Cosmic microwave background Definition and 54 Threads

I've already got "Personal Speculation Warning" and I had a private conversation with @Nugatory, who told me, that I have to publish it in an appropriate peer-reviewed journal before it can be posted for discussion here. I replied with a question, if he is willing to believe, that...

CMB photons can be affected by the expansion of the universe through the linear integrated Sachs-Wolfe effect (ISW) [1] and the non-linear ISW effect or also called Rees-Sciama effect [1]. In particular, according to the ISW effect, the photons crossing superclusters would leave them having a...

The signal-to-noise ratio for angular power spectrum signal Cl under theoretical noise Nl, where Cl and Nl are functions of multipole l, is given as (S/N)^2= \sum (2l+1) (Cl/Nl)^2To increase the S/N we bin the power spectrum signal, if bin width \Delta l, this in principle decreases Nl by a...

If I understand correctly, by reference say here, the results seem to relate to a survey of the Milky Way. 1. Is the Milky Way a 'closed' system? 2. Whether or not, were the surveys based on data from the visible Universe, or restricted in all or part to the data form 'within' the Milky Way.

<unacceptable reference deleted> As our universe is expanding, that is, our vacuum is becoming more and more sparse, I believe it is possible that some key characterics of our vacuum is also variable.

Hi, I have some questions about cosmic microwave background radiation, CMB, and I thought it's better to ask them together. I have combined all related content for each question to make the question clearer, understandable, and to provide proper context for any person like who stumbles upon...

Hi, The following is my basic understanding of blackbody radiation spectrum. The important sections are in boldface. Source: https://en.wikipedia.org/wiki/Black-body_radiation#Spectrum Question 1: The quote above says that at room temperature (let's say 20 C or 293 K) the emission is in the...

Suppose we receive a cosmic microwave background (CMB) photon from space. According to the Big Bang model, this photon became free to travel when the universe was about 0.38 million years (Myr) old. At that time, it was about 42 million light years (Mly) away from our location. Because of the...

So, as I understand it, the photons from the microwave background were the result of photon decoupling. Now, if I remember correctly, because of the accelerated expansion of the universe, the diameter of the universe is not about 28 Gyr, but about 90 Gyr, the consequence of which is that there...

I've been searching for weeks and still with the doubt. I just know scientist look the content of the CMB and with general relativity calculates the expansion rate today that is 73 km/s/Mpc, but nowhere does it say how exactly. What does the contents of the universe have to do with the...

Hi, I have few questions about cosmic microwave background radiation (CMBD) and trying to find simple answer at a basic level. I really appreciate your help and time! The universe is almost 13.799 billion years old and currently has radius of around 46.5 billion light-years. It is said that...

If my understanding is correct... From Earth the cmb is fairly uniform around us. From a galaxy that is 12 billion light years away, would they also see a uniform distribution of the cmb? to add to that question, would the radiation be less redshifted. From my understanding on why we aren't...

Conformal Cyclic Cosmology, or CCC, is a hypothesis put forward by Roger Penrose in the early 2000s. My understanding of physics is lacking so my explanation will not be that clear, but I will summarize it here. Essentially, the existence of a previous spacetime, or "aeon," is postulated. This...

Hello! I am reading some basic stuff in cosmology and I am a bit confused by the microwave background. As far as I understand, it is the radiation produced at the beginning of the universe, when the matter density was not that high so the photon can escape and travel freely. So the microwave...

If the cosmic microwave background occurred at the moment that electrons and protons joined together and photons were now free to travel across the universe, then why haven't those photons already passed it. I'm having a hard time understanding why we can see the CMB forever if it was simply a...

When a "layman" hears of the cosmic microwave background, and this layman also has a passing knowledge of big bang theory, it can be difficult for said layman to wrap his head around what the CMB really is. That layman might ask, wouldn't this primordial radiation have "passed" us by now, and...

Awhile ago, I was considering what sort of dangers a spacecraft moving at relativistic speeds would face in interstellar space. Aside from the obvious pieces of space dust being relativistic bullets in the ship's frame of reference, the cosmic microwave background (CMB) would become a big...

Hi This question may have already been answered elsewhere. If so please accept my apologies in advance. I am confused! The textbok(s) I am reading describe a whole bunch of different causes for there being temperature fluctuations in the CBM, so I am confused about which one(s) of these...

Hello everyone I've a question about the cosmic microwave background which my nephew asked me a couple of days ago. How much energy hits the Earth each year from the CMB? I'm assuming here that it is measurable in this way, but apologies if not. Thanks in advance for your help. Chris

Hi Guys, I studied physics for my bachelor but still I am not a super expert, although I am still working closely to physics (but not so much astronomy). I was wondering if it would be possible to build a radio, or some other devise (any ideas?) that could be tuned at the frequency where the...

How do we know that the cmb is not just related to just our galaxy, and that all galaxies have there own cmb?

I was going over some past papers ( OCR Physics A2 ) and I came across this question about cosmic microwave background radiation-the topic I seem to be struggling with the most :/ and I wasn't sure how to structure my answer. It's worth 5 marks. The question is : Describe the important...

"The cosmic microwave background radiation" is an electromagnetic radiation observed in all directions of the sky and presents a profile type black body with about 3 K temperature. The fact that this allows us to infer the conditions of evolution of matter with radiation of the universe?

I heard sometime ago that the cosmic microwave background may be a candidate for an absolute frame of reference. Did this idea ever get any credence?

