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Superior highly composite number

A superior highly composite number is a positive n for which there exists some \epsilon > 0 such that \frac{d(n)}{n^\epsilon} \geq \frac{d(k)}{k^\epsilon} for all positive integers k, where d(m) denotes the number of positive divisors of m. These numbers represent the maxima of the normalized by a power of the itself, providing a refined class within highly composite numbers, which are positive integers with strictly more divisors than any smaller positive . Introduced by the Indian mathematician in his 1915 paper "Highly Composite Numbers," superior highly composite numbers extend the study of numbers with unusually many divisors, motivated by their role in asymptotic estimates for d(n). Ramanujan proved that every such number has a prime factorization of the form n = 2^{a_1} 3^{a_2} 5^{a_3} \cdots p_r^{a_r}, where the exponents a_1 \geq a_2 \geq \cdots \geq a_r \geq 1 are non-increasing, the primes p_i are the first r primes, and the exponents satisfy specific inequalities derived from logarithmic considerations. Key properties include that all superior highly composite numbers are also highly composite, but the converse does not hold, and they achieve equality in certain upper bounds for the divisor function, such as d(n) < C_\epsilon n^\epsilon for any \epsilon > 0 and suitable constant C_\epsilon. The sequence begins with 2, 6, 12, 60, 120, 360, 2520, 5040, and continues infinitely, listed in OEIS A002201. These numbers have applications in , particularly in deriving explicit bounds for the growth of d(n) and in problems related to the distribution of prime factors.

Definition and Motivation

Formal Definition

A positive integer n is a superior highly composite number if there exists a positive real number \epsilon > 0 such that \frac{d(n)}{n^{\epsilon}} \geq \frac{d(m)}{m^{\epsilon}} for all positive integers m, where d(k) denotes the number of positive divisors of k. Ramanujan's original formulation specified \geq for m < n and strict > for m > n, which is equivalent to the modern global maximization in practice. This inequality characterizes n as achieving the maximum value of the adjusted divisor count d(k)/k^{\epsilon} over all k, for some exponent \epsilon > 0. The ratio d(n)/n^{\epsilon} serves as a measure of divisor density, emphasizing numbers with exceptionally many divisors relative to their size, scaled by the power \epsilon to capture "superior" performance across a range of sensitivities to growth. Superior highly composite numbers constitute a proper of the highly composite numbers, inheriting their property of having more divisors than any smaller positive integer while satisfying the stronger uniformity condition via \epsilon. 1 is sometimes considered the smallest superior highly composite number (as in OEIS A002201), though excluded in some definitions including Ramanujan's original due to lack of prime factors. For appropriate large \epsilon > 1, d(1)/1^{\epsilon} = 1 > d(m)/m^{\epsilon} for all m > 1, since d(m) < m^{\epsilon}.

Historical Motivation

The historical motivation for superior highly composite numbers originates from the quest to characterize natural numbers that possess an exceptionally large number of divisors relative to their magnitude, a key problem in analytic number theory for understanding the extremal behavior of the divisor function d(n). Prior work had established the average order of d(n), as explored by Dirichlet, Voronoi, and Landau, but the maximum or irregular growth remained less understood, with Wigert providing early upper bounds such as d(n) < \exp\left( C \frac{\log n}{\log \log n} \right) for some constant C. Ramanujan sought to identify the numbers achieving these upper bounds in a precise manner, recognizing that such extremal values occur at specific discrete points rather than continuously. This pursuit connects to broader concepts of numerical abundance, where superior highly composite numbers maximize d(n)/n^\epsilon for some \epsilon > 0. These maximizations prove useful in for approximating the growth of divisor-related functions and bounding arithmetic functions in problems involving prime factorizations. Ramanujan's thus provides tools for such theoretical bounds. Intuitively, early interest in such "superior" numbers arose from observations of small integers like 12 (with 6 divisors) and 60 (with 12 divisors), which outperform smaller numbers in divisor count without being excessively large, hinting at an underlying in highly divisible structures. Ramanujan's key insight was that superior highly composite numbers form a countable with explicit rules, enabling rigorous analysis of their role in achieving the normal maximum order of d(n). This structure not only elucidates theoretical bounds but also ties into deeper conjectures, such as the , under which these numbers precisely realize the upper limits for d(n).

