STEPHEN HAWKING AUTOBIOGRAPHY
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This document summarizes a seminar presentation on black holes. It defines a black hole as a region of spacetime where gravity is so strong that nothing, not even light, can escape. It describes three types of black holes based on size: primordial, stellar, and supermassive. Key properties of black holes are discussed, including the event horizon boundary and singularity at the center. As mass falls into a black hole, its properties like shape and composition vanish. The document also briefly outlines concepts like accretion disks, how black holes generate energy, and limits on their brightness.
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The document introduces black holes by discussing their origins from proposals in the 18th century and definitions put forth by Einstein. It describes black holes as regions of space where gravity is so strong that not even light can escape, and that are created when large stars collapse at the end of their life cycles. The document outlines three main types of black holes and describes the key parts of black holes, including their event horizons, singularities, accretion disks, and ergospheres. Hawking radiation, in which black holes are predicted to emit and evaporate over time via quantum effects, is also summarized.
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Black hole
Recent advances in the study of black holes include:
1. The first image of a black hole was captured in 2019 using the Event Horizon Telescope, showing the shadow of the supermassive black hole at the center of the Messier 87 galaxy.
2. Gravitational waves detected in 2015 by the LIGO observatory provided direct evidence of black holes from the merger of two stellar-mass black holes.
3. Observations of stars orbiting Sagittarius A* provided evidence of a supermassive black hole at the center of the Milky Way galaxy.
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The blackhole origins........
This document discusses the history and properties of black holes. It explains that black holes were first proposed in the 18th century and describes how Einstein's general relativity theory led to the modern understanding of them. The key aspects covered include: the formation of black holes via gravitational collapse; the defining presence of an event horizon and singularity at the center; Hawking's prediction that black holes emit thermal radiation and eventually evaporate; and ongoing questions around merging black holes and resolving information paradoxes.
Big Bang Theory & Other Recent Sciences || 2014 - Dr. Mahbub Khan
RECENT SCIENCES
Big Bang, Dark Matter, Dark Energy, Black Hole, Neutrino, God Particle, Higgs Field, Graviton, Expansion of Universe, and Search for Life elsewhere in the Cosmos
Blackhole
A black hole is a region of spacetime where the gravitational pull is so strong that nothing, not even light, can escape. The boundary of this region is called the event horizon. Black holes form when very massive stars collapse at the end of their life cycle. Supermassive black holes millions of times the mass of our sun may form at the centers of galaxies by absorbing other stars and merging with other black holes. While black holes themselves are invisible, their presence can be inferred through their interaction with surrounding matter like accretion disks and the orbits of nearby stars.
Black holes
1) A black hole is a region of spacetime where gravity is so strong that nothing, not even light, can escape. It has an event horizon boundary that marks the point of no return.
2) Black holes form when very massive stars collapse at the end of their life cycle. Supermassive black holes millions of times the mass of our sun may form at the centers of galaxies through mergers with other black holes and stars.
3) While black holes themselves are invisible, their presence can be inferred through their interaction with nearby matter like gas and stars. This surrounding material often forms an accretion disk and bright radiation that astronomers can observe.
Recommended
Black hole ppt
The document introduces black holes by discussing their origins from proposals in the 18th century and definitions put forth by Einstein. It describes black holes as regions of space where gravity is so strong that not even light can escape, and that are created when large stars collapse at the end of their life cycles. The document outlines three main types of black holes and describes the key parts of black holes, including their event horizons, singularities, accretion disks, and ergospheres. Hawking radiation, in which black holes are predicted to emit and evaporate over time via quantum effects, is also summarized.
Conquering space
This presentation is prepared for the students of 12 grade to make them familiar with the cosmic system.
GSA.pptx
The document summarizes key concepts related to astronomical bodies and phenomena. It discusses comets, asteroids, meteoroids, nebulae, constellations, and other universal objects. It then covers concepts like the Big Bang theory, the composition of the universe including dark matter and dark energy, black holes, and galaxies. Methods for determining the age of the universe are also mentioned.
Black hole
Recent advances in the study of black holes include:
1. The first image of a black hole was captured in 2019 using the Event Horizon Telescope, showing the shadow of the supermassive black hole at the center of the Messier 87 galaxy.
2. Gravitational waves detected in 2015 by the LIGO observatory provided direct evidence of black holes from the merger of two stellar-mass black holes.
3. Observations of stars orbiting Sagittarius A* provided evidence of a supermassive black hole at the center of the Milky Way galaxy.
4. X-ray binaries, where matter falls from a donor star onto a compact object like a neutron star or black hole
The blackhole origins........
This document discusses the history and properties of black holes. It explains that black holes were first proposed in the 18th century and describes how Einstein's general relativity theory led to the modern understanding of them. The key aspects covered include: the formation of black holes via gravitational collapse; the defining presence of an event horizon and singularity at the center; Hawking's prediction that black holes emit thermal radiation and eventually evaporate; and ongoing questions around merging black holes and resolving information paradoxes.
