Schechter luminosity function (integration)

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SUMMARY

The discussion focuses on the integration of the Schechter luminosity function for galaxies, defined by the parameters α = 1.25, L* = 2.0E10 solar luminosities, and φ* = (3 Mpc)^-3. The integration process reveals that the total number density of galaxies diverges, indicating an infinite number of galaxies due to the contribution from low luminosity galaxies. Participants emphasize the importance of correctly applying integration limits and the implications of the results, particularly the significance of the lower limit approaching zero luminosity.

PREREQUISITES
  • Understanding of the Schechter luminosity function
  • Familiarity with integration techniques in calculus
  • Knowledge of astrophysical units, specifically solar luminosities
  • Basic concepts of galaxy number density
NEXT STEPS
  • Study the derivation and implications of the Schechter luminosity function
  • Learn advanced integration techniques in calculus, focusing on improper integrals
  • Explore the significance of luminosity functions in galaxy formation theories
  • Investigate observational methods for measuring galaxy luminosities
USEFUL FOR

Astronomers, astrophysicists, and students studying galaxy formation and evolution will benefit from this discussion, particularly those interested in the mathematical modeling of galaxy distributions.

iloveannaw
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Suppose the luminosity function of galaxies is given by the approximation:

dn = [tex]\varphi[/tex] L dL = [tex]\varphi[/tex]* (L / L*)^-[tex]\alpha[/tex] dL/L* when L < L*
and
dn = [tex]\varphi[/tex] L dL = 0 when L > L*

where [tex]\alpha[/tex] = 1.25, L* = 2.0E10 solar luminosities and [tex]\varphi[/tex]* = (3Mpc)^-3

Integrate the above eqn to find the total number density of galaxies, integrated over all luminosities. Ypu should find that the integral diverges (e.g. the number of galaxies is infinite)

Well the integration part seemed fairly straight forward, taking x = (L/L*) and dx = dL/L* I got:

I = [tex]\int[/tex] [tex]\varphi[/tex]* (L / L*)^-[tex]\alpha[/tex] dL/L* = [tex]\varphi[/tex]*[tex]\int[/tex] x^-[tex]\alpha[/tex] dx

I = [tex]\varphi[/tex]* (x^(1-[tex]\alpha[/tex])) / (1-[tex]\alpha[/tex])
I = ((3 Mpc)^-3 . (2.0E10 SLs)^-0.25) / -0.25 = (very small negative value)(1 SL)

Im pretty sure the number of galaxies is not less than zero just can't figure this question out. As limits I've taken:
upper limit = L*
lower limit = 0

thanks in advance
 
Last edited:
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It really hurts my eyes when you write the latex code like that :D Just write the entire equation inside the brackets next time. Also, don't forget to plug in your integration limits since they are usually important for getting the right answer. You get an answer which is "[tex]\infty[/tex] - something small", where the infinity comes from the lower limit (as you might expect, since there are many galaxies with near-zero luminosity as seen from earth.)
 

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