Redshift and Energy Conservation Alasdair Macleod§
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Glossary Physics (I-Introduction)
1 Glossary Physics (I-introduction) - Efficiency: The percent of the work put into a machine that is converted into useful work output; = work done / energy used [-]. = eta In machines: The work output of any machine cannot exceed the work input (<=100%); in an ideal machine, where no energy is transformed into heat: work(input) = work(output), =100%. Energy: The property of a system that enables it to do work. Conservation o. E.: Energy cannot be created or destroyed; it may be transformed from one form into another, but the total amount of energy never changes. Equilibrium: The state of an object when not acted upon by a net force or net torque; an object in equilibrium may be at rest or moving at uniform velocity - not accelerating. Mechanical E.: The state of an object or system of objects for which any impressed forces cancels to zero and no acceleration occurs. Dynamic E.: Object is moving without experiencing acceleration. Static E.: Object is at rest.F Force: The influence that can cause an object to be accelerated or retarded; is always in the direction of the net force, hence a vector quantity; the four elementary forces are: Electromagnetic F.: Is an attraction or repulsion G, gravit. const.6.672E-11[Nm2/kg2] between electric charges: d, distance [m] 2 2 2 2 F = 1/(40) (q1q2/d ) [(CC/m )(Nm /C )] = [N] m,M, mass [kg] Gravitational F.: Is a mutual attraction between all masses: q, charge [As] [C] 2 2 2 2 F = GmM/d [Nm /kg kg 1/m ] = [N] 0, dielectric constant Strong F.: (nuclear force) Acts within the nuclei of atoms: 8.854E-12 [C2/Nm2] [F/m] 2 2 2 2 2 F = 1/(40) (e /d ) [(CC/m )(Nm /C )] = [N] , 3.14 [-] Weak F.: Manifests itself in special reactions among elementary e, 1.60210 E-19 [As] [C] particles, such as the reaction that occur in radioactive decay. -
Arxiv:1401.0181V1 [Gr-Qc] 31 Dec 2013 † Isadpyia Infiac Fteenwcodntsaediscussed
Painlev´e-Gullstrand-type coordinates for the five-dimensional Myers-Perry black hole Tehani K. Finch† NASA Goddard Space Flight Center Greenbelt MD 20771 ABSTRACT The Painlev´e-Gullstrand coordinates provide a convenient framework for pre- senting the Schwarzschild geometry because of their flat constant-time hyper- surfaces, and the fact that they are free of coordinate singularities outside r=0. Generalizations of Painlev´e-Gullstrand coordinates suitable for the Kerr geome- try have been presented by Doran and Nat´ario. These coordinate systems feature a time coordinate identical to the proper time of zero-angular-momentum ob- servers that are dropped from infinity. Here, the methods of Doran and Nat´ario arXiv:1401.0181v1 [gr-qc] 31 Dec 2013 are extended to the five-dimensional rotating black hole found by Myers and Perry. The result is a new formulation of the Myers-Perry metric. The proper- ties and physical significance of these new coordinates are discussed. † tehani.k.finch (at) nasa.gov 1 Introduction By using the Birkhoff theorem, the Schwarzschild geometry has been shown to be the unique vacuum spherically symmetric solution of the four-dimensional Einstein equations. The Kerr geometry, on the other hand, has been shown only to be the unique stationary, rotating vacuum black hole solution of the four-dimensional Einstein equations. No distri- bution of matter is currently known to produce a Kerr exterior. Thus the Kerr geometry does not necessarily correspond to the spacetime outside a rotating star or planet [1]. This is an indication of the complications encountered upon trying to extend results found for the Schwarzschild spacetime to the Kerr spacetime. -
M204; the Doppler Effect
MISN-0-204 THE DOPPLER EFFECT by Mary Lu Larsen THE DOPPLER EFFECT Towson State University 1. Introduction a. The E®ect . .1 b. Questions to be Answered . 1 2. The Doppler E®ect for Sound a. Wave Source and Receiver Both Stationary . 2 Source Ear b. Wave Source Approaching Stationary Receiver . .2 Stationary c. Receiver Approaching Stationary Source . 4 d. Source and Receiver Approaching Each Other . 5 e. Relative Linear Motion: Three Cases . 6 f. Moving Source Not Equivalent to Moving Receiver . 6 g. The Medium is the Preferred Reference Frame . 7 Moving Ear Away 3. The Doppler E®ect for Light a. Introduction . .7 b. Doppler Broadening of Spectral Lines . 7 c. Receding Galaxies Emit Doppler Shifted Light . 8 4. Limitations of the Results . 9 Moving Ear Toward Acknowledgments. .9 Glossary . 9 Project PHYSNET·Physics Bldg.·Michigan State University·East Lansing, MI 1 2 ID Sheet: MISN-0-204 THIS IS A DEVELOPMENTAL-STAGE PUBLICATION Title: The Doppler E®ect OF PROJECT PHYSNET Author: Mary Lu Larsen, Dept. of Physics, Towson State University The goal of our project is to assist a network of educators and scientists in Version: 4/17/2002 Evaluation: Stage 0 transferring physics from one person to another. We support manuscript processing and distribution, along with communication and information Length: 1 hr; 24 pages systems. We also work with employers to identify basic scienti¯c skills Input Skills: as well as physics topics that are needed in science and technology. A number of our publications are aimed at assisting users in acquiring such 1. -
