• Study Resource
  • Explore Categories
    • Arts & Humanities
    • Business
    • Engineering & Technology
    • Foreign Language
    • History
    • Math
    • Science
    • Social Science

    Top subcategories

    • Advanced Math
    • Algebra
    • Basic Math
    • Calculus
    • Geometry
    • Linear Algebra
    • Pre-Algebra
    • Pre-Calculus
    • Statistics And Probability
    • Trigonometry
    • other →

    Top subcategories

    • Astronomy
    • Astrophysics
    • Biology
    • Chemistry
    • Earth Science
    • Environmental Science
    • Health Science
    • Physics
    • other →

    Top subcategories

    • Anthropology
    • Law
    • Political Science
    • Psychology
    • Sociology
    • other →

    Top subcategories

    • Accounting
    • Economics
    • Finance
    • Management
    • other →

    Top subcategories

    • Aerospace Engineering
    • Bioengineering
    • Chemical Engineering
    • Civil Engineering
    • Computer Science
    • Electrical Engineering
    • Industrial Engineering
    • Mechanical Engineering
    • Web Design
    • other →

    Top subcategories

    • Architecture
    • Communications
    • English
    • Gender Studies
    • Music
    • Performing Arts
    • Philosophy
    • Religious Studies
    • Writing
    • other →

    Top subcategories

    • Ancient History
    • European History
    • US History
    • World History
    • other →

    Top subcategories

    • Croatian
    • Czech
    • Finnish
    • Greek
    • Hindi
    • Japanese
    • Korean
    • Persian
    • Swedish
    • Turkish
    • other →
 
Profile Documents Logout
Upload
An evolutionary channel towards the accreting millisecond pulsar
An evolutionary channel towards the accreting millisecond pulsar

... In the MESA code, we consider three types of orbital-angularmomentum loss during the evolution of LMXBs: (1) gravitationalwave radiation; (2) magnetic braking: we adopt the standard magnetic braking prescription given by Rappaport, Verbunt & Joss (1983), and take γ = 4; (3) mass-loss: the mass-loss ...
OpenStax Physics Text for 2B - Chapter 7
OpenStax Physics Text for 2B - Chapter 7

... 1. Electric field lines originate on positive charges and terminate on negative charges. The electric field is defined as the force per unit charge on a test charge, and the strength of the force is related to the electric constant ε 0 , also known as the permittivity of free space. From Maxwell’s f ...
Circumstellar grains: radiation pressure and
Circumstellar grains: radiation pressure and

... the course of previous works on interplanetary grains (Lamy, 1974; Burns et al., 1979), we have noticed that it was important to introduce, not only the actual optical properties of the materials, but also the actual spectral flux of the source. In the present study, measured spectrophotometric data ...
New features of ion acoustic waves in inhomogeneous and
New features of ion acoustic waves in inhomogeneous and

... In the present work we shall show that the ion acoustic waves may be produced on massive scales directly in the upper solar atmosphere. Their energy may further be transformed into internal energy of the plasma by at least two different mechanisms which will be discussed. We shall describe two very ...
30155-doc - Project Gutenberg
30155-doc - Project Gutenberg

Microscopic analysis of rotating Black Holes
Microscopic analysis of rotating Black Holes

... 4.1.2 Microscopic derivation of the superradiant frequency bound 4.1.3 Four-dimensional black holes . . . . . . . . . . . . . . . . . 4.1.4 Other systems with ergoregion . . . . . . . . . . . . . . . . 4.1.5 No superradiant emission of linear momentum . . . . . . . 4.1.6 Superradiant amplification, ...
biennial 2004_05_engl_FINAL.indd - Albert Einstein Institute
biennial 2004_05_engl_FINAL.indd - Albert Einstein Institute

electromagnetic waves
electromagnetic waves

... (a) the same direction but differ in phase by 900 (b) the same direction and are in phase (c) mutually perpendicular directions and are in phase (d) mutually perpendicular directions and differ in phase by 900 ...
Part-VI
Part-VI

Waves 2006 11 04
Waves 2006 11 04

24 electromagnetic waves - Wright State University
24 electromagnetic waves - Wright State University

... Electromagnetic waves carry energy away from their source, similar to a sound wave carrying energy away from a standing wave on a guitar string. An antenna for receiving EM signals works in reverse. And like antennas that produce EM waves, receiver antennas are specially designed to resonate at part ...
The role of black holes in galaxy formation and evolution
The role of black holes in galaxy formation and evolution