Big Bang Theory & Other Recent Sciences || 2014 - Dr. Mahbub Khan
RECENT SCIENCES
Big Bang, Dark Matter, Dark Energy, Black Hole, Neutrino, God Particle, Higgs Field, Graviton, Expansion of Universe, and Search for Life elsewhere in the Cosmos
Blackhole
A black hole is a region of spacetime where the gravitational pull is so strong that nothing, not even light, can escape. The boundary of this region is called the event horizon. Black holes form when very massive stars collapse at the end of their life cycle. Supermassive black holes millions of times the mass of our sun may form at the centers of galaxies by absorbing other stars and merging with other black holes. While black holes themselves are invisible, their presence can be inferred through their interaction with surrounding matter like accretion disks and the orbits of nearby stars.
Black holes
1) A black hole is a region of spacetime where gravity is so strong that nothing, not even light, can escape. It has an event horizon boundary that marks the point of no return.
2) Black holes form when very massive stars collapse at the end of their life cycle. Supermassive black holes millions of times the mass of our sun may form at the centers of galaxies through mergers with other black holes and stars.
3) While black holes themselves are invisible, their presence can be inferred through their interaction with nearby matter like gas and stars. This surrounding material often forms an accretion disk and bright radiation that astronomers can observe.
Black holes
1) A black hole is a region of spacetime where gravity is so strong that nothing, not even light, can escape. It has an event horizon boundary that marks the point of no return.
2) Black holes form when very massive stars collapse at the end of their life cycle. Supermassive black holes millions of times the mass of our sun may form at the centers of galaxies through mergers with other black holes and stars.
3) While black holes themselves are invisible, their presence can be inferred through their interaction with nearby matter like gas and stars. This surrounding material often forms an accretion disk and bright radiation that astronomers can observe.
Black holes
Black holes are regions of extreme gravity from which nothing, not even light, can escape. They form from the collapse of very massive stars over 3 solar masses. Black holes come in different types depending on their charge and rotation. They contain a central singularity of infinite density and an event horizon boundary. Near a black hole, time dilates such that time slows greatly and stops at the event horizon. Black holes also emit Hawking radiation over time by emitting virtual particle pairs, causing them to lose mass.
Black holes (2)
Black holes are formed when giant stars collapse under their own gravity. If the star's mass is large enough, its gravitational pull becomes so strong that not even light can escape, forming an event horizon around the black hole. Anything that crosses this boundary, including light, cannot escape the black hole. Black holes can also rotate, forming an ergosphere outside the event horizon where the rotation of the black hole drags spacetime itself along. While black holes themselves are invisible, astronomers can detect them through their interaction with nearby matter and the strong gravitational lensing they produce.
Black Holes
This document provides information about black holes, including their structure, theories about their formation and properties, and how they are detected. It discusses that a black hole has a singularity at its center with infinite density, is surrounded by an event horizon beyond which nothing can escape, and may be accompanied by an accretion disk and jets. It also describes Sagittarius A*, the supermassive black hole at the center of the Milky Way, and Cygnus X-1, the first identified black hole.
Black hole
1) A black hole is a region of spacetime where the gravitational pull is so strong that nothing, not even light, can escape.
2) The boundary of this region is called the event horizon. Although nothing can escape the event horizon, it appears to have no detectable features from within.
3) Black holes form when very massive stars collapse at the end of their life cycle. They can continue growing by absorbing mass and merging with other black holes, potentially forming supermassive black holes containing millions of solar masses.
Black holes
Black holes are regions of extremely strong gravity from which nothing, not even light, can escape. They form from the collapse of massive stars and come in several types depending on properties like charge and rotation. Black holes distort both space and time near them, slowing the flow of time for outside observers and bending light in a process called gravitational lensing. They also emit Hawking radiation and obey laws analogous to thermodynamics. Gravitational waves produced by black holes can help detect their presence.
Black hole
1) A black hole is an object with such strong gravity that not even light can escape, forming at the collapse of a massive star.
2) It has an "event horizon", the point of no return beyond which nothing, not even light, can escape the black hole.
3) Black holes were first theorized by geologist John Michell in 1783, and the modern theory was proposed by physicist Stephen Hawking.
Shadow of rotating Hayward blackhole bounded by Perfect Fluid Dark Matter
I do not have any questions. The document appears to be a research proposal on various topics related to black holes, including their formation, properties of rotating and charged black holes, geodesic motion, dark matter, Hawking radiation, and the shadow they cast.
black hole.pptx
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Presentation regarding some unknown facts about Black hole.
This project was given to me during my Engineering period.
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A REVIEW ARTICLE ON BLACK HOLE A MYSTERY IN THE UNIVERSE
This article reviews black holes, mysterious celestial objects with gravitational pulls so strong that not even light can escape. It discusses the historical background of black hole theory, defines what a black hole is, describes different types including stellar, supermassive, and microscopic black holes. The formation of black holes from collapsing stars is explained. While black holes pose no threat to life on Earth, objects close to a black hole's event horizon would be stretched out in a process called spaghettification. Though black holes themselves are invisible, astronomers can detect them through gravitational effects on nearby objects and energetic x-ray emissions from accretion disks.
