EBK AN INTRODUCTION TO MODERN ASTROPHYS
EBK AN INTRODUCTION TO MODERN ASTROPHYS
2nd Edition
ISBN: 9781108390248
Author: Carroll
Publisher: YUZU
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Question
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Chapter 6, Problem 6.11P

(a)

To determine

The value of vl, vm and vu.

(a)

Expert Solution
Check Mark

Answer to Problem 6.11P

The value of vl is 1.405GHz, value of vm is 1.43GHz and the value of vu is 1.455GHz.

Explanation of Solution

Write the expression for bandwidth at the center when vlvvm.

    fv=vvmvlvlvmvl        (1)

Here, fv is the bandwidth and ν is the frequency.

Write the expression for bandwidth at the center, when vmvvu.

    fv=vvuvm+vuvuvm        (2)

Write the expression for relation between the different frequency.

    vvl=vmvl        (3)

Conclusion:

Substitute 1 fv, 1.430GHz for v and (50MHz2) for vmvl in equation (1).

    1=1.430GHzvl50MHz2vl1.430GHzvl=(50MHz2×1GHz103MHz)vl=1.430GHz0.025GHz=1.405GHz

Substitute 1 fv, 1.430GHz for v and (50MHz2) for vuvm in equation (2).

    1=vu1.430GHzvu50MHz2vu1.430GHz=(50MHz2×1GHz103MHz)vu=1.430GHz+0.025GHz=1.455GHz

Substitute 1.430GHz for v in equation (3).

    vvl=vmvlvm=vvl+vl=1.43GHz

Thus, the value of vl is 1.405GHz, value of vm is 1.43GHz and the value of vu is 1.455GHz.

(b)

To determine

The total power measured at the receiver.

(b)

Expert Solution
Check Mark

Answer to Problem 6.11P

The total power measured at the receiver is 4.908×1018W.

Explanation of Solution

Write the expression for amount of energy detected per second.

    P=AvS(v)fvdvdA        (4)

Here, S(v) is the spectral flux density and fv is the efficiency of the detector.

Conclusion:

Substitute functional form of filter function and integrate equation (4).

    P=AvS(v)fvdvdA=πS0(D2)2vlvufvdv=πS0(D2)2[12(vuvl)]        (5)

Substitute 2.5mJy S0, 100m for D, 1.455GHz for vu and 1.405GHz for vl in equation (5).

    P=π(2.5mJy)(100m2)2[12(1.455GHz1.405GHz)]=π(2.5mJy×1029Wm2Hz11mJy)(100m2)2[12(1.455GHz1.405GHz)]=4.908×1018W

Thus, the total power measured at the receiver is 4.908×1018W.

(c)

To determine

The power emitted at the source.

(c)

Expert Solution
Check Mark

Answer to Problem 6.11P

The power emitted at the source is 7.45×1042W.

Explanation of Solution

Write the expression of power of telescope at distance d.

    Ptec=Pemit(π(D/2)24πd2)        (6)

Here, Ptec is the power of telescope, Pemit is the power emitted at the source and d is the distance from telescope.

Conclusion:

Substitute 4.908×1018W Ptec, 100Mpc for d and 100m for D in equation (6).

    (4.908×1018W)=Pemit(π(100m2)24π(100Mpc)2)Pemit=(4.908×1018W)(4π(100Mpc×3.086×1022m1Mpc)2π(100m2)2)=7.45×1042W

Thus, the power emitted at the source is 7.45×1042W.

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