Lecture Notes 17: Proper Time, Proper Velocity, the Energy-Momentum 4-Vector, Relativistic Kinematics, Elastic/Inelastic
UIUC Physics 436 EM Fields & Sources II Fall Semester, 2015 Lect. Notes 17 Prof. Steven Errede LECTURE NOTES 17 Proper Time and Proper Velocity As you progress along your world line {moving with “ordinary” velocity u in lab frame IRF(S)} on the ct vs. x Minkowski/space-time diagram, your watch runs slow {in your rest frame IRF(S')} in comparison to clocks on the wall in the lab frame IRF(S). The clocks on the wall in the lab frame IRF(S) tick off a time interval dt, whereas in your 2 rest frame IRF( S ) the time interval is: dt dtuu1 dt n.b. this is the exact same time dilation formula that we obtained earlier, with: 2 2 uu11uc 11 and: u uc We use uurelative speed of an object as observed in an inertial reference frame {here, u = speed of you, as observed in the lab IRF(S)}. We will henceforth use vvrelative speed between two inertial systems – e.g. IRF( S ) relative to IRF(S): Because the time interval dt occurs in your rest frame IRF( S ), we give it a special name: ddt = proper time interval (in your rest frame), and: t = proper time (in your rest frame). The name “proper” is due to a mis-translation of the French word “propre”, meaning “own”. Proper time is different than “ordinary” time, t. Proper time is a Lorentz-invariant quantity, whereas “ordinary” time t depends on the choice of IRF - i.e. “ordinary” time is not a Lorentz-invariant quantity. 222222 The Lorentz-invariant interval: dI dx dx dx dx ds c dt dx dy dz Proper time interval: d dI c2222222 ds c dt dx dy dz cdtdt22 = 0 in rest frame IRF(S) 22t Proper time: ddtttt 21 t 21 11 Because d and are Lorentz-invariant quantities: dd and: {i.e. -
Determining the Motion of Galaxies Using Doppler Redshift
Determining the Motion of Galaxies Using Doppler Redshift Caitlin M. Matyas The Arts Academy at Benjamin Rush Overview Rationale Objective Strategies Classroom Activities Annotated Bibliography / Resources Standards Appendices Overview The Doppler effect of sound is a method used to determine the relative speeds of an object emitting a sound and an observer. Depending on whether the source and/or observer are moving towards or away from each other, the frequency of the wave will change. This in turn creates a change in pitch perceived by the observer. The relative speeds can easily be calculated using the following formula: � ± �′ = �( ), � ± where f’ represents the shifted frequency, f represents the frequency of the source, v is the speed of sound, vo is the speed of the observer, and vs is the speed of the source. Vo is added if moving towards and subtracted if moving away from the source. vs is added if moving away and subtracted if moving towards the observer. The figures below help to demonstrate the perceived change in frequency. The source is located at the center of the smallest circle. The picture shows waves expanding as they move outwards away from the source, so the earliest emitted waves create the biggest circles. If both the source and observer were stationary, the waves appear to pass at equal periods of time, as seen in figure IA. However, if the source is moving, the frequency appears to change. Figure IB shows what would happen if the source moves towards the right. Although the waves are emitted at a constant frequency, they seem closer together on the right side and farther spaced on the left. -
Glossary | Speed Measuring Device Resources 191.94 KB
GLOSSARY Absorption - The transmitted R.A.D.A.R. beam will, unless otherwise acted upon (absorbed, reflected, or refracted), travel infinitely far. Under practical circumstances, the beam may be partially absorbed by natural and man-made substances. Vegetation such as trees, grass, and bushes will absorb R.A.D.A.R. energy. Freshly turned earth, such as that in a freshly plowed field, will also absorb R.A.D.A.R. Plastics of certain types and foam products will absorb R.A.D.A.R., as makers of "stealth" automotive accessories have discovered. Absorption of R.A.D.A.R. will not result in any inaccuracies in the R.A.D.A.R. readings. It will reduce the strength of the returned signal, and the operational range of the device depending upon the circumstances. Absolute speed limits - Holds that a given speed limit is in force, regardless of environment conditions, i.e., 35 mph or 50 mph. Accuracy - When used in conjunction with R.A.D.A.R. devices means the degree to which the R.A.D.A.R. device measures and displays the correct speed of a target vehicle that it is tracking. Ambient interference - The conducted and/or radiated electromagnetic interference and/or mechanical motion interference at a specific location and at a time which would be detrimental to proper R.A.D.A.R. performance. Antenna horn - The antenna horn is that portion of the R.A.D.A.R. device that shapes and directs the microwave energy (beam). The antenna horn also "catches" the returning microwave energy and directs it to the R.A.D.A.R. -