What is a black hole
Black holes are regions of space where gravity is so strong that not even light can escape. They form when very massive stars collapse at the end of their life cycles. While black holes cannot be seen directly, astronomers can detect them by observing their effects on nearby objects like stars and gas, and through detection of x-rays emitted during accretion. Black holes come in different sizes, from stellar-mass black holes up to supermassive black holes that may exist at the centers of galaxies.
Black holes Samriddha Shil.....S@S
The document discusses black holes and their theoretical definition. It explains that black holes are areas of space-time with gravitational fields so strong that their escape velocity exceeds the speed of light. Black holes are theorized to form when very massive stars undergo supernovas and collapse inward. The document also discusses different types of black holes like stellar-mass, mid-mass, and supermassive black holes found at the centers of galaxies.
What are dead stars good for?
A lesson I gave to high school students during my time at Yale, with the Yale SPLASH student organisation.
Particle Properties of Waves
This document discusses the development of quantum mechanics. It summarizes that classical physics could not explain certain experimental observations, leading to quantum theory. Key events were Planck's blackbody radiation law, Einstein's explanation of the photoelectric effect using light quanta (photons), and Compton's discovery that photons transfer momentum to electrons. The photoelectric effect showed that light behaves as particles (photons), while the de Broglie hypothesis and Davisson-Germer experiment showed that electrons can behave as waves. This established the wave-particle duality of both light and matter.
BLACK HOLE-THE OTHER DIMENSION
"Black holes are where God divided by zero" - Albert Einstein
Black hole – A region in the space where the gravitational pull is so strong that neither substance nor light can leave this area.
period 7 Sheharyar Sohail Black Holes
Black holes are regions of space where the gravitational pull is so strong that nothing, not even light, can escape. Surrounding the black hole is an event horizon, which marks the point of no return beyond which the gravitational forces are inescapable. Albert Einstein's theory of general relativity first theorized black holes by explaining how gravity can bend space and time. Black holes have immense gravitational forces that can feed on and destroy stars that come too close, collapsing them into the black hole. The largest known black holes are supermassive black holes that can be millions of times the size of our sun.
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1) A black hole is a region of spacetime where gravity is so strong that nothing, not even light, can escape. It has an event horizon boundary that marks the point of no return.
2) Black holes form when very massive stars collapse at the end of their life cycle. Supermassive black holes millions of times the mass of our sun may form at the centers of galaxies through mergers with other black holes and stars.
3) While black holes themselves are invisible, their presence can be inferred through their interaction with nearby matter like gas and stars. This surrounding material often forms an accretion disk and bright radiation that astronomers can observe.
Black holes
Black holes are regions of extreme gravity from which nothing, not even light, can escape. They form from the collapse of very massive stars over 3 solar masses. Black holes come in different types depending on their charge and rotation. They contain a central singularity of infinite density and an event horizon boundary. Near a black hole, time dilates such that time slows greatly and stops at the event horizon. Black holes also emit Hawking radiation over time by emitting virtual particle pairs, causing them to lose mass.
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Black holes are formed when giant stars collapse under their own gravity. If the star's mass is large enough, its gravitational pull becomes so strong that not even light can escape, forming an event horizon around the black hole. Anything that crosses this boundary, including light, cannot escape the black hole. Black holes can also rotate, forming an ergosphere outside the event horizon where the rotation of the black hole drags spacetime itself along. While black holes themselves are invisible, astronomers can detect them through their interaction with nearby matter and the strong gravitational lensing they produce.
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This document provides information about black holes, including their structure, theories about their formation and properties, and how they are detected. It discusses that a black hole has a singularity at its center with infinite density, is surrounded by an event horizon beyond which nothing can escape, and may be accompanied by an accretion disk and jets. It also describes Sagittarius A*, the supermassive black hole at the center of the Milky Way, and Cygnus X-1, the first identified black hole.
Black hole
1) A black hole is a region of spacetime where the gravitational pull is so strong that nothing, not even light, can escape.
2) The boundary of this region is called the event horizon. Although nothing can escape the event horizon, it appears to have no detectable features from within.
3) Black holes form when very massive stars collapse at the end of their life cycle. They can continue growing by absorbing mass and merging with other black holes, potentially forming supermassive black holes containing millions of solar masses.
Black holes
Black holes are regions of extremely strong gravity from which nothing, not even light, can escape. They form from the collapse of massive stars and come in several types depending on properties like charge and rotation. Black holes distort both space and time near them, slowing the flow of time for outside observers and bending light in a process called gravitational lensing. They also emit Hawking radiation and obey laws analogous to thermodynamics. Gravitational waves produced by black holes can help detect their presence.
Black hole
1) A black hole is an object with such strong gravity that not even light can escape, forming at the collapse of a massive star.
2) It has an "event horizon", the point of no return beyond which nothing, not even light, can escape the black hole.
3) Black holes were first theorized by geologist John Michell in 1783, and the modern theory was proposed by physicist Stephen Hawking.
