What is Cmb: Definition and 250 Discussions

The cosmic microwave background (CMB, CMBR), in Big Bang cosmology, is electromagnetic radiation which is a remnant from an early stage of the universe, also known as "relic radiation". The CMB is faint cosmic background radiation filling all space. It is an important source of data on the early universe because it is the oldest electromagnetic radiation in the universe, dating to the epoch of recombination. With a traditional optical telescope, the space between stars and galaxies (the background) is completely dark. However, a sufficiently sensitive radio telescope shows a faint background noise, or glow, almost isotropic, that is not associated with any star, galaxy, or other object. This glow is strongest in the microwave region of the radio spectrum. The accidental discovery of the CMB in 1965 by American radio astronomers Arno Penzias and Robert Wilson was the culmination of work initiated in the 1940s, and earned the discoverers the 1978 Nobel Prize in Physics.
CMB is landmark evidence of the Big Bang origin of the universe. When the universe was young, before the formation of stars and planets, it was denser, much hotter, and filled with an opaque fog of hydrogen plasma. As the universe expanded, both the plasma and the radiation filling it grew cooler. When the temperature had dropped enough, protons and electrons combined to form neutral hydrogen atoms. Unlike the plasma, these newly conceived atoms could not scatter the thermal radiation by Thomson scattering, and so the universe became transparent. Cosmologists refer to the time period when neutral atoms first formed as the recombination epoch, and the event shortly afterwards when photons started to travel freely through space is referred to as photon decoupling. The photons that existed at the time of photon decoupling have been propagating ever since, though growing fainter and less energetic, since the expansion of space causes their wavelength to increase over time (and wavelength is inversely proportional to energy according to Planck's relation). This is the source of the alternative term relic radiation. The surface of last scattering refers to the set of points in space at the right distance from us so that we are now receiving photons originally emitted from those points at the time of photon decoupling.

View More On Wikipedia.org
  1. F

    Calculation of CMB anisotropies size

    hello, I am interested in calculating the size of the anisotropies of the CMB to make the comparison with the observed angle through the WMAP satellite. I found an article on the physics of microwave background anisotropies and which explains all the different physical processes that occur...
  2. B

    Confused about cmb decoupling/recombination

    I went to wikipedia to look up decoupling and ended up getting a pretty crappy result "In physical cosmology, the term decoupling is often used for the moment during recombination when the rate of Compton scattering became slower than the expansion of the universe. At that moment, photons...
  3. D

    Current CMB photon number density?

    Question Estimate the current number of cosmic microwave background (CMB) photons there are now, per cubic meter, given that the mean photon energy of a blackbody distribution is about 2.70kT. Method http://en.wikipedia.org/wiki/Planck_function" gives the energy density (i.e. energy per...
  4. C

    CMB SLS one instant or over a period of time

    My question is regarding when the the CMB was created. I understand that it is predicted to have been "when the universe cooled to about 3,000K". However, might it have been possible that different areas of the universe reached that temperature and decoupled a little earlier than others? This...
  5. B

    Does recent expansion change the predicted CMB temperature?

    During the interval from t = 380,000 yr (CMB last surface) to the present, if the Universe were exclusively matter at critical density, the scale factor [1+z] would be proportional to t to the 2/3 power. Note that [13.7 Gyr/380,000 yr] raised to the power 2/3 corresponds to [1+z] = 1090. This of...
  6. X

    Cmb 13.7 billion light years away

    Cosmic Microwave Background radiation is coming to us from about 13.7 billion light years away... is that correct? The reason its coming from 13.7 billion ly away is because the universe is 13.7 billion years old... is that correct? so when the universe was only 12 billion years old the...
  7. M

    Calc. Temperature of CMB | Textbook Info

    Which textbook does contain some accessible details of the calculation of the temperature of CMB? Thx!
  8. M

    CMB Cosmic Microwave Background

    How does one convert measurements in radio astronomical terms to temperature (Kelvin)? Specifically: Penzias & Wilson's measurement of CMB was "excess temperature at 4080 Mc/s." HOW does this yield a "value of about 3.5 degrees Kelvin higher than expected?" Basically, how do you get from...
  9. S

    CMB fluctuations and large scale fluctuations nowadays do not match ?

