter the body and the brain, dysregulate immune function and lead to conditions like asthma, allergies and autoimmune diseases. 

    The scientific literature has confirmed the association between gifted children and an increased rate of allergies and asthma. One study shows that 44% of those with an IQ over 160 suffered from allergies compared to 20% of age-matched peers. Тhe exploratory study done by the authors of this latest paper further supports that connection.

    Based on their findings and previous studies the researchers have termed this phenomenon the hyper brain / hyper body theory of integration, explaining that: 

    The overexcitabilities specific to those with high intelligence may put these individuals at risk for hypersensitivity to internal and/or external environmental events. The rumination and worry that accompanies this heightened awareness may contribute to a chronic pattern of fight, flight, or freeze responses which then launch a cascade of immunological events. [...] Ideally, immune regulation is an optimal balance of pro- and anti-inflammatory response. It should zero in on inflammation with force and then immediately return to a calm state. In those with the overexcitabilities previously discussed, including in those with ASD, this system appears to fail to achieve a balance and thus inflammatory signals create a state of chronic activation.




    Credit: Journal of Intelligence / High intelligence: A risk factor for psychological and physiological overexcitabilities

    The authors conclude that it is important to further study the relationship between high intelligence (particularly the top 2%) and illness, especially in order to demonstrate causation and further bring to light the negative aspects of having a high IQ. As they say, “this gift can either be a catalyst for empowerment and self-actualization or it can be a predictor of dysregulation and debilitation” and in order to serve this group, it is important “to acknowledge the rumbles of thunder that follow in the wake of their brilliance.”







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    Posted by sayanyein at 7:01 PM No comments:

    27 dec. 2017 ဘအမိ္် ုး ဘိုးတူ ေမာင္ေနာင္တ နဲ႕ေျမး " ေတာင္ေပၚသား"

    Hla Myint added 2 new photos.
    March 21 ·
    ဘအမိ္် ုး ဘိုးတူ
    ေမာင္ေနာင္တ နဲ႕ေျမး " ေတာင္ေပၚသား"


    ေမာ္လီသန္း ေခၚ
    ေဒၚခင္ေမာ္ေမာ္ က  "သူ .သားလပ္ ေတာင္ေပၚသား " ဟာ သူ႕ အေဖ ပီတာဘသန္း ေခၚ
    ေမာင္ေနာင္တ
    ေခၚ
    ဧရာဝတီ ကိုယ္စားလွယ္ၾကီ း ဦးဘသန္း နဲ႔ တူတာဗ်
    အဲဒီဘိုးေတာ္က အဂၤလိပ္ ေခတ္က
    မႏၲေလး ကယ္လီ ေက်ာင္းကေနပီး ၁၀ တန္းကို အဂၤလိပ္ စာဂုဏ္ထူး နဲ႕ေအာင္တာ တဲ႕ ဗ်
    ရန္ကုန္ တကၠသို္လ္မွာ ဆရာေဇာ္ဂ်ီ ေခၚ ဦးသိန္းဟန္ / ေဗဒါလမ္း ကဗ်ာဆရာ တို ့
    ဝန္ ၾကီးခ် ုပ္ ဦ းန ုတို ့
    နဲ႕ တတန္းထဲ တက္ခဲ႔ တာတဲ႕ ဗ်
    သူ ့ ရီးစားကို မိဘေတြ က ICS တေယာက္နဲ႔ သေဘာတူတာနဲ ႕ သူက ေနာက္ဆုတ္ေပးလိုက္တာကေန အသဲကြဲ ျပီ း
    BA အထက္တန္းေရာက္မွ တႏွစ္လံုးအတန္းမတက္ဘဲ အင္းယားကန္ေဘးသြားထိုင္ထိုင္ေနတာတဲ႕ ဗ်
    သူ အေဖကေတာ့ တႏွစ္လံုး မႏၲေလးကေန
    ေငြပို ့ရတာေပါ့ ဗ်ာ
    အခ်စ္ကိစၥ နဲ႕ အသဲကြဲျပီ း
    BA ဘြဲ႕ မရေတာ့ ဘူး ဗ်
    ICS ဆိုတာက Imperial Civil Service
    ဘုရင္မ ပဋိဥာဏ္ ခံ အုပ္ခ် ုပ္ေရး မွ ူးေပါ့
    အရပ္ အေခၚ နယ္ပိုင္ ဝန္ေထာက္ေပါ့ ဗ်ာ
    ေနာက္ေတာ့ ေနာင္တ ရျပီ း ေမာင္ေနာင္တ ကေလာင္နံမယ္နဲ႕ စာေရ းတာေပါ့ ဗ်ာ
    ဆရာ ၾကီးေဇာ္ ဂ်ီ တို ့ မင္းသု ဝဏ္ တို ့နဲ႕
    ေခတ္ျပိ ုင္ေပါ့
    ေမာင္ေနာင္တ က ဘာသာျပန္ေကာင္းတာဗ်
    သူ ရဲ ႕ masterpiece ကေတာ့ ကမၻာ ေက်ာ္ The vagabond ဝတၳ ုဘာသာျပန္
    ဝတၴ ုဘဲဗ်
    အဲ ဒီ အေၾကာင္း ရန္ကုန္တကၠသိုလ္ ေရႊ ရ တု
    အထိမ္းအမွတ္ မဂၢဇင္းမွာ သူ ေရးဘူးတယ္ ဗ်
    ေမာင္ေနာင္တ၏ေျမး ေတာင္ေပၚသား ကိုဝင္းေခၚ လွျမင့္ဝင္း ကသူအဖိုးေလာက္ေတာ့
    အခ်စ္အတြက္ သိတ္ မထိဘူးဗ်
    ေတာ္သေလာက္ေတာ့ ျဖစ္မလာရွာဘူး ဗ်
    အင္ဂ်င္နီယာ အမွတ္ကို ၂မွတ္ထဲ နဲ႕ လြဲသြားရွာတယ္
    မႏၲေလး အထက ၁၆ က သူ ရီးစား ေကာင္မေလးနဲ႕ အဆင္မေျပ လို႕ တမွိ ုင္
    တေထြေထြ ျဖစ္ေနလို႕ သူအေမက ရန္ကုန္
    RU ပို ့လိုက္တာ math ဘြဲ႕ေလးေတာ့ ရသြား
    ရွာတယ္
    RU မွာလဲ အတန္းမတက္ဘဲ ဓါတ္ပံုထဲက အတိုင္းပါ ဘဲဗ်ာ
    အင္းယားကန္ ေဘး သြားလိုက္ campus ထဲတမွိ ုင္တေထြေထြ နဲ႕
    သစ္ပုပ္ ပင္ၾကီးေအာက္သြားသြားထိုင္ေနလိုက္လုပ္ေန
    တာသူ႕အကို ေရႊမင္းသားက သနားပီး
    ရန္ကုန္ျမိ ု႕ လယ္
    ဘုန္း ၾကီးလမ္း က ကြမ္းေတာင္ကိုင္ သူတိုး သမီးေခ်ာနဲ႕ ေပးစားလိုက္လို႕ ကံေကာင္းေထာက္မ ပီး math ဘြဲ႕ေလးေတာ့
    ရလိုက္ရွာပါတယ္ဗ်ာ
    သေဗၺ သခၤါရာ အနတၱာ
    ဆရာျငိမ္း
    from mandalay with love.
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    14 You, Oo Kyaw, Si Thar Htwe and 11 others
    Posted by sayanyein at 8:19 AM No comments:
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