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The gravitational interaction of light: from weak to strong fields
The gravitational interaction of light: from weak to strong fields

... equations representing pure gravitational waves, or the gravitational field of electromagnetic pulses or beams. For these metrics, the Einstein field equations exhibit a linearity property that allows one to superpose two pp–waves propagating parallely without apparent interaction, and obtain anothe ...
Recitation 3
Recitation 3

... so y must also rotate around the reference circle at 600 Hz. Problem 14.6. Two identical sinusoidal waves with wavelengths of 3.00 m travel in the same direction at a speed of 2.00 m/s. The second wave originates from the same point as the first, but at a later time. The amplitude of the resultant w ...
MULTIPLE CHOICE FINAL REVIEW Multiple Choice Protons and
MULTIPLE CHOICE FINAL REVIEW Multiple Choice Protons and

... 75. A mirror that curves away from you is a __________________________ mirror. It can form both ________________ and _________________ images. 76. Electric power is found by multiplying __________ by current. 77. Electric power is the rate of __________ transferred over time. 78. A short piece of wi ...
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Micro_lect20

Properties of long gamma-ray bursts from massive compact binaries
Properties of long gamma-ray bursts from massive compact binaries

... flaring activity, with the flare peaking between 104 and 105 s, the peak time being correlated with the flare energy. We show that these times are set by the semi-major axis of the binary, and hence the process of tidal spin-up; furthermore, they are consistent with flares seen in the X-ray light cu ...
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Answers

The Life Cycle of Spiral Arm Galaxies
The Life Cycle of Spiral Arm Galaxies

... As  a  star  goes  supernova,  it  releases  a  great  amount  of  energy  (light)  and  also  ejects  a   massive  amount  of  matter  (galactic  cosmic  rays),  which  are  charged  particles  such  as   protons  and  pieces  of   ...
Microlensing experiments Several experiments have searched for
Microlensing experiments Several experiments have searched for

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Topic 6 Introduction

... •  We talk of supernovae (SN) in this course on Nuclear Astrophysics because SN are responsible for dispersing pre-processed elements into the interstellar medium for further processing during (new) star formation •  SN are the death throes of massive stars –  Typical kinetic energy release: 1044 J ...
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Physics p1 revision 2017 PPTX

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SupernovaExplosionPhysics_8pages

... General Relativity • large angular velocity • large magnetic fields On the note of strong gravity, we finish by mentioning the Schwarzschild radius, Rs , predicted by GR as the “event horizon” where proper time intervals go to zero and light cannot escape. It is given by Rs = 2GM/c2 . For M = 5M! , ...
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Kein Folientitel

Wave particle-interactions
Wave particle-interactions

... aspects of microscopic plasma theory. The moments like density, flow speed, temperature are of macroscopic nature, and their gradients induce corresponding flows in the plasma related with diffusion, viscosity, or heat conduction, which will cause irreversibility in the system. In a collisionless pl ...
Ch. 24 Electromagnetic Waves
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... A vertical slit would allow the wave to p pass through, g , since the slit is parallel to the oscillations: Direction of electric field ...
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chapter18StarDeath

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Chapter 18 The Bizarre Stellar Graveyard What is a white dwarf

... • Observations show that at least some gamma-ray bursts are produced by supernova explosions • Some others may come from collisions between neutron stars ...
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... By stepping up the voltage ( using the step up transformer) the current goes down. Low current means the wires don’t get hot so less energy is wasted .The voltage is then stepped down ( by the step down transformer ) to houses so its safer. The transformers make the system more efficient. ...
Linking Asteroids and Meteorites through Reflectance Spectroscopy
Linking Asteroids and Meteorites through Reflectance Spectroscopy

... of energy since the rest of the star collapses and then bounces off the neutron core • 1044-46 Joules • Annual energy generation of Sun is 1034 Joules ...
Astronomy Talk July 2016 - Unitarian Universalist Church of
Astronomy Talk July 2016 - Unitarian Universalist Church of

... Maybe they don’t want us to know they’re out there. If they are picking up our radio and TV news programs, maybe they’ve had ...
Gravity - South High School
Gravity - South High School

... we will be looking at today. Which one would be considered the independent variable and which would be the dependent variable? ...
Lecture 16: Iron Core Collapse, Neutron Stars, and Nucleosynthesis
Lecture 16: Iron Core Collapse, Neutron Stars, and Nucleosynthesis

... One of the most challenging computer problems in the world ...
Lecture 14
Lecture 14

... spheres are called Stromgren spheres. At the outer boundary, there is some recombination. With the short lifetime of massive, UV-creating stars, the size of Stromgren spheres often reaches a ...
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Black Holes - Wayne State University Physics and Astronomy
Black Holes - Wayne State University Physics and Astronomy

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First observation of gravitational waves

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