... winds in two ways. They can heat the gas and cause it to expand (thermal “energy-driven” winds) or they can push it out (pressure “momentum-driven” winds). Photons heat the gas by photoionising metals such as iron, which retain their inner electrons even at high temperature, and by Compton scatteri ...
universal gravitation - Youngbull Science Center
universal gravitation - Youngbull Science Center

... Newton’s Hypothesis Newton compared the motion of the moon to a cannonball fired from the top of a high mountain. If the mountaintop was above Earth’s atmosphere, air resistance would not impede the motion of the cannonball. If a cannonball were fired with a small horizontal speed, it would follow a ...
BBO
BBO

Extragalactic Background Light Encyclopedia of Astronomy & Astrophysics eaa.iop.org Rebecca A Bernstein
Extragalactic Background Light Encyclopedia of Astronomy & Astrophysics eaa.iop.org Rebecca A Bernstein

ray emission from the distant BL Lac PG 1553+113
ray emission from the distant BL Lac PG 1553+113

... distribution (SED), PG 1553+113 is now classified as a highfrequency peaked BL Lac (Giommi et al. 1995), similar to essentially all of the AGN detected at VHE (very high energy; >100 GeV) energies. ...
Abundance Anomalies In Tidal Disruption Events
Abundance Anomalies In Tidal Disruption Events

... burning, the anomalies outside the helium core begin to drop again. However, first dredge up also mixes them into the outer parts of the star beyond the shell. Figure 2 extends a little past the horizontal branch, where we first see a rapid increase in helium followed by a rapid increase in carbon. ...
A dearth of dark matter in strong gravitational lenses
A dearth of dark matter in strong gravitational lenses

... In other words, it appears that the dynamics of the outer ‘haloes’, more than 100 kpc in extent, is determined by the small fraction of baryons in the very centre, a very strange fact indeed when viewed in the context of dark matter. On the other hand, there are persistent claims that strong gravita ...
Searching for and Identifying Pulsars
Searching for and Identifying Pulsars

... some very interesting phenomena1 . The most important of these phenomena for us is that radiation is beamed from the magnetic poles of the pulsar. Let’s take a moment to discuss this more fully. If you have ever played with a bar magnet before, you know that magnets have a north and south pole. This ...
The Mock LISA Data Challenges: from Challenge 1B to
The Mock LISA Data Challenges: from Challenge 1B to

... of a number of new groups that successfully recovered signals from galactic binaries and MBH binaries, and the first convincing demonstration of EMRI detection and parameter estimation. Section 2 provides a brief summary of the entries; additional details about the work of individual collaborations ...
Thermal Noise Issue in the monolithic suspensions of the Virgo+
Thermal Noise Issue in the monolithic suspensions of the Virgo+

MS-SCI-PS-Unit 4 -- Chapter 15- Stars, Galaxies
MS-SCI-PS-Unit 4 -- Chapter 15- Stars, Galaxies

... light in the night sky. But they could see few details with their eyes alone. It was not until the invention of the telescope in 1608 that people could observe objects in the sky more closely. Recall that a telescope is a device that makes distant objects appear to be closer. The telescope revolutio ...
PhYSiCS
PhYSiCS

... National Institute of Education ...
Chapter 21: Waves in Cold Plasmas: Two-Fluid Formalism
Chapter 21: Waves in Cold Plasmas: Two-Fluid Formalism

... separately as fluids, upon which act electromagnetic forces. This is called the two-fluid formalism for plasmas. In the next chapter, we shall show when and how waves are sensitive to the actual distribution of particle speeds by developing the more sophisticated kinetic-theory formalism and using i ...
Star Formation in Isolated Disk Galaxies. I. Models and
Star Formation in Isolated Disk Galaxies. I. Models and

... positions as we vary the number of the processors. The unmodified GADGET v1.1 also shows such small deviations as processor number is changed. These variations are due to the differences in the extent of the domain on each processor. When the force on a particular particle is computed, the force exe ...
< 1 ... 16 17 18 19 20 21 22 23 24 ... 136 >

First observation of gravitational waves

  • studyres.com © 2026
  • DMCA
  • Privacy
  • Terms
  • Report