    CMB fluctuations and large scale fluctuations nowadays do not match ? The CMB dark matter density fluctuations for big scales is d_rho/rho~ 10^-5 and lower. The scale factor increased ~ 1000 times from last scattering to now. Linear perturbation theory predicts that the density fluctuations...
  10. S

    Absolute velocity, CMB, and doppler shift

    I've heard it said that it is impossible to determine an objects absolute velocity, all one can do is find it relative to some other object... but, if the CMB is everywhere, why could you not just measure the doppler shift in all directions, and adjust your velocity so the CMB has no doppler...
  11. F

    The Curvature of Space: Understanding the Flatness of the Universe

    Good day. I've been reading and reviewing the posts and linked references on this forum for about 3 weeks now (enjoying the heck out of the exchanges BTW) and have assimilated much of the information (I think). I am trying to understand how it fits together and several questions remain. This...
  12. Nabeshin

    CMB Flux Density: Deriving For Present Cosmology

    Does anyone know where I can find numbers (or how to derive) the CMB flux density (W/m^2)? I'm only really interested in our present cosmological time, so a solution may assume the CMB to be at a constant temperature.
  13. T

    The first CMB peak - Flat Universe

    The size of bouncing lumps of charged particles, DM and photons in the primordial universe is supposed to be around 220,000 lyr (= sound horizon since the acoustic speed is approx 0.6c). If we then calculate the angle A subtended at Earth by a lump of this size W, some 13.8 Glyr away D (back at...
  14. B

    CMB Anisotropy: Measuring Our Motion Through Space

    Smoot et. al. have measure a dipole (as well as higher order anisotropies) in the cosmic microwave background. This has been interpreted as our motion through the universe. so how do we know that the dipole is due to our motion through space and not the anisotropic expansion of space? the...
  15. C

    CMB Redshift Question (Visible Wavelengths)

    I've looked quite a bit on this forum and also elsewhere online and I cannot really find any information on my inquiry. If this is a double post please delete and send me in the right direction. Now I may be totally off on my thought process, but as I understand it the CMB first started off...
  16. Spinnor

    Does the CMB allow special rest frames to be defined?

    Does the CMB allow special "almost" rest frames to be defined? In this sense, use a rocket to put yourself in a frame of reference such that in this frame observations of the CMB would average to zero (average over photon momentum) over your celestial sphere. In such a rest frame is the total...
  17. E

    Is the Cosmic Microwave Background a Picture of the Universe's Past?

    Hi, Am I right when I say that the cosmic microwave background is a picture of the radiation left from recombination but that the picture (from COBE or WMAP) that we see today is not exactly the same as it was then due to the redshifting of the radiation particles. The flucuations that we see...
  18. S

    CMB: Is it a Background & Why Do We Need Alternatives?

    Why do we require a background-free theory when we have such a convenient and universal cosmic microwave background map?
  19. L

    How do astronomers look at historic CMB?

    How do astronomers "look" at historic CMB? I have a few question regarding CMB (Cosmic Microwave Background): I am confused, when I look at this is this a 360 degree view or a normal one sided view? As recent study that shown the universe is flat, do astronomer did consider at which...
  20. C

    Olbers' Paradox, the CMB and the observable universe

    From Olbers' paradox, the night sky is dark because the universe is finite in age, so some stars' light hasn't had time to reach us. BUT, we see the CMB which occurred some 13 billion years ago (14 billion maybe?) So, if light from the cmb has had time to reach us, shouldn't every object's light...
  21. 8

    CMB Particle Distribution: Shell or Ball?