Shadow of rotating Hayward blackhole bounded by Perfect Fluid Dark Matter
I do not have any questions. The document appears to be a research proposal on various topics related to black holes, including their formation, properties of rotating and charged black holes, geodesic motion, dark matter, Hawking radiation, and the shadow they cast.
black hole.pptx
black hole ,types of black hole, size,relativity theory of einstein, components of black hole. how somethings convert into black hole
Black Holes [Krunal Saija]
Detail about Black holes. It's definition, components and then history of black hole and General theory of relativity.
Life cycle of a star and formation of black hole in space.
Different types of choice after star's life end.
Different types of Black hole on basis on mass of Parent star. and classification of black holes on basis of charge and rotational motion of black holes. Quantum theory of physics.
Study of Black holes using Quantum mechanics by Steaphen Hawking.
Current research on black holes.
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It is said that fact is sometimes stranger than fiction, and nowhere is this more true than in the case of black holes. Black holes are stranger than anything dreamt up by science fiction writers, but they are firmly matters of science ~fact.
Dark matter ~ Introduction
How the concept was introduced by the astrophycists and examples that provide the base for the existence of dark matter. Basic introduction to types of dark matter according to standard cosmological theory.
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Presentation regarding some unknown facts about Black hole.
This project was given to me during my Engineering period.
Thanks for being here 🙂
A REVIEW ARTICLE ON BLACK HOLE A MYSTERY IN THE UNIVERSE
This article reviews black holes, mysterious celestial objects with gravitational pulls so strong that not even light can escape. It discusses the historical background of black hole theory, defines what a black hole is, describes different types including stellar, supermassive, and microscopic black holes. The formation of black holes from collapsing stars is explained. While black holes pose no threat to life on Earth, objects close to a black hole's event horizon would be stretched out in a process called spaghettification. Though black holes themselves are invisible, astronomers can detect them through gravitational effects on nearby objects and energetic x-ray emissions from accretion disks.
What is a black hole
Black holes are regions of space where gravity is so strong that not even light can escape. They form when very massive stars collapse at the end of their life cycles. While black holes cannot be seen directly, astronomers can detect them by observing their effects on nearby objects like stars and gas, and through detection of x-rays emitted during accretion. Black holes come in different sizes, from stellar-mass black holes up to supermassive black holes that may exist at the centers of galaxies.
Black holes Samriddha Shil.....S@S
The document discusses black holes and their theoretical definition. It explains that black holes are areas of space-time with gravitational fields so strong that their escape velocity exceeds the speed of light. Black holes are theorized to form when very massive stars undergo supernovas and collapse inward. The document also discusses different types of black holes like stellar-mass, mid-mass, and supermassive black holes found at the centers of galaxies.
What are dead stars good for?
A lesson I gave to high school students during my time at Yale, with the Yale SPLASH student organisation.
Particle Properties of Waves
This document discusses the development of quantum mechanics. It summarizes that classical physics could not explain certain experimental observations, leading to quantum theory. Key events were Planck's blackbody radiation law, Einstein's explanation of the photoelectric effect using light quanta (photons), and Compton's discovery that photons transfer momentum to electrons. The photoelectric effect showed that light behaves as particles (photons), while the de Broglie hypothesis and Davisson-Germer experiment showed that electrons can behave as waves. This established the wave-particle duality of both light and matter.
BLACK HOLE-THE OTHER DIMENSION
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Black hole – A region in the space where the gravitational pull is so strong that neither substance nor light can leave this area.
period 7 Sheharyar Sohail Black Holes
Black holes are regions of space where the gravitational pull is so strong that nothing, not even light, can escape. Surrounding the black hole is an event horizon, which marks the point of no return beyond which the gravitational forces are inescapable. Albert Einstein's theory of general relativity first theorized black holes by explaining how gravity can bend space and time. Black holes have immense gravitational forces that can feed on and destroy stars that come too close, collapsing them into the black hole. The largest known black holes are supermassive black holes that can be millions of times the size of our sun.
