What is the Initial Mass Function Problem?

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SUMMARY

The discussion focuses on solving the Initial Mass Function (IMF) problem for a globular cluster with a total mass of 106 solar masses. The initial mass function is defined as dN/dm = a·m-2.35, where m represents the mass in solar units, ranging from 0.1 to 20 solar masses. The user attempts to find the normalization constant 'a' by integrating the IMF over the specified mass range to equal the total number of stars, 106. The method of using the integral of N(m)dm to derive 'a' is confirmed as correct by another participant in the discussion.

PREREQUISITES
  • Understanding of Initial Mass Function (IMF) in astrophysics
  • Knowledge of integration techniques in calculus
  • Familiarity with globular cluster characteristics and mass ranges
  • Basic concepts of stellar populations and their distributions
NEXT STEPS
  • Study the derivation and applications of the Initial Mass Function (IMF)
  • Learn advanced integration techniques for astrophysical applications
  • Explore the properties and formation of globular clusters
  • Investigate the implications of different IMF shapes on stellar evolution
USEFUL FOR

Astronomy students, astrophysicists, and researchers focusing on stellar populations and the dynamics of globular clusters will benefit from this discussion.

kranav
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Homework Statement


Hello! I am currently working on a initial mass problem and getting nowhere, I need a little help here, the question states

consider a newly formed globular cluster, with total mass 10e6 times that of the sun, and an initial mass function dN/dm = a.m(-2.35) (-2.35 being the power of m of course) in the mass range 0.1-20 mass of the sun, where m=M/mass of the sun. find a.

Homework Equations





The Attempt at a Solution


what i did till now is
we know that globular clusters have 10e4 to 10e6 stars so

integral of N(m)dm = 10e6 where m ranges from .1 to 20 mass of the sun
with this equation I got the value of N which was too small and used the given equation dN/dm = a.m(-2.35) to find a. Is this method correct ?
Thanks.
 
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kranav said:
integral of N(m)dm = 10e6 where m ranges from .1 to 20 mass of the sun
with this equation I got the value of N which was too small and used the given equation dN/dm = a.m(-2.35) to find a. Is this method correct ?
Thanks.

Shouldn't the number of stars in a given mass range m_1\leq m\leq m_2 be equal to

N=\int_{m_1}^{m_2} dN=\int_{m_1}^{m_2} \frac{dN}{dm}dm

?
 
thank you, ill try using this now
 

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