Historical Development

Ramanujan's Original Work

Srinivasa Ramanujan introduced superior highly composite numbers in his 1915 paper "Highly Composite Numbers," published in the Proceedings of the London Mathematical Society, where he refined the earlier concept of highly composite numbers by focusing on a stricter subclass distinguished by their maximal value of the normalized by a power of the number relative to all other positive integers. Ramanujan's approach centered on positive integers n for which there exists some \epsilon > 0 such that \frac{d(n)}{n^\epsilon} \geq \frac{d(k)}{k^\epsilon} for all positive integers k, where d(m) is the number of positive divisors of m. This ensures these numbers achieve an optimal density. He constructed such numbers explicitly through their prime , requiring the exponents to form a non-increasing . In a key , Ramanujan proved that every superior highly composite number takes the form p_1^{a_1} p_2^{a_2} \cdots p_k^{a_k}, where p_1 < p_2 < \cdots < p_k are the first k primes and the exponents satisfy a_1 \geq a_2 \geq \cdots \geq a_k \geq 1. This structural condition guarantees the superior property by maximizing the divisor function under the given constraints. Ramanujan provided a table of superior highly composite numbers, with the first few being 2, 6, 12, 60, 120, 360, 840, 1260, 2520, and 5040, illustrating the progressive inclusion of smaller primes with diminishing exponents to sustain the superior property. These initial results laid the groundwork for understanding the discrete nature of numbers optimizing divisor functions.

Post-Ramanujan Advancements

In the 1940s, Leonidas Alaoglu and Paul Erdős provided rigorous proofs confirming several of Ramanujan's conjectures regarding (SHCNs), including their precise canonical form in terms of decreasing exponents in the prime factorization and the infinitude of such numbers. Their work extended the theory by characterizing SHCNs as a subclass of where the ratio of the divisor function to the number raised to any positive power exceeds that of all larger integers, establishing foundational results on their structure. During the 1980s, Jean-Louis Nicolas advanced the study by linking SHCNs to extremal problems in the divisor function and refinements related to the . Concurrently, Guy Robin's 1984 work on inequalities for the sum-of-divisors function \sigma(n) connected colossally abundant numbers—a class analogous to SHCNs but optimizing \sigma(n)/n—to the , showing that \sigma(n) < e^\gamma \log \log n + 0.6483\ldots / \log \log n for all n \geq 5041 if and only if the hypothesis holds, with colossally abundant numbers marking the points where this bound is nearly tight. While SHCNs focus on d(n), these developments highlight parallels in numbers with many divisors or sums of divisors. Computational progress in the 1990s, led by Achim Flammenkamp, extended the enumeration of —which include as a subset—to over 700,000 terms using optimized algorithms that systematically check exponent conditions for primorial-like structures. These efforts facilitated the identification of larger by leveraging computer-assisted verification of divisor maximality. Recent developments up to 2025 have integrated generation with computer algebra systems like , enabling efficient computation of terms with thousands of digits and exploration of their properties in broader contexts. For instance, a 2025 study utilized to derive explicit upper bounds for generalized divisor functions, highlighting their utility in . Ongoing research also connects to unsolved problems, such as the precise density of their distribution among integers, remaining an open challenge in .