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一比一原版(dmu毕业证书)英国德蒙福特大学毕业证如何办理
原版一模一样【微信：741003700 】【(dmu毕业证书)英国德蒙福特大学毕业证成绩单】【微信：741003700 】学位证，留信认证（真实可查，永久存档）原件一模一样纸张工艺/offer、雅思、外壳等材料/诚信可靠,可直接看成品样本，帮您解决无法毕业带来的各种难题！外壳，原版制作，诚信可靠，可直接看成品样本。行业标杆！精益求精，诚心合作，真诚制作！多年品质 ,按需精细制作，24小时接单,全套进口原装设备。十五年致力于帮助留学生解决难题，包您满意。
本公司拥有海外各大学样板无数，能完美还原。
1:1完美还原海外各大学毕业材料上的工艺：水印，阴影底纹，钢印LOGO烫金烫银，LOGO烫金烫银复合重叠。文字图案浮雕、激光镭射、紫外荧光、温感、复印防伪等防伪工艺。材料咨询办理、认证咨询办理请加学历顾问Q/微741003700
【主营项目】
一.毕业证【q微741003700】成绩单、使馆认证、教育部认证、雅思托福成绩单、学生卡等！
二.真实使馆公证(即留学回国人员证明,不成功不收费)
三.真实教育部学历学位认证（教育部存档！教育部留服网站永久可查）
四.办理各国各大学文凭(一对一专业服务,可全程监控跟踪进度)
如果您处于以下几种情况：
◇在校期间，因各种原因未能顺利毕业……拿不到官方毕业证【q/微741003700】
◇面对父母的压力，希望尽快拿到；
◇不清楚认证流程以及材料该如何准备；
◇回国时间很长，忘记办理；
◇回国马上就要找工作，办给用人单位看；
◇企事业单位必须要求办理的
◇需要报考公务员、购买免税车、落转户口
◇申请留学生创业基金
留信网认证的作用:
1:该专业认证可证明留学生真实身份
2:同时对留学生所学专业登记给予评定
3:国家专业人才认证中心颁发入库证书
4:这个认证书并且可以归档倒地方
5:凡事获得留信网入网的信息将会逐步更新到个人身份内，将在公安局网内查询个人身份证信息后，同步读取人才网入库信息
6:个人职称评审加20分
7:个人信誉贷款加10分
8:在国家人才网主办的国家网络招聘大会中纳入资料，供国家高端企业选择人才
办理(dmu毕业证书)英国德蒙福特大学毕业证【微信：741003700 】外观非常简单，由纸质材料制成，上面印有校徽、校名、毕业生姓名、专业等信息。
办理(dmu毕业证书)英国德蒙福特大学毕业证【微信：741003700 】格式相对统一，各专业都有相应的模板。通常包括以下部分：
校徽：象征着学校的荣誉和传承。
校名:学校英文全称
授予学位：本部分将注明获得的具体学位名称。
毕业生姓名：这是最重要的信息之一，标志着该证书是由特定人员获得的。
颁发日期：这是毕业正式生效的时间，也代表着毕业生学业的结束。
其他信息：根据不同的专业和学位，可能会有一些特定的信息或章节。
办理(dmu毕业证书)英国德蒙福特大学毕业证【微信：741003700 】价值很高，需要妥善保管。一般来说，应放置在安全、干燥、防潮的地方，避免长时间暴露在阳光下。如需使用，最好使用复印件而不是原件，以免丢失。
综上所述，办理(dmu毕业证书)英国德蒙福特大学毕业证【微信：741003700 】是证明身份和学历的高价值文件。外观简单庄重，格式统一，包括重要的个人信息和发布日期。对持有人来说，妥善保管是非常重要的。
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【网址🎉ac99.net🎉】欧洲杯外围是爱尔兰的博彩公司，成立于1988年，位于爱尔兰的都柏林。欧洲杯外围通过在爱尔兰和英国的一系列持牌博彩商店以及经营爱尔兰最大的电话博彩服务来开展业务。在互联网上，欧洲杯外围提供体育博彩，在线扑克，在线宾果游戏，在线赌场和在线游戏。
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【网址🎉ac10.net🎉】欧洲杯买球是一家极具特色的欧洲主流博彩公司，对于自己所擅长的赛事往往把赔率值压得很低，掩饰平局是他们一贯的手法。例如，当伟德旗帜鲜明地支持客胜，降低客胜值，提升主胜值，而平局赔率却与欧洲杯买球、欧洲杯买球的态度较吻合时，这场比赛往往以平局收场。
一比一原版美国西北大学毕业证(NWU毕业证书)学历如何办理
原版办理【微信号:BYZS866】【美国西北大学毕业证(NWU毕业证书)】【微信号:BYZS866】《成绩单、外壳、雅思、offer、真实留信官方学历认证（永久存档/真实可查）》采用学校原版纸张、特殊工艺完全按照原版一比一制作（包括：隐形水印，阴影底纹，钢印LOGO烫金烫银，LOGO烫金烫银复合重叠，文字图案浮雕，激光镭射，紫外荧光，温感，复印防伪）行业标杆！精益求精，诚心合作，真诚制作！多年品质 ,按需精细制作，24小时接单,全套进口原装设备，十五年致力于帮助留学生解决难题，业务范围有加拿大、英国、澳洲、韩国、美国、新加坡，新西兰等学历材料，包您满意。
【我们承诺采用的是学校原版纸张（纸质、底色、纹路）我们拥有全套进口原装设备，特殊工艺都是采用不同机器制作，仿真度基本可以达到100%，所有工艺效果都可提前给客户展示，不满意可以根据客户要求进行调整，直到满意为止！】
【业务选择办理准则】
一、工作未确定，回国需先给父母、亲戚朋友看下文凭的情况，办理一份就读学校的毕业证【微信号BYZS866】文凭即可
二、回国进私企、外企、自己做生意的情况，这些单位是不查询毕业证真伪的，而且国内没有渠道去查询国外文凭的真假，也不需要提供真实教育部认证。鉴于此，办理一份毕业证【微信号BYZS866】即可
三、进国企，银行，事业单位，考公务员等等，这些单位是必需要提供真实教育部认证的，办理教育部认证所需资料众多且烦琐，所有材料您都必须提供原件，我们凭借丰富的经验，快捷的绿色通道帮您快速整合材料，让您少走弯路。
留信网认证的作用:
1:该专业认证可证明留学生真实身份
