Why can't nanosecond pulsars be used to measure universe expansion?

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wolram
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why can't we use nanosecond pulsars to gauge expansion of
universe? even if they are irregular ,if the "tendancy "of
pulses measured in a second is always downward then at
least it would be a partial proof.
 
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One possible problem with this might be that pulsars are already known to slow down over time. Since this deceleration is considered to be a result of the pulsar losing energy and spinning more slowly, any measured increase in the rate could be the result of expansion, or it could just be the pulsar slowing down more. I can't think of any way to tell the difference.
 
wolfram:
why can't we use nanosecond pulsars
(my emphasis)
Do you have a link describing observations of such bizarre denizens of the cosmic zoo?
 
sorry nereid, i do not have a link its something i read
these nanosecond pulses are coming from a small area
of a microsecond pulsar, a matter of a few squar METRs
if i remember correctly the smallesr thing so far detected
in space,
i hope one of the more informed members can jump in
and save me.
 
In 2003 observations of the Crab nebula pulsar's signal revealed "sub-pulses" within the main signal with durations of only nanoseconds. It is thought that these nanosecond pulses are emitted by regions on the pulsar's surface 60cm in diameter or smaller, making them the smallest structures outside the solar system to be measured.

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found this in wikipida something similar to the article
i read. only this refers to CMs.
 
Thanks wolfram.

So they are nanosecond pulses rather than pulsars.

To turn to your original question:
why can't we use nanosecond pulsars to gauge the expansion of the universe?
I'm not clear on what you had in mind; something special about the pulsar frequency? or simply that the frequency can be measured with extraordinary accuracy?

One difficulty to overcome would be what LURCH pointed to: how to disentangle any 'expansion of the universe' signal in the data from other causes of any slowing that might be observed.

Have you done a calculation of how big the 'expansion of the universe' effect might be?
 
Have you done a calculation of how big the 'expansion of the universe' effect might be?
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well I am sure not qualified in that area, maybe someone has
some figures.
i have 80 cubic kilometers per sec per mega parsec, for
expantion.
cant even remember where i got these from, i may have look
on google later.
the origonal post wasnt well thought out, i just posted it
as a "maybe if".
 
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http://antwrp.gsfc.nasa.gov/apod/ap960513.html

which Freedman and team have used to identify some 50 Cepheids. Their distance and velocity measurements determine Hubble's constant to be about 80 kilometers per second per megaparsec.
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i don t know how upto date this is, but the accuracy of a
nanosecond pulse would give an indication, if only an
average over time?
 
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Assume that there are pulsars which emit nanosecond (sub-)pulses, and that these
are very regular and stable.

How could one use observations of these to "gauge the expansion of the universe"?

BTW, here's a link to the Freedman "Final Results" HST paper on the Hubble constant:
http://arxiv.org/abs/astro-ph/0012376
 
it would depend on how regular the pulsar is, if you
recorded say 60 seconds of the pulses also record
the time t1 of first pulse, then wait a week, month
and do same again, if time of first pulse changes
ie t1+X seconds or the comparison of first and
second recording is out of sync then you know the
source is mooving, after several recordings you
would build a better picture.


thankyou for link.
 
Originally posted by wolram
it would depend on how regular the pulsar is, if you
recorded say 60 seconds of the pulses also record
the time t1 of first pulse, then wait a week, month
and do same again, if time of first pulse changes
ie t1+X seconds or the comparison of first and
second recording is out of sync then you know the
source is mooving, after several recordings you
would build a better picture.
If I can summarise:

We make two measurements of the frequency of the pulses, one 'now' and the other a week (month, year, ...) from 'now'.

Although we don't know what the pulsar's recession speed is, at either time, we can see if the frequency of the pulses has changed.

If the pulse frequency is lower at the second measurement, this might be due, in part, to the expansion of the universe; the further away the pulsar is, the higher its recession speed.