Mathematical Properties

Abundancy and Divisor Function

The abundancy index of a positive integer n is the ratio \frac{\sigma(n)}{n}, where \sigma(n) is the sum-of-divisors function, which counts the sum of all positive divisors of n. For a superior highly composite number n with prime factorization n = \prod p_i^{a_i}, the multiplicativity of \sigma yields the explicit formula \frac{\sigma(n)}{n} = \prod_i \frac{1 - p_i^{-(a_i + 1)}}{1 - p_i^{-1}}, where the product is over the distinct primes p_i dividing n, and the exponents a_i are non-increasing with the primes p_i as dictated by the superiority condition. This formula arises from the geometric series summation for each prime power: \sigma(p_i^{a_i}) = 1 + p_i + \cdots + p_i^{a_i} = \frac{p_i^{a_i + 1} - 1}{p_i - 1}, so \frac{\sigma(p_i^{a_i})}{p_i^{a_i}} = \frac{1 - p_i^{-(a_i + 1)}}{1 - p_i^{-1}}. The decreasing exponents in superior highly composite numbers ensure that the product is optimized by favoring small primes with higher powers, leading to a relatively large abundancy index compared to numbers of similar magnitude. The superiority condition on the exponents a_i, which requires that there exists \epsilon > 0 such that \frac{d(n)}{n^\epsilon} \geq \frac{d(k)}{k^\epsilon} for all positive integers k, indirectly constrains the abundancy index to achieve values near the maximal possible order. Specifically, for superior highly composite n, \frac{\sigma(n)}{n} > \log \log n + B for some constant B > 0. More precisely, the maximal order is given by \limsup_{n \to \infty} \frac{\sigma(n)/n}{\log \log n} = e^\gamma, where \gamma \approx 0.57721 is the Euler-Mascheroni constant; while colossally abundant numbers approach this bound, superior highly composite numbers also exhibit high abundancy due to their factorization structure. Superior highly composite numbers achieve local maxima in abundancy because their exponent configuration balances the trade-off between increasing the sum of divisors and the growth in n. To see this, consider modifying n by either increasing an exponent a_j for some prime p_j or multiplying by a new prime q > all p_i. Increasing a_j to a_j + 1 multiplies the abundancy by \frac{1 + 1/p_j^{a_j + 1}}{1 + 1/p_j^{a_j}}, which is greater than 1 but approaches 1 as a_j grows large, while n increases by a factor of p_j; for large enough a_j, this modification decreases the overall \frac{\sigma(n')}{n'}. Similarly, multiplying by a new prime q multiplies the abundancy by $1 + 1/q < 2, but n increases by q; if q is sufficiently large, $1 + 1/q < 1 + \log q / q in logarithmic terms, leading to a net decrease in the ratio. The superiority condition ensures the exponents are set such that any such modification would violate the maximality for the divisor count ratio d(n)/n^\epsilon, and the analogous logarithmic comparison for \sigma(n)/n (replacing d with \sigma in the optimization) shows that the configuration also locally maximizes the abundancy, with the ratio decreasing upon further modifications until the next superior highly composite number.

Multiplicative and Order Properties

Superior highly composite numbers exhibit a strictly increasing order in their sequence, commencing with 1 (sometimes excluded) and proceeding as 2, 6, 12, 60, 120, 360, 2520, 5040, and continuing onward. Each successive number is generated by multiplying the prior term by a prime or a prime power, ensuring the resulting number maximizes the ratio of the divisor function to a power of the number for some positive exponent e. This construction guarantees that the sequence is ordered by magnitude, with no overlaps or repetitions. The set of superior highly composite numbers is not closed under , meaning the product of two such numbers is generally not superior highly composite. For example, both 6 and 12 are superior highly composite, but 6 × 12 = 72 is not, as 72 fails to achieve the required maximization of d(n)/n^e for any e > 0. However, products of specific superior highly composite numbers can yield another under conditions where the aligns with the prescribed decreasing exponent pattern in the prime , such as extending the factorization by adding a new prime factor with exponent 1 or increasing an existing exponent appropriately. Each superior highly composite number possesses a unique prime , with exponents that are non-increasing across the primes in a manner determined by a related to , ensuring no two share identical exponents for the same set of primes. This uniqueness stems from the parametric form introduced by Ramanujan, where each number corresponds to a distinct of exponents optimized for a particular . Superior highly composite numbers have zero in the natural numbers, as their count grows much slower than any positive power of x. The asymptotic number of such numbers up to x is on the order of \frac{\log x}{\log \log x}, reflecting the prime-counting nature of the parameters governing their . Although the is zero, the set has positive logarithmic due to the divergent sum of reciprocals over these numbers.