2:同时对留学生所学专业登记给予评定
3:国家专业人才认证中心颁发入库证书
4:这个认证书并且可以归档倒地方
5:凡事获得留信网入网的信息将会逐步更新到个人身份内，将在公安局网内查询个人身份证信息后，同步读取人才网入库信息
6:个人职称评审加20分
7:个人信誉贷款加10分
8:在国家人才网主办的国家网络招聘大会中纳入资料，供国家高端企业选择人才
留信网服务项目：
1、留学生专业人才库服务（留信分析）
2、国（境）学习人员提供就业推荐信服务
3、留学人员区块链存储服务
【关于价格问题（保证一手价格）】
我们所定的价格是非常合理的，而且我们现在做得单子大多数都是代理和回头客户介绍的所以一般现在有新的单子 我给客户的都是第一手的代理价格，因为我想坦诚对待大家 不想跟大家在价格方面浪费时间
对于老客户或者被老客户介绍过来的朋友，我们都会适当给一些优惠。
选择实体注册公司办理，更放心，更安全！我们的承诺：客户在留信官方认证查询网站查询到认证通过结果后付款，不成功不收费！
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I am an accomplished and driven administrative management professional with a proven track record of supporting senior executives and managing administrative teams. I am skilled in strategic planning, project management, and organizational development, and have extensive experience in improving processes, enhancing productivity, and implementing solutions to support business objectives and growth.
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在线办理(UOIT毕业证书)安大略省理工大学毕业证在读证明一模一样
原件一模一样【微信：bwp0011】《(UOIT毕业证书)安大略省理工大学毕业证》【微信：bwp0011】学位证，留信认证（真实可查，永久存档）原件一模一样纸张工艺/offer、雅思、外壳等材料/诚信可靠,可直接看成品样本，帮您解决无法毕业带来的各种难题！外壳，原版制作，诚信可靠，可直接看成品样本。行业标杆！精益求精，诚心合作，真诚制作！多年品质 ,按需精细制作，24小时接单,全套进口原装设备。十五年致力于帮助留学生解决难题，包您满意。
本公司拥有海外各大学样板无数，能完美还原。
1:1完美还原海外各大学毕业材料上的工艺：水印，阴影底纹，钢印LOGO烫金烫银，LOGO烫金烫银复合重叠。文字图案浮雕、激光镭射、紫外荧光、温感、复印防伪等防伪工艺。材料咨询办理、认证咨询办理请加学历顾问微bwp0011
【主营项目】
一.毕业证【微bwp0011】成绩单、使馆认证、教育部认证、雅思托福成绩单、学生卡等！
二.真实使馆公证(即留学回国人员证明,不成功不收费)
三.真实教育部学历学位认证（教育部存档！教育部留服网站永久可查）
四.办理各国各大学文凭(一对一专业服务,可全程监控跟踪进度)
如果您处于以下几种情况：
◇在校期间，因各种原因未能顺利毕业……拿不到官方毕业证【微bwp0011】
◇面对父母的压力，希望尽快拿到；
◇不清楚认证流程以及材料该如何准备；
◇回国时间很长，忘记办理；
◇回国马上就要找工作，办给用人单位看；
◇企事业单位必须要求办理的
◇需要报考公务员、购买免税车、落转户口
◇申请留学生创业基金
留信网认证的作用:
1:该专业认证可证明留学生真实身份
2:同时对留学生所学专业登记给予评定
3:国家专业人才认证中心颁发入库证书
4:这个认证书并且可以归档倒地方
5:凡事获得留信网入网的信息将会逐步更新到个人身份内，将在公安局网内查询个人身份证信息后，同步读取人才网入库信息
6:个人职称评审加20分
7:个人信誉贷款加10分
8:在国家人才网主办的国家网络招聘大会中纳入资料，供国家高端企业选择人才
一比一原版(EUR毕业证)鹿特丹伊拉斯姆斯大学毕业证如何办理
原件一模一样【微信：95270640】【鹿特丹伊拉斯姆斯大学毕业证EUR学位证成绩单】【微信：95270640】（留信学历认证永久存档查询）采用学校原版纸张、特殊工艺完全按照原版一比一制作（包括：隐形水印，阴影底纹，钢印LOGO烫金烫银，LOGO烫金烫银复合重叠，文字图案浮雕，激光镭射，紫外荧光，温感，复印防伪）行业标杆！精益求精，诚心合作，真诚制作！多年品质 ,按需精细制作，24小时接单,全套进口原装设备，十五年致力于帮助留学生解决难题，业务范围有加拿大、英国、澳洲、韩国、美国、新加坡，新西兰等学历材料，包您满意。
【业务选择办理准则】
一、工作未确定，回国需先给父母、亲戚朋友看下文凭的情况，办理一份就读学校的毕业证【微信：95270640】文凭即可
二、回国进私企、外企、自己做生意的情况，这些单位是不查询毕业证真伪的，而且国内没有渠道去查询国外文凭的真假，也不需要提供真实教育部认证。鉴于此，办理一份毕业证【微信：95270640】即可
三、进国企，银行，事业单位，考公务员等等，这些单位是必需要提供真实教育部认证的，办理教育部认证所需资料众多且烦琐，所有材料您都必须提供原件，我们凭借丰富的经验，快捷的绿色通道帮您快速整合材料，让您少走弯路。
留信网认证的作用:
1:该专业认证可证明留学生真实身份【微信：95270640】
2:同时对留学生所学专业登记给予评定
3:国家专业人才认证中心颁发入库证书
4:这个认证书并且可以归档倒地方
5:凡事获得留信网入网的信息将会逐步更新到个人身份内，将在公安局网内查询个人身份证信息后，同步读取人才网入库信息