    Are the particles that comprise the CMB in the shape of a "shell" so that all of these particles are very far from our Solar System, or are they in the form of a solid "ball" so that they are evenly distributed throughout our Observable Universe in which case some would be located right here...
  22. M

    CMB Clarifications: Understanding the Impact of Expansion and Temperature Shift

    Hi, I am trying to get some confirmation of a few facts about how CMB underwrites the current cosmological model. I actually have a few questions on this topic, but will first try my luck with an issue I believe described in terms of a blackbody radiator, which is then said to explain how the...
  23. I

    Exploring CMB Mass Corresponding with Dark Matter

    I heard that dark matter could be the CMB mass corresponding, but I am not satisfied from that. What about this?
  24. Barnak

    Temperature of the CMB, from WMAP

    Maybe someone could help me on a technical detail and the WMAP (the latest "five years" results). On this website (and several others too), you can find some very nice textures of the CMB from the WMAP study : http://lambda.gsfc.nasa.gov/product/map/current/sos/ Then, they say (read the WMAP...
  25. I

    Could we expect that temperature of CMB decreases or increases?

    Could we expect that temperature of CMB decreases or increases? Could we suppose that we are in a contracting universe?
  26. ThomasT

    Dark Energy and CMB: Exploring their Possible Connection

    Is it possible to relate the hypothesized dark energy of the universe with the CMB wavelength?
  27. M

    Untangling the Implications of CMB for the Cosmological Model

    While I think I understand the general principle behind CMB and blackbody radiation, I am trying to understand whether it directly supports the current assumptions about age and size of the universe. Therefore, I was hoping that some members of this forum might be able to clarify what basic...
  28. I

    What will happen when the CMB will raise the zero?

    What will happen when the CMB will raise the zero?
  29. marcus

    Three video-talks on the CMB and structure of universe

    Joao Magueijo. Cosmologist at London Imperial, and Perimeter Institute. Three introductory lectures on the CMB observation and interpretation The first talk is a light intro to the technology, the software that does the mapping, and the analysis that derives the power spectrum (what...
  30. marcus

    Lyman Page new idea for CMB observations

    Lyman Page is a senior observational cosmologist who publishes in good company like with Charles Bennett, Joanna Dunkley, David Spergel and Ned Wright. He and an associate have a new idea about getting information from the CMB http://arxiv.org/abs/0706.3908 to me it seems conceptually novel...
  31. D

    Illustrating the CMB: Drawing Concentric Circles to Show Expansion Over Time

    On a sheet of paper draw four concentric circles, one outside the other. Fill the innermost circle with dots. This is the CMB photons at the point in time when they were scattered throughout the early universe and first became liberated from the spreading dense matter cloud that scattered...
  32. Nim

    Why is the peak frequency of the Cosmic Microwave Background 160 GHz?

    What is the peak frequency of the Cosmic Microwave Background? Using Wien's Displacement (#1) and then converting the wavelength of frequency (#2), I get 282 GHz. #1. 0.0028977685 / 2.728 = 0.00106223185483871 Meters (1 millimeter) #2. 299792458 / 0.00106223185483871 =...
  33. H

    Exploring the Cosmological Frame of CMB

    How to understand that the cosmic microwave background (CMB) can define a cosmological frame? Cheers!
  34. T

    How do they measure the CMB temperature?

    How do they measure the CMB temperature? Aren't they just some radiation?
  35. C

    CMB vs Neutrino BG: Why Does Neutrino Transparency Occur First?

    Hey, Was reading how the CMB is ~2.75 Kelvin, while the Neutrino BG is ~2 Kelvin. Clearly this means that neutrino transparency occurred before photon transparency did in the early evolution of the universe. My question is why? Does is have anything to do with neutron-to-proton decay...
  36. D

    CMB and prefered lorentz frames

    Consider two farmes of reference moving relative each other. In one of the frames the CMD is fully isotropic, i.e., it looks the same in all directions. In the other frame however, the CMD should be red shifted in one direction and blue shifted in the other direction. Thus, the first frame can...
  37. K

    What is the logical setup that determines the epoch of the CMB?

    I'm not sure how it is derived. Do we follow this order? 1. Temperature at last scattering/recombination/decoupling (3000 K) 2. Measuring the temperature of the CMB (~3K) 3. 3000K/~3K = 1100 4. z=1100 5. t(z) Or this order? 1. Assume Big Bang and Inflation 2. Determine Volume and Pressure 3...
  38. V

    Is the CMB dipole influenced by the recession velocity of the CMB?