Prime Factorization Structure

Exponent Conditions

Superior highly composite numbers exhibit a specific structure in their prime . Every such number n can be expressed as n = \prod_{i=1}^k p_i^{a_i}, where p_1 = 2 < p_2 = 3 < \cdots < p_k are the first k primes, and the exponents satisfy a_1 \geq a_2 \geq \cdots \geq a_k \geq 1. This non-increasing sequence of exponents ensures that the factorization prioritizes smaller primes with higher powers, optimizing the divisor-related properties central to the definition. This form is a fundamental characteristic derived from the maximization principles underlying these numbers. The superiority condition imposes strict constraints on these exponents to maintain the number's optimal status. Specifically, for the largest prime p_k in the factorization, introducing a new prime p > p_k with exponent 1 (or higher) or increasing any existing exponent a_i must not produce a multiple m > n such that d(m)/m^\epsilon > d(n)/n^\epsilon for the \epsilon > 0 associated with n. This local maximality ensures that n achieves a peak in the normalized by a power relative to nearby multiples, preventing any simple adjustment from improving the ratio. Such conditions guarantee that superior highly composite numbers form a discrete sequence where each entry dominates in this metric over a range of scales. Ramanujan's criterion provides a precise way to determine these exponents: for a parameter x > 0, the exponent of the prime p is given by a_p = \left\lfloor p^{1/x} - 1 \right\rfloor, with the primes taken as the first k such that p_k \leq 2^x and the sequence is non-increasing. This form arises from the iterative optimization process in constructing the sequence, where exponents are chosen to balance the contribution of each prime while preserving the non-increasing order and overall superiority. The criterion links the structure directly to the broader of highly composite numbers, ensuring consistency across the . For instance, consider n = 12 = 2^2 \times 3^1, an early superior highly composite number. Here, the exponents 2 and 1 are non-increasing, and the configuration satisfies local maximality: multiplying by the next prime 5 to get increases the size but aligns with the sequence's progression, while alternatives like $2^3 \times 3 = [24](/page/24) or $2^2 \times 3^2 = [36](/page/36) do not yield a superior ratio at that scale without violating the conditions. This example illustrates how the exponent rules enforce the number's position in the sequence.

Radices and Their Role

In the theory of superior highly composite numbers (SHCN), the sequence of exponents (a_1, a_2, \dots, a_k) in the prime of an SHCN, where n = 2^{a_1} \cdot 3^{a_2} \cdot \dots \cdot p_k^{a_k} with a_1 \geq a_2 \geq \dots \geq a_k \geq 1 and p_k the k-th prime, encapsulates the structural form of the number. This sequence ensures the exponents decrease or remain constant as larger primes are incorporated. The sequence of exponents plays a central role in defining and generating SHCN by determining the "shape" of their prime factorizations; each SHCN corresponds uniquely to one such sequence, and the superiority property requires that the sequence maximizes d(n)/n^\epsilon for some \epsilon > 0 relative to all smaller numbers. Transitions between sequences of consecutive SHCN typically occur through two mechanisms: appending a new exponent a_{k+1} = 1 for the next prime to extend the sequence, or adjusting existing exponents while preserving the non-increasing order to optimize the divisor function growth. This constructive process ensures that SHCN form a chain where each subsequent sequence builds upon the previous to achieve ever-higher relative divisor counts. Ramanujan illustrated these sequences in his foundational table of SHCN, beginning with the trivial case of 1 corresponding to the empty sequence, followed by (1) for $2 = 2^1, (1,1) for $6 = 2^1 \cdot 3^1, and (2,1) for $12 = 2^2 \cdot 3^1, demonstrating the initial pattern of strict monotonic decrease before allowing plateaus in later entries. These examples highlight how sequences evolve to incorporate more primes only when it enhances the overall divisor density, maintaining the non-increasing property throughout. A sequence of exponents is deemed "superior" precisely when it maximizes the ratio for its fixed length k, balancing the trade-off between including more small primes with higher exponents and adding larger primes with minimal exponents. Extending this to an infinite , where the continues indefinitely across all primes, yields a limiting form tied to the Euler product for the \zeta(s) = \prod_p (1 - p^{-s})^{-1}, as the optimal exponents align with the expansions that bound the maximal order of the .