6:个人职称评审加20分
7:个人信誉贷款加10分
8:在国家人才网主办的国家网络招聘大会中纳入资料，供国家高端企业选择人才
→ 【关于价格问题（保证一手价格）
我们所定的价格是非常合理的，而且我们现在做得单子大多数都是代理和回头客户介绍的所以一般现在有新的单子 我给客户的都是第一手的代理价格，因为我想坦诚对待大家 不想跟大家在价格方面浪费时间
对于老客户或者被老客户介绍过来的朋友，我们都会适当给一些优惠。
选择实体注册公司办理，更放心，更安全！我们的承诺：可来公司面谈，可签订合同，会陪同客户一起到教育部认证窗口递交认证材料，客户在教育部官方认证查询网站查询到认证通过结果后付款，不成功不收费！
办理鹿特丹伊拉斯姆斯大学毕业证毕业证offerEUR学位证【微信：95270640 】外观非常精致，由特殊纸质材料制成，上面印有校徽、校名、毕业生姓名、专业等信息。
办理鹿特丹伊拉斯姆斯大学毕业证EUR学位证毕业证offer【微信：95270640 】格式相对统一，各专业都有相应的模板。通常包括以下部分：
校徽：象征着学校的荣誉和传承。
校名:学校英文全称
授予学位：本部分将注明获得的具体学位名称。
毕业生姓名：这是最重要的信息之一，标志着该证书是由特定人员获得的。
颁发日期：这是毕业正式生效的时间，也代表着毕业生学业的结束。
其他信息：根据不同的专业和学位，可能会有一些特定的信息或章节。
办理鹿特丹伊拉斯姆斯大学毕业证毕业证offerEUR学位证【微信：95270640 】价值很高，需要妥善保管。一般来说，应放置在安全、干燥、防潮的地方，避免长时间暴露在阳光下。如需使用，最好使用复印件而不是原件，以免丢失。
综上所述，办理鹿特丹伊拉斯姆斯大学毕业证毕业证offerEUR学位证【微信：95270640 】是证明身份和学历的高价值文件。外观简单庄重，格式统一，包括重要的个人信息和发布日期。对持有人来说，妥善保管是非常重要的。
一比一原版坎特伯雷大学毕业证(UC毕业证书)学历如何办理
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【业务选择办理准则】
一、工作未确定，回国需先给父母、亲戚朋友看下文凭的情况，办理一份就读学校的毕业证【微信：176555708】文凭即可
二、回国进私企、外企、自己做生意的情况，这些单位是不查询毕业证真伪的，而且国内没有渠道去查询国外文凭的真假，也不需要提供真实教育部认证。鉴于此，办理一份毕业证【微信：176555708】即可
三、进国企，银行，事业单位，考公务员等等，这些单位是必需要提供真实教育部认证的，办理教育部认证所需资料众多且烦琐，所有材料您都必须提供原件，我们凭借丰富的经验，快捷的绿色通道帮您快速整合材料，让您少走弯路。
留信网认证的作用:
1:该专业认证可证明留学生真实身份【微信：176555708】
2:同时对留学生所学专业登记给予评定
3:国家专业人才认证中心颁发入库证书
4:这个认证书并且可以归档倒地方
5:凡事获得留信网入网的信息将会逐步更新到个人身份内，将在公安局网内查询个人身份证信息后，同步读取人才网入库信息
6:个人职称评审加20分
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→ 【关于价格问题（保证一手价格）
我们所定的价格是非常合理的，而且我们现在做得单子大多数都是代理和回头客户介绍的所以一般现在有新的单子 我给客户的都是第一手的代理价格，因为我想坦诚对待大家 不想跟大家在价格方面浪费时间
对于老客户或者被老客户介绍过来的朋友，我们都会适当给一些优惠。
选择实体注册公司办理，更放心，更安全！我们的承诺：可来公司面谈，可签订合同，会陪同客户一起到教育部认证窗口递交认证材料，客户在教育部官方认证查询网站查询到认证通过结果后付款，不成功不收费！
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校名:学校英文全称
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毕业生姓名：这是最重要的信息之一，标志着该证书是由特定人员获得的。
颁发日期：这是毕业正式生效的时间，也代表着毕业生学业的结束。
其他信息：根据不同的专业和学位，可能会有一些特定的信息或章节。
办理西蒙菲莎大学毕业证（SFU学位证）学位证【微信：176555708 】价值很高，需要妥善保管。一般来说，应放置在安全、干燥、防潮的地方，避免长时间暴露在阳光下。如需使用，最好使用复印件而不是原件，以免丢失。
综上所述，办理西蒙菲莎大学毕业证（SFU学位证）学位证【微信：176555708 】是证明身份和学历的高价值文件。外观简单庄重，格式统一，包括重要的个人信息和发布日期。对持有人来说，妥善保管是非常重要的。
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一比一原版(kcl毕业证书)英国金斯顿大学毕业证如何办理
原版一模一样【微信：741003700 】【(kcl毕业证书)英国金斯顿大学毕业证成绩单】【微信：741003700 】学位证，留信认证（真实可查，永久存档）原件一模一样纸张工艺/offer、雅思、外壳等材料/诚信可靠,可直接看成品样本，帮您解决无法毕业带来的各种难题！外壳，原版制作，诚信可靠，可直接看成品样本。行业标杆！精益求精，诚心合作，真诚制作！多年品质 ,按需精细制作，24小时接单,全套进口原装设备。十五年致力于帮助留学生解决难题，包您满意。
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2:同时对留学生所学专业登记给予评定
3:国家专业人才认证中心颁发入库证书
4:这个认证书并且可以归档倒地方
5:凡事获得留信网入网的信息将会逐步更新到个人身份内，将在公安局网内查询个人身份证信息后，同步读取人才网入库信息
6:个人职称评审加20分
7:个人信誉贷款加10分
