What is the Initial Mass Function Problem?

In summary, the conversation is about a question regarding finding the value of a in an initial mass problem for a newly formed globular cluster with a total mass of 10e6 times that of the sun. The person asking the question has attempted to solve it by using the equation dN/dm = a.m(-2.35) and integrating it with the given mass range, but is unsure if this method is correct. Another person suggests using the equation N = integral of dN = integral of (dN/dm)dm to find the number of stars in a given mass range.
  • #1
kranav
34
0

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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  • #2
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 [itex]m_1\leq m\leq m_2[/itex] be equal to

[tex]N=\int_{m_1}^{m_2} dN=\int_{m_1}^{m_2} \frac{dN}{dm}dm[/tex]

?
 
  • #3
thank you, ill try using this now
 

What is the Initial Mass Function problem?

The Initial Mass Function problem is a question in astrophysics that asks why there is a consistent distribution of masses among stars in a given star-forming region. This distribution is known as the Initial Mass Function (IMF) and it has been observed to be similar in different star-forming regions, leading scientists to wonder why this is the case.

Why is the Initial Mass Function important?

The Initial Mass Function is important because it plays a crucial role in understanding the formation and evolution of galaxies. The IMF determines the number of stars that are formed in a given region and their masses, which ultimately affects the chemical enrichment and energy input of galaxies. It also has implications for the study of stellar populations, star formation rates, and the overall structure of galaxies.

What is the current understanding of the Initial Mass Function?

The current understanding of the Initial Mass Function is that it is a result of the balance between the processes of star formation and the destruction of stars. This balance is believed to be affected by factors such as the physical conditions of the star-forming region, the efficiency of star formation, and the feedback from already-formed stars. However, the exact mechanism that leads to the observed IMF is still not fully understood.

How do scientists study the Initial Mass Function?

Scientists study the Initial Mass Function through various methods, including observations, simulations, and theoretical models. Observations involve using telescopes to gather data on the masses and numbers of stars in different star-forming regions. Simulations use computer models to reproduce the conditions and processes of star formation, while theoretical models use mathematical equations to describe the physical processes involved in star formation and the resulting IMF.

What are the implications of solving the Initial Mass Function problem?

Solving the Initial Mass Function problem would have significant implications for our understanding of the formation and evolution of galaxies. It would also allow us to make more accurate predictions about the properties of stars and their populations, which could have practical applications in fields such as cosmology and astrobiology. Additionally, solving this problem could also lead to a better understanding of the fundamental laws of physics that govern the universe.

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