Enumeration and Examples

Generation Methods

Superior highly composite numbers can be generated using methods based on their prime factorization structure, as described by Ramanujan. Each such number corresponds to a real parameter x > 0, with the form n = \prod_{i=1}^r p_i^{a_i}, where p_i are the first r primes, the exponents a_i are non-increasing positive integers given by a_i = \left\lfloor p_i^{1/x} - 1 \right\rfloor (or adjusted to satisfy boundary conditions), and r is chosen such that p_r \leq 2^x < p_{r+1}. By decreasing x from infinity (yielding n=1) in suitable steps, one obtains all superior highly composite numbers in increasing order. This parametric approach ensures the superiority condition by deriving exponents from logarithmic inequalities that maximize \log d(n) - \epsilon \log n. Computational implementations adapt this by enumerating possible non-increasing exponent sequences over the first primes, verifying the superiority via bounds on the divisor function or direct computation of d(n). Software like and supports arbitrary-precision calculations for factorizations and divisor counts, enabling generation of terms up to very large sizes. For instance, algorithms have computed superior highly composite numbers with hundreds of prime factors. Verification for candidates involves checking that no smaller number achieves a higher d(n)/n^\epsilon for the associated \epsilon, often using theoretical estimates on the growth of d(n) to avoid exhaustive searches.

List of Small Superior Highly Composite Numbers

The superior highly composite numbers form a sequence that grows rapidly, with each term incorporating additional primes or increased exponents in a manner that maximizes the divisor density relative to their size. This list focuses on the first 20 terms (excluding 1, as per OEIS A002201), illustrating their prime factorizations and the number of divisors d(n), which increases with each term. These values highlight the rapid growth in the number of divisors characteristic of these numbers.
IndexNumber nPrime Factorizationd(n)
12$2^12
26$2^1 \times 3^14
312$2^2 \times 3^16
460$2^2 \times 3^1 \times 5^112
5120$2^3 \times 3^1 \times 5^116
6360$2^3 \times 3^2 \times 5^124
72520$2^3 \times 3^2 \times 5^1 \times 7^148
85040$2^4 \times 3^2 \times 5^1 \times 7^160
955440$2^4 \times 3^2 \times 5^1 \times 7^1 \times 11^1100
10720720$2^4 \times 3^2 \times 5^1 \times 7^1 \times 11^1 \times 13^1120
111441440$2^5 \times 3^2 \times 5^1 \times 7^1 \times 11^1 \times 13^1144
124324320$2^5 \times 3^3 \times 5^1 \times 7^1 \times 11^1 \times 13^1192
1321621600$2^5 \times 3^3 \times 5^2 \times 7^1 \times 11^1 \times 13^1288
14367567200$2^5 \times 3^3 \times 5^2 \times 7^1 \times 11^1 \times 13^1 \times 17^1576
156983776800$2^6 \times 3^3 \times 5^2 \times 7^1 \times 11^1 \times 13^1 \times 17^1768
1613967553600$2^6 \times 3^4 \times 5^2 \times 7^1 \times 11^1 \times 13^1 \times 17^11296
17321253732800$2^6 \times 3^4 \times 5^2 \times 7^2 \times 11^1 \times 13^1 \times 17^11728
182248776129600$2^7 \times 3^4 \times 5^2 \times 7^2 \times 11^1 \times 13^1 \times 17^12304
1965214507758400$2^7 \times 3^4 \times 5^2 \times 7^2 \times 11^1 \times 13^1 \times 17^1 \times 19^14608
20195643523275200$2^7 \times 3^5 \times 5^2 \times 7^2 \times 11^1 \times 13^1 \times 17^1 \times 19^16912
The sequence is cataloged as A002201 in the Online Encyclopedia of Integer Sequences (OEIS). Among smaller examples, 5040 stands out as $7!, and earlier terms like 120 align with $5!, underscoring a connection to factorials where the prime exponents match the requirements for superiority without delving into generative methods. This rapid escalation in size—spanning from single digits to over $10^{14} by the 20th term—demonstrates the stringent conditions defining these numbers.