What's the bandwidth of CMB and what was the bandwidth of CMB when it was emitted (at the moment when the Universe was 379,000 years old)?

When the Universe was 379,000 years old, the radiation could travel into space. From that point in time the CMB started to be emitted in form of visible light. Am I correct? my question is: for how long the CMB was emitted? Or is it still emitted today? If the CMB was emitted for 10...

Homework Statement The cosmic microwave background radiation has a blackbody type spectrum. Determine its max frequency and the correspondent wavelenght. Verify if found frequency is a microwave frequency and compare with the following curve: Homework Equations Using the...

So to detect the EM waves from this background, did the device that measured it focus on one single point in the sky, kinda like hubble, or did it do a full panoramic spherical measurement of the whole sky around it?

For about the 7th time I've been told the story of how Penzias and Wilson discovered a noise the source of which they could not detect. It turned out to be the CMB. Well, why should the cmb make a noise? It's just photons in the microwave spectrum.

A hypothetical question relating to 1) moving a physical object at a significant % of c. 2) interaction with the cosmic microwave background radiation Is it the case that doppler effect and time dilation means that the CMB is going to be physically damaging to the object? Further...

Is it a section of sky or a full 100% 360 degree panoramic view? I am referring to the cosmic microwave background picture that can be found here: http://en.wikipedia.org/wiki/Cosmic_microwave_background_radiation

Never seen this addressed anywhere, and maybe it doesn't matter; but, regarding the cosmic background radiation, in any given instant, how many 2.73K (on average) photons are in a given volume ? See, we would measure the same background temperature with our instruments over a range of...

Hello, I just have a quick question about CMB. Why is it from 380,000 years after big bang? Why not before? Will you please tell me if my explantion is right? Before 380,000 years, the universe was too dense to have any neutral atoms (free electrons and protons / plasma). And...

Hi firstly I am a photographer not a physicist, When taking photos there is always 'noise' in the image, especially at higher ISO. I presumed this is the same noise that we would hear on a radio, or see on a tv? Would it be possible to create a room that blocked out the background radiation...

In order for the black hole to evaporate it must have a temperature greater than that of the present-day black-body radiation of the Universe. Cosmic microwave background radiation temperature: T_u = 2.725 \; \text{K} Hawking radiation temperature: T_H = \frac{\hbar c^3}{8 \pi G M k_B}...

Homework Statement (a)The cosmic microwave background fits the blackbody radiation spectrum well with a temperature of 2.7 K and a corresponding peak wavelength at 1.9nm. Applying the relationship between the radiant emittance, i.e. the total power emitted per unit area, and the photon energy...

Hi everyone, I'm a lowly computer programmer who has been interested in the CMB lately and recently became curious about one thing... As I understand it, the CMB is the left-over radiation from the Big Bang spread uniformly throughout the universe. Does this mean that this radiation is...

Present critical density of Universe rho_crit = 3 H^2 / 8 Pi G H = Hubble Constant = 2.2E-18 sec^-1 rho_crit = 8.6E-27 kg / m^3 What particle mass does this represent? The length scale associated with a quantum particle of mass m is the Compton wavelength lambda where lambda =...

I am a little confused about how exactly the CMB "works". At first hearing, it makes perfect sense that as time goes on and the universe expands radiation would decrese in frequence, but when I think about it a little more deeply I miss something. My thought is how exactly does the light...

Is the CMBR distinguished by a particular set of spectrometry signatures? If not, how is it differentiated?

CMB hot spots have a physical size that corresponds to the size of the horizon at age 300; 000 yrs. Assume one such hot spot region has been expanding together with the universe, how big in physical size (express in unit of light-year) has it become today? For this exercise, use a model of...

I hope this is an appropriate forum for this question. What kind sort of impact might intensely blue shifted cosmic microwave background (CMB) photons have on hawking radiation? Could intensely blue shifted CMB photons drive a portion of newly created electrons and positrons into the even...

If the light from a distant galaxy was red shifted far enough wouldn't it appear as microwave? Is it possible that the CMB is just more galaxies beyond what we consider to be the "observeable universe?"

Question> The fact (simplified) is that our planet is rotating arount the Sun, also our solar system is rotating... Is there available information on direction of CMBR in relation to our planet or to our solar system? THX foun answer myself Re: does the cosmos have direction...

[FONT="Fixedsys"][SIZE="4"]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?"...

I am trying to wrap my head around the Cosmic Microwave Background and how it is that the low frequency ancient photons we observe could be only 'passing' us in space now. If we think of a photon as an entity that is traveling away from the origin of the Big Bang at 300,000km/s, why would these...

Dear Friends A fleet of spaceships is given, each equipped with a differential microwave radiometer, just like COBE was, whose detectors are antipodeanly pointing (this way one should catch blue shifted radiation and the other one red shifted). Could their acquisitions be used to...

I was looking at a map of the cosmic microwave background, and began wondering if the cmb would look the same from another vantage point, perhaps Pluto, or a nearby star. Or what about if it were seen from another galaxy? And, in a related question, does the cmb evolve with time? I suppose...

We know that the CMB has been decreasing in temperature since the big bang. This is due to the continuing expansion of the universe that results to an increase in the wavelengths of the CMB photons. Increased wavelength => less energy => less temperature. My question is why do the photons have...

According to the standard cosmological model, the description for cosmic temperature falls is:T=A*t^-0.5. So when t-->infinite, T-->0. It means the temperature of microwave background will approach 0k after billions of years. Microwave background will disappear?:confused: