I know the definitions of both of them, but what is the reason sometimes I see O(1) and other times Θ(1) written in textbooks?
Thanks.
O(1) and Θ(1) aren't necessarily the same if you are talking about functions over real numbers. For example, consider the function f(n) = 1/n. This function is O(1) because for any n ≥ 1, f(n) ≤ 1. However, it is not Θ(1) for the following reason: one definition of f(n) = Θ(g(n)) is that the limit of |f(n) / g(n)| as n goes to infinity is some finite value L satisfying 0 < L. Plugging in f(n) = 1/n and g(n) = 1, we take the limit of |1/n| as n goes to infinity and get that it's 0. Therefore, f(n) ≠ Θ(1).
Hope this helps!
Big-O notation expresses an asymptotic upper bound, whereas Big-Theta notation additionally expresses an asymptotic lower bound. Often, the upper bound is what people are interested in, so they write O(something), even when Theta(something) would also be true. For example, if you wanted to count the number of things that are equal to x in an unsorted list, you might say that it can be done in linear time and is O(n), because what matters to you is that it won't take any longer than that. However, it would also be true that it's Omega(n) and therefore Theta(n), since you have to examine all of the elements in the list - it can't be done in sub-linear time.
UPDATE:
Formally:
f in O(g) iff there exists a c and an n0 such that for all n > n0, f(n) <= c * g(n).
f in Omega(g) iff there exists a c and an n0 such that for all n > n0, f(n) >= c * g(n).
f in Theta(g) iff f in O(g) and f in Omega(g), i.e. iff there exist a c1, a c2 and an n0 such that for all n > n0, c1 * g(n) <= f(n) <= c2 * g(n).
Related
Just started learning algorithm. But, I don't know what n0 represent in calculating time complexity.
Full quoto for the mergeSort time complexity.
Ө(nlogn) - C1 * nlogn <= T(n) <= C2 * logn, if n >= n0
O(nlogn) - T(n) <= C * nlogn, if n >= n0
Intuitively speaking, the statement f(n) = O(g(n)) means
For any sufficiently large value of n, the value of f(n) is bounded from above by a constant multiple of g(n).
In other words, although f(n) might initially start off significantly larger than g(n), in the long-run, you'll find that f(n) is eventually matched, or overtaken, by some constant multiple of g(n).
The n0 you're referring to here is the formal mathematical way of pinning down this idea of "sufficiently large." Specifically, if the claim being made is
T(n) ≤ C2 n log n, if n ≥ n0,
the value n0 is some cutoff threshold. That is, it's the point where we say that n is "sufficiently large."
The particular choice of n0 and C2 in the above statements will depend on the particular problem that you're working through, but hopefully this gives you a sense of how to interpret what you're looking at.
I was given the function 5n^3+2n+8 to prove for big-O and big-Omega. I finished big-O, but for big-Omega I end up with a single-term function. I canceled out 2n and 8 because they're positive and make my function larger, so I just end up with 5n^3. How do I choose C and n_0? or is it simply trivial in this case?
From Big-Ω (Big-Omega) notation (slightly modified):
If a running time of some function f(n) is Ω(g(n)), then for large
enough n, say n > n_0 > 0, the running time of f(n) is at least
C⋅g(n), for some constant C > 0.
Hence, if f(n) is in Ω(g(n)), then there exists some positive constants C and n_0 such at the following holds
f(n) ≥ C⋅g(n), for all n > n_0 (+)
Now, the choice of C and n_0 is not unique, it suffices that you can show one such set of constants (such that (+) holds) to be able to describe the running time using the Big-Omega notation, as posted above.
Hence, you are indeed almost there
f(n) = 5n^3+2n+8 > 5n^3 holds for all n larger than say, 1
=> f(n) ≥ 5⋅n^3 for all n > n_0 = 1 (++)
Finally, (++) is just (+) for g(n) = n^3 and C=5, and hence, by (+), f(n) is in Ω(n^3).
I'm fairly new to the Big-O stuff and I'm wondering what's the complexity of the algorithm.
I understand that every addition, if statement and variable initialization is O(1).