Doppler Effect
Physical Science Workshop: Astronomy Applications of Light & Color 1 Activity: Doppler Effect Background: • The Doppler effect causes a train whistle, car, or airplane to sound higher when it is moving towards you, and lower when it is moving away from you. From: http://www.physics.purdue.edu/astr263l/inlabs/doppler.html • For sound: high pitch = high frequency = short wavelength • Light is also a wave, and affected by the Doppler effect o longer wavelengths (lower frequencies) of light appear redder o The spectrum of a star moving towards you will appear blueshifted (shorter wavelengths / higher frequencies) o The spectrum of a star moving away from you will appear redshifted (longer wavelengths / lower frequencies) From: http://www.astrosociety.org/education/publications/tnl/55/astrocappella3.html Lab Materials: • computer with internet access S. Sallmen Activity: Doppler Effect Physical Science Workshop: Astronomy Applications of Light & Color 2 Activity: Doppler Basics: • Go to: http://www.fearofphysics.com/Sound/dopwhy2.html 1. Watch the waves reaching your ear if: • the source moves towards your ear at 100 meters / second • the source moves away from your ear at 100 meters / second a. In which case is the frequency of sound higher? b. In which case is the wavelength of the sound waves longest? c. If these were light waves, in which case would the light reaching your eye be redder? d. If these were light waves, in which case would the light reaching your eye be bluer? 2. Watch the waves reaching your ear if: • the source moves away from your ear at 100 meters / second • the source moves away from your ear at 200 meters / second a. -
A One-Map Two-Clock Approach to Teaching Relativity in Introductory Physics
A one-map two-clock approach to teaching relativity in introductory physics P. Fraundorf Department of Physics & Astronomy University of Missouri-StL, St. Louis MO 63121 (December 22, 1996) observation that relativistic objects behave at high speed This paper presents some ideas which might assist teachers as though their inertial mass increases in the −→p = m−→v incorporating special relativity into an introductory physics expression, led to the definition (used in many early curriculum. One can define the proper-time/velocity pair, as 1 0 well as the coordinate-time/velocity pair, of a traveler using textbooks ) of relativistic mass m ≡ mγ. Such ef- only distances measured with respect to a single “map” frame. forts are worthwhile because they can: (A) potentially When this is done, the relativistic equations for momentum, allow the introduction of relativity concepts at an earlier energy, constant acceleration, and force take on forms strik- stage in the education process by building upon already- ingly similar to their Newtonian counterparts. Thus high- mastered classical relationships, and (B) find what is school and college students not ready for Lorentz transforms fundamentally true in both classical and relativistic ap- may solve relativistic versions of any single-frame Newtonian proaches. The concepts of transverse (m0) and longi- problems they have mastered. We further show that multi- tudinal (m00 ≡ mγ3) masses have similarly been used2 frame calculations (like the velocity-addition rule) acquire to preserve relations of the form Fx = max for forces simplicity and/or utility not found using coordinate velocity perpendicular and parallel, respectively, to the velocity alone. -
The Extended Relativity Theory in Clifford Spaces
THE EXTENDED RELATIVITY THEORY IN CLIFFORD SPACES C. Castroa and M. Pav·si·cb May 21, 2004 aCenter for Theoretical Studies of Physical Systems, Clark Atlanta University, Atlanta bJo·zef Stefan Institute, Jamova 39, SI-1000 Ljubljana, Slovenia; Email: [email protected] Abstract A brief review of some of the most important features of the Extended Rela- tivity theory in Cli®ord-spaces (C-spaces) is presented whose " point" coordinates are noncommuting Cli®ord-valued quantities and which incorporate the lines, ar- eas, volumes,.... degrees of freedom associated with the collective particle, string, membrane,... dynamics of p-loops (closed p-branes) living in target D-dimensional spacetime backgrounds. C-space Relativity naturally incorporates the ideas of an invariant length (Planck scale), maximal acceleration, noncommuting coordinates, supersymmetry, holography, higher derivative gravity with torsion and variable di- mensions/signatures that allows to study the dynamics of all (closed) p-branes, for all values of p, on a uni¯ed footing. It resolves the ordering ambiguities in QFT and the problem of time in Cosmology. A discussion of the maximal-acceleration Rela- tivity principle in phase-spaces follows along with the study of the invariance group of symmetry transformations in phase-space that allows to show why Planck areas are invariant under acceleration-boosts transformations and which seems to suggest that a maximal-string tension principle may be operating in Nature. We continue by pointing out how the relativity of signatures of the underlying n-dimensional spacetime results from taking di®erent n-dimensional slices through C-space. The conformal group emerges as a natural subgroup of the Cli®ord group and Relativity in C-spaces involves natural scale changes in the sizes of physical objects without the introduction of forces nor Weyl's gauge ¯eld of dilations. -