If the pulsar is (observed to be) 1 Mpc from Earth 'now' (so its recession speed is (observed to be) 80 km/s), what will its recession speed be 1 million seconds from 'now' (assume 1 Mpc = 3 x 1019 km)?
{Assume, for the moment, that the pulsar is not accelerating (in its local environment), and that we can factor out all the changes in the Earth's speed over the 1 million seconds.}
 
If the pulsar is (observed to be) 1 Mpc from Earth 'now' (so its recession speed is (observed to be) 80 km/s), what will its recession speed be 1 million seconds from 'now' (assume 1 Mpc = 3 x 1019 km)?
{Assume, for the moment, that the pulsar is not accelerating (in its local environment), and that we can factor out all the changes in the Earth's speed over the 1 million seconds.} [/B]

Wow! this is the first time I wandered in here (since the format changed and categories like Cel Mech were established) and already I see a problem! This is a sign that Nereid is a nice person. Among astronomers giving each other problems is like grooming among monkeys or giving backrubs, it is a friendly gesture

She says wait a million seconds so the thing is 80 million km farther and then how much faster is it going?
She is an astronomer so she makes clear that the distance in the Hubble formula is the distance measured 'now' (so many people do not realize this!)

The fractional increase in distance is 8E7 km/3E19 km so it is around 2.7E-12. This is a negligible fractional increase so the increase in speed is also negligible, it was 80 km/s and it after you have waited E6 seconds it still is 80 km/s

How did this come up. Fraid I haven't read the thread, just saw Nereids name and scrolled down
 
Originally posted by marcus
Wow! this is the first time I wandered in here (since the format changed and categories like Cel Mech were established) and already I see a problem! This is a sign that Nereid is a nice person. Among astronomers giving each other problems is like grooming among monkeys or giving backrubs, it is a friendly gesture

She says wait a million seconds so the thing is 80 million km farther and then how much faster is it going?
She is an astronomer so she makes clear that the distance in the Hubble formula is the distance measured 'now' (so many people do not realize this!)

The fractional increase in distance is 8E7 km/3E19 km so it is around 2.7E-12. This is a negligible fractional increase so the increase in speed is also negligible, it was 80 km/s and it after you have waited E6 seconds it still is 80 km/s

How did this come up. Fraid I haven't read the thread, just saw Nereids name and scrolled down
Thank you for the kind words marcus :smile:

wolfram posted a very good question, about the possibility of using pulsars as (another) means to measure the expansion of the universe. Various people have contributed ideas to how feasible this might be. As you point out, the difference in apparent recession speed would be very small.

Does anyone know how accurately we could measure the signals from a pulsar? I mean, could we tell if a pulsar's period changed by 1 part in 109? or 1 part in 1015? Assume that the signal is sufficiently strong (or that we can integrate over enough signals) so signal detection is not an issue. Assume also that all local contributions to any apparent change in period can be nulled out.
 
Originally posted by Nereid


Does anyone know how accurately we could measure the signals from a pulsar? I mean, could we tell if a pulsar's period changed by 1 part in 109? or 1 part in 1015? Assume that the signal is sufficiently strong (or that we can integrate over enough signals) so signal detection is not an issue. Assume also that all local contributions to any apparent change in period can be nulled out.

even the simplifying assumptions of this question are fun to consider, like the Earth is moving all over the place at one tenthousandth of the speed of light so it is changing the timing of the pulses by one part in 104 all the time by its own
velocity changes and the rotation of the Earth by one part per million by its velocity. So nulling out the local contributions of all the local motion would already be fun.

this is a question that Phobos or Labguy or chroot maybe or selfAdjoint----cant think of which other people---would love to reply to but might not see because of the FORMAT having so many pigeonholes.

there is some historical observation of change of timing of pulsar showing radiation away of energy in form of gravitywaves. it is historical because of the accuracy achieved in measuring the change of timing (whenever the accuracy of measurement in astronomy changes this generates historical advances in some area or other) so by looking at that celebrated measurment you could tell what the leading edge accuracy for pulsar timing at the present era----one of those people would remember the numbers

I don't want to hog the witnessbox so I will get out and let someone else reply. Jeez why isn't everybody all over this question?
 
accuracy of measuring time

IIRC, the NIST time standard claims an accuracy of 10-15. Within a decade this may be improved by up to three orders of magnitude. However, this degree of accuracy is, for all practical purposes, useless. Why?

Assuming a pulsar's distance from the Earth was determined solely by the expansion of the universe (and all local - to the Earth - motions could be accurately determined), at what distance (and over what time period) would a pulsar be for observations of a change in its period to be able to show the Hubble expansion? Assume the arrival time of the pulsar's pulses could be recorded accurately to 1 part in 1015.