From my understanding first 'i' loop will run 'n' times and the second 'j' loop will run 'n^2' times. Now, the third 'k' loop is where I'm having issues.
Is it running '(n^3)/2' times since the average value of 'j' will be half of 'n'?
Does it mean the Big-O is O((n^3)/2)?
We can use Sigma notation to calculate the number of iterations of the inner-most basic operation of you algorithm, where we consider the sum = sum + A[k] to be a basic operation.
Now, how do we infer that T(n) is in O(n^3) in the last step, you ask?
Let's loosely define what we mean by Big-O notation:
f(n) = O(g(n)) means c · g(n) is an upper bound on f(n). Thus
there exists some constant c such that f(n) is always ≤ c · g(n),
for sufficiently large n (i.e. , n ≥ n0 for some constant n0).
I.e., we want to find some (non-unique) set of positive constants c and n0 such that the following holds
|f(n)| ≤ c · |g(n)|, for some constant c>0 (+)
for n sufficiently large (say, n>n0)
for some function g(n), which will show that f(n) is in O(g(n)).
Now, in our case, f(n) = T(n) = (n^3 - n^2) / 2, and we have:
f(n) = 0.5·n^3 - 0.5·n^2
{ n > 0 } => f(n) = 0.5·n^3 - 0.5·n^2 ≤ 0.5·n^3 ≤ n^3
=> f(n) ≤ 1·n^3 (++)
Now (++) is exactly (+) with c=1 (and choose n0 as, say, 1, n>n0=1), and hence, we have shown that f(n) = T(n) is in O(n^3).
From the somewhat formal derivation above it's apparent that any constants in function g(n) can just be extracted and included in the constant c in (+), hence you'll never (at least should not) see time complexity described as e.g. O((n^3)/2). When using Big-O notation, we're describing an upper bound on the asymptotic behaviour of the algorithm, hence only the dominant term is of interest (however not how this is scaled with constants).
If I have already known f(n) is O(g(n)). From the definition of little-oh, how to prove that f(n) is o(n * g(n))?
Given: f(n) is in O(g(n)).
Using the definition of big-O notation, we can write this as:
f(n) is in O(g(n))
=> |f(n)| ≤ k*|g(n)|, for some constant k>0 (+)
for n sufficiently large (say, n>N)
For the definition of big-O used as above, see e.g.
https://www.khanacademy.org/computing/computer-science/algorithms/asymptotic-notation/a/big-o-notation
Prove: Given (+), then f(n) is in o(n*g(n)).
Lets first state what little-o notation means:
Formally, f(n) = o(g(n)) (or f(n) ∈ o(g(n))) as n → ∞ means that
for every positive constant ε there exists a constant N such that
|f(n)| ≤ ε*|g(n)|, for all n > N (++)
From https://en.wikipedia.org/wiki/Big_O_notation#Little-o_notation.
Now, using (+), we can write
|f(n)| ≤ k*|g(n)|, som k>0, n sufficiently large
<=> { n > 0 } <=> n*|f(n)| ≤ k*n*|g(n)|
<=> n*|f(n)| ≤ k*|n*g(n)|
<=> |f(n)| ≤ (k/n)*|n*g(n)| (+++)
Return to the definition of little-o, specifically (++), and let, without loss of generality, k be fixed. Now, every positive constant ε can be described as
ε = k/C, for some constant C>0 (with k fixed, k>0) (*)
Now, assume, without loss of generality, that n is larger than this C, i.e., n>C. Then, (*) and (+++) yields
|f(n)| ≤ (k/n)*|n*g(n)| < (k/C)*|n*g(n)| = ε*|n*g(n)| (**)
^ ^
| |
since `n>C` (*)
Since we're studying asymptotic behaviour, we can choose to to assign a lower bound to n to any value larger than C (in fact, that's in the definition of both big-O and little-o, "n sufficiently large"), and hence---by the definition of little-oh above---, we have:
- As shown above, (+) implies (**)
- By the definition of little-o, (**) shows that f(n) is in o(n*g(n))
- Subsequently, we've shown that, given (+), then: f(n) is in o(n*g(n))
Result: If f(n) is in O(g(n)), then f(n) is in o(n*g(n)), where these two relations refer big-O and litte-O asymptotic bounds, respectively.