Gravity Tests with Radio Pulsars
universe Review Gravity Tests with Radio Pulsars Norbert Wex 1,* and Michael Kramer 1,2 1 Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany; [email protected] 2 Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, UK * Correspondence: [email protected] Received: 19 August 2020; Accepted: 17 September 2020; Published: 22 September 2020 Abstract: The discovery of the first binary pulsar in 1974 has opened up a completely new field of experimental gravity. In numerous important ways, pulsars have taken precision gravity tests quantitatively and qualitatively beyond the weak-field slow-motion regime of the Solar System. Apart from the first verification of the existence of gravitational waves, binary pulsars for the first time gave us the possibility to study the dynamics of strongly self-gravitating bodies with high precision. To date there are several radio pulsars known which can be utilized for precision tests of gravity. Depending on their orbital properties and the nature of their companion, these pulsars probe various different predictions of general relativity and its alternatives in the mildly relativistic strong-field regime. In many aspects, pulsar tests are complementary to other present and upcoming gravity experiments, like gravitational-wave observatories or the Event Horizon Telescope. This review gives an introduction to gravity tests with radio pulsars and its theoretical foundations, highlights some of the most important results, and gives a brief outlook into the future of this important field of experimental gravity. Keywords: gravity; general relativity; pulsars 1. -
Observer with a Constant Proper Acceleration Cannot Be Treated Within the Theory of Special Relativity and That Theory of General Relativity Is Absolutely Necessary
Observer with a constant proper acceleration Claude Semay∗ Groupe de Physique Nucl´eaire Th´eorique, Universit´ede Mons-Hainaut, Acad´emie universitaire Wallonie-Bruxelles, Place du Parc 20, BE-7000 Mons, Belgium (Dated: February 2, 2008) Abstract Relying on the equivalence principle, a first approach of the general theory of relativity is pre- sented using the spacetime metric of an observer with a constant proper acceleration. Within this non inertial frame, the equation of motion of a freely moving object is studied and the equation of motion of a second accelerated observer with the same proper acceleration is examined. A com- parison of the metric of the accelerated observer with the metric due to a gravitational field is also performed. PACS numbers: 03.30.+p,04.20.-q arXiv:physics/0601179v1 [physics.ed-ph] 23 Jan 2006 ∗FNRS Research Associate; E-mail: [email protected] Typeset by REVTEX 1 I. INTRODUCTION The study of a motion with a constant proper acceleration is a classical exercise of special relativity that can be found in many textbooks [1, 2, 3]. With its analytical solution, it is possible to show that the limit speed of light is asymptotically reached despite the constant proper acceleration. The very prominent notion of event horizon can be introduced in a simple context and the problem of the twin paradox can also be analysed. In many articles of popularisation, it is sometimes stated that the point of view of an observer with a constant proper acceleration cannot be treated within the theory of special relativity and that theory of general relativity is absolutely necessary. -
Lecture 21: the Doppler Effect
Matthew Schwartz Lecture 21: The Doppler effect 1 Moving sources We’d like to understand what happens when waves are produced from a moving source. Let’s say we have a source emitting sound with the frequency ν. In this case, the maxima of the 1 amplitude of the wave produced occur at intervals of the period T = ν . If the source is at rest, an observer would receive these maxima spaced by T . If we draw the waves, the maxima are separated by a wavelength λ = Tcs, with cs the speed of sound. Now, say the source is moving at velocity vs. After the source emits one maximum, it moves a distance vsT towards the observer before it emits the next maximum. Thus the two successive maxima will be closer than λ apart. In fact, they will be λahead = (cs vs)T apart. The second maximum will arrive in less than T from the first blip. It will arrive with− period λahead cs vs Tahead = = − T (1) cs cs The frequency of the blips/maxima directly ahead of the siren is thus 1 cs 1 cs νahead = = = ν . (2) T cs vs T cs vs ahead − − In other words, if the source is traveling directly towards us, the frequency we hear is shifted c upwards by a factor of s . cs − vs We can do a similar calculation for the case in which the source is traveling directly away from us with velocity v. In this case, in between pulses, the source travels a distance T and the old pulse travels outwards by a distance csT .