8:在国家人才网主办的国家网络招聘大会中纳入资料，供国家高端企业选择人才
办理(kcl毕业证书)英国金斯顿大学毕业证【微信：741003700 】外观非常简单，由纸质材料制成，上面印有校徽、校名、毕业生姓名、专业等信息。
办理(kcl毕业证书)英国金斯顿大学毕业证【微信：741003700 】格式相对统一，各专业都有相应的模板。通常包括以下部分：
校徽：象征着学校的荣誉和传承。
校名:学校英文全称
授予学位：本部分将注明获得的具体学位名称。
毕业生姓名：这是最重要的信息之一，标志着该证书是由特定人员获得的。
颁发日期：这是毕业正式生效的时间，也代表着毕业生学业的结束。
其他信息：根据不同的专业和学位，可能会有一些特定的信息或章节。
办理(kcl毕业证书)英国金斯顿大学毕业证【微信：741003700 】价值很高，需要妥善保管。一般来说，应放置在安全、干燥、防潮的地方，避免长时间暴露在阳光下。如需使用，最好使用复印件而不是原件，以免丢失。
综上所述，办理(kcl毕业证书)英国金斯顿大学毕业证【微信：741003700 】是证明身份和学历的高价值文件。外观简单庄重，格式统一，包括重要的个人信息和发布日期。对持有人来说，妥善保管是非常重要的。
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留信网认证的作用:
1:该专业认证可证明留学生真实身份
2:同时对留学生所学专业登记给予评定
3:国家专业人才认证中心颁发入库证书
4:这个认证书并且可以归档倒地方
5:凡事获得留信网入网的信息将会逐步更新到个人身份内，将在公安局网内查询个人身份证信息后，同步读取人才网入库信息
6:个人职称评审加20分
7:个人信誉贷款加10分
8:在国家人才网主办的国家网络招聘大会中纳入资料，供国家高端企业选择人才
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STEPHEN HAWKING AUTOBIOGRAPHY
- 1. Seminar on Black hole Presented by Name- Bibek Mishra Admission no- 201721219 Calss-sem1 Msc physics Guided by Dr vinod kumar Sayal Professor and HOD
- 2. Black Holes A black hole is a region of space time exhibiting such strong gravitational effects that nothing including particles and electromagnetic radiation such as light can escape from inside. Types: • Primordial(smallest) • Steller(medium) • Supermassive(largest)
- 3. Gravity bends the path of light
- 5. A nonrotating black hole has only a “center” and a “surface” The black hole is surrounded by an event horizon which is the sphere from which light cannot escape The distance between the black hole and its event horizon is the Schwarzschild radius (RSch= 2GM/c2) The center of the black hole is a point of infinite density and zero volume, called a singularity
- 7. Mass Total electric charge Spin = angular momentum Three parameters completely describe the structure of a black hole Most properties of matter vanish when matter enters a black hole, such as chemical composition, texture, color, shape, size, distinctions between protons and electrons, etc
- 8. As you fall into to a black hole, you shine a blue flashlight at a friend exterior to the hole, she sees 1. blue light 2. blue light at first, then turning red 3. blue light, then red, then nothing 4. nothing
- 10. An accretion disk is a structure formed by diffused material in orbital motion around a black hole.
- 12. Gravitational energy Black holes generate energy from matter falling into them.
- 14. Eddington Luminosit y Limit on the brightness of a black hole
- 16. Electromagnetic spectrum Black holes are so hot that they mainly produce X-rays
- 17. THANK YOU