Comment: The result is, in fact, quite trivial. The big-O and little-o notation differ only in one of the two constants used in proving the upper bounds, i.e., we can write the definitions of big-O and little-O as:
f(n) is said to be in O(g(n)) if we can find a set of positive constants (k, N), such that f(n) < k*g(n) holds for all n>N.
f(n) is said to be in o(g(n)) if we can find a positive constant N, such that f(n) < ε*g(n) holds for all n>N, and for every positive constant ε.
The latter is obvious a stricter constraint, but if we can make use of one extra power of n in the left-hand-side of f(n) < ε*g(n) (i.e., f(n) < ε*n*g(n)), then even for infinitesimal values of ε, we can always choose the other constant N freely to be sufficiently large for ε*n to provide us any constant k that can be used to show that f(n) is in O(g(n)) (as, recall, n>N).
Why is ω(n) smaller than O(n)?
I know what is little omega (for example, n = ω(log n)), but I can't understand why ω(n) is smaller than O(n).
Big Oh 'O' is an upper bound and little omega 'ω' is a Tight lower bound.
O(g(n)) = { f(n): there exist positive constants c and n0 such that 0 ≤ f(n) ≤ cg(n) for all n ≥ n0}
ω(g(n)) = { f(n): for all constants c > 0, there exists a constant n0 such that 0 ≤ cg(n) < f(n) for all n ≥ n0}.
ALSO: infinity = lim f(n)/g(n)
n ∈ O(n) and n ∉ ω(n).
Alternatively:
n ∈ ω(log(n)) and n ∉ O(log(n))
ω(n) and O(n) are at the opposite side of the spectrum, as is illustrated below.
Formally,
For more details, see CSc 345 — Analysis of Discrete Structures
(McCann), which is the source of the graph above. It also contains a compact representation of the definitions, which makes them easy to remember:
I can't comment, so first of all let me say that n ≠ Θ(log(n)). Big Theta means that for some positive constants c1, c2, and k, for all values of n greater than k, c1*log(n) ≤ n ≤ c2*log(n), which is not true. As n approaches infinity, it will always be larger than log(n), no matter log(n)'s coefficient.
jesse34212 was correct in saying that n = ω(log(n)). n = ω(log(n)) means that n ≠ Θ(log(n)) AND n = Ω(log(n)). In other words, little or small omega is a loose lower bound, whereas big omega can be loose or tight.
Big O notation signifies a loose or tight upper bound. For instance, 12n = O(n) (tight upper bound, because it's as precise as you can get), and 12n = O(n^2) (loose upper bound, because you could be more precise).
12n ≠ ω(n) because n is a tight bound on 12n, and ω only applies to loose bounds. That's why 12n = ω(log(n)), or even 12n = ω(1). I keep using 12n, but that value of the constant does not affect the equality.
Technically, O(n) is a set of all functions that grow asymptotically equal to or slower than n, and the belongs character is most appropriate, but most people use "= O(n)" (instead of "∈ O(n)") as an informal way of writing it.
Algorithmic complexity has a mathematic definition.
If f and g are two functions, f = O(g) if you can find two constants c (> 0) and n such as f(x) < c * g(x) for every x > n.
For Ω, it is the opposite: you can find constants such as f(x) > c * g(x).
f = Θ(g) if there are three constants c, d and n such as c * g(x) < f(x) < d * g(x) for every x > n.
Then, O means your function is dominated, Θ your function is equivalent to the other function, Ω your function has a lower limit.
So, when you are using Θ, your approximation is better for you are "wrapping" your function between two edges ; whereas O only set a maximum. Ditto for Ω (minimum).
To sum up:
O(n): in worst situations, your algorithm has a complexity of n
Ω(n): in best case, your algorithm has a complexity of n
Θ(n): in every situation, your algorithm has a complexity of n
To conclude, your assumption is wrong: it is Θ, not Ω. As you may know, n > log(n) when n has a huge value. Then, it is logic to say n = Θ(log(n)), according to previous definitions.