Relations to Other Number Classes

Comparison with Highly Composite Numbers

Highly composite numbers are positive integers n such that the number of d(n) is strictly greater than d(m) for every positive integer m < n. This definition emphasizes maximizing the absolute count of divisors relative to all smaller numbers. In contrast, superior highly composite numbers extend this concept by requiring the existence of some \epsilon > 0 such that d(n)/n^\epsilon \geq d(k)/k^\epsilon for all positive integers k, capturing a scaled maximization of that accounts for the number's magnitude. Every superior highly composite number is also a highly composite number, establishing them as a proper of the highly composite numbers. However, the does not hold; many highly composite numbers fail the stricter condition for superior highly composite numbers. For instance, 36 = $2^2 \times 3^2 is highly composite since d(36) = 9, which exceeds d(m) for all m < 36 (the maximum being 8 for numbers like 24 and 30), but it is not superior highly composite because no \epsilon > 0 satisfies the across all k. Similarly, 24 = $2^3 \times 3 is highly composite with d(24) = 8 > d(m) for m < 24, yet it lacks the required \epsilon for the scaled divisor ratio. This distinction arises from the structural constraints on prime exponents: highly composite numbers allow more flexible decreasing exponents in their prime factorization, while superior highly composite numbers impose tighter bounds tied to the parameter \epsilon, often resulting in exponents that decrease more rapidly and incorporate fewer primes overall. Representative shared examples include 6 = $2 \times 3 and 12 = $2^2 \times 3, both of which satisfy both definitions, with d(6) = 4 > d(m) for m < 6 and the \epsilon-condition holding for appropriate \epsilon. The subset property ensures that superior highly composite numbers inherit the divisor-maximizing trait but refine it to prioritize efficiency in divisor growth relative to size. Colossally abundant numbers are natural numbers n that maximize the ratio \sigma(n)/n^{1+\epsilon} for some \epsilon > 0, where \sigma(n) denotes the sum-of-divisors function, meaning \sigma(n)/n^{1+\epsilon} \geq \sigma(m)/m^{1+\epsilon} for all positive integers m. This definition generalizes the concept of superior highly composite numbers, which maximize the divisor function d(n)/n^{\epsilon} for some \epsilon > 0, where d(n) is the number of divisors of n. In both cases, the parameter \epsilon tunes the trade-off between the multiplicative function ( \sigma(n) or d(n) ) and the size of n, with \epsilon = 0 corresponding to untwisted maximization of \sigma(n)/n or d(n), respectively. The sequences of superior highly composite numbers and overlap completely for the first 15 terms (2, 6, 12, 60, 120, 360, 2520, 5040, 55440, 720720, 1441440, 4324320, 21621600, 367567200, 6983776800), but diverge for larger values; for example, the 16th is 160626866400, while the 16th superior highly composite number is 13967553600. All are superabundant (maximizing \sigma(n)/n relative to smaller numbers), but the converse does not hold. A key shared property is the structure of their prime factorizations: both classes feature non-increasing exponents in the primes, ensuring optimality in their respective maximization criteria, with exponents for explicitly given by k_q(\epsilon) = \left\lfloor \frac{\log \left( \frac{q^{1+\epsilon} - 1}{q^\epsilon (q - 1)} \right)}{\log q} \right\rfloor for each prime q. The sequence of colossally abundant numbers interpolates between superior highly composite numbers (or superabundant numbers, in the as \epsilon \to 0^+) and primorials (products of the first k primes), as smaller \epsilon favors structures closer to primorials with mostly exponent 1, while larger \epsilon aligns more with the denser factorizations of superior highly composite numbers. This parameterized family highlights distinctions in focus: superior highly composite numbers emphasize count for applications in orders of d(n), whereas colossally abundant numbers prioritize abundancy \sigma(n)/n for studying harmonic means of divisors. Both classes find applications in , particularly in bounding the and estimating prime gaps. Colossally abundant numbers equivalently characterize the through the growth of their maximal order, as shown by requiring that the ratio of consecutive such numbers exceeds the primorial logarithm. Additionally, computations of colossally abundant numbers contribute to density estimates for abundant integers, with Deléglise establishing bounds like $0.2474 < A(2) < 0.2480 for the natural of abundant numbers using properties of these sequences.

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