    The Local Groups motion relative to the CMB is said to be around 700 km/s. I would have thought there would be no motion relative to the rest frame of the CMB, and instead expected it to be at a constant distance regardless of motion. Do we have to factor in the speed at which the CMB is...
  39. marcus

    What is the Latest Update on CMB (end 2005)?

    http://arxiv.org/abs/astro-ph/0601307 Cosmic Microwave Background Mini-Review Douglas Scott, George Smoot 8 pages, 2005 partial update for the 2006 edition of "The Review of Particle Physics", available on the PDG WWW pages at http://pdg.lbl.gov/ "A compact overview of the status of...
  40. vincentm

    CMB: Understanding Uniformity & Isotropy

    Ok, I'm reading up on the Cosmic Microwave background radiation guys. And I'm at a part that confuses me (actually i kinda don't understand the whole thing, but I'm trying) regarding the uniformity or isotropy. If someone can put this in a simpler form so that i can understand it easier i'd...
  41. honestrosewater

    Quickie: CP and power spectrum of the CMB

    Would the power spectrum of the CMB tell you whether the cosmological principle is correct? Ack, I was going to try to explain my reasoning, but it doesn't really count as reasoning. :redface: I guess I was wondering what the CMB power spectrum tells you. If it's complicated, nevermind; I'm...
  42. marcus

    What impact on QG if the CMB map is revised?

    A paper just came out this month that makes it more certain that the Cosmic Microwave map will have to be revised, with even less quadrupole and octopole power. http://www.arxiv.org/abs/astro-ph/0508047/ On the large-angle anomalies of the microwave sky I opened a thread on this paper in...
  43. T

    Where Can I Find Comprehensive Resources on the Cosmic Microwave Background?

    Does anyone here know of any good books or sites that describe the CMB in a comprehensive way? I want to learn more about it, because I find it very interesting, but most of what I've found is just snippets here and there, or descriptions that either take for granted that I know a lot about...
  44. M

    Where did the energy in the CMB go to?

    This may seem like a silly question, but it has me puzzled. Theory tells us that as space expands then photons (and I guess all form of energy?) in that space are red-shifted, ie their wavelength increases, ie they lose energy. The most obvious example of this is the CMB, which consists of...
  45. Chronos

    What is the latest research on CMB anisotropy and its implications?

    Here is the latest entry in the CMB anisotropy derby: The Multipole Vectors of WMAP, and their frames and invariants http://arxiv.org/abs/astro-ph/0502574 The authors, Land and Magueijo, are prominent among the more active researchers in this arena. They apply an apparently more...
  46. S

    CMB, Sky Surveys, & Computational Cosmology

    Recently, several groups have endeavored to experimentally map the large-scale structure of the Universe with the Sloan Survey being the most ambitious. At the same time, we've been able to map the cosmic microwave background to 10^-6 degrees. I believe these two maps agree but I'm confused...
  47. B

    Ekpyrotic model and CMB observations?

    Hello folks, I'm new to this fine forum and wondered if anyone here knows which present or future spacecraft (perhaps even balloon borne mission?) are capable of discriminating the effects of the strongly blue shifted gravitational spectrum that should be evident in the CMB as the Ekpyrotic...
  48. A

    CMB Anisotropies Reveal Quantized Gravity

    Dated as of today: http://arxiv.org/abs/astro-ph/0401070 What do you think guys? :)
  49. H

    CMB anisotropies and matter structures

    CMB anisotropies are deviations of the temperature of the black body emission mainly (but not only) by photons, which have to climb out gravitational potential of higher density concentrations during recombination epoch and during their spatio-temporal trajectory till now (Sachs-Wolfe effect)...
  50. H

    Gravitational waves and CMB polarization

    Gravitational waves generated during inflation should produce a special component in linear polarization in the CMB. Why? Could anyone give an easy qualitative explanation? Thanx.
Back
Top