USAAAO 2025, I кръг — Задача 27
USAAAO 2025 - First Round · 8 февруари 2025 г.
Внимание: Бележка към темата
All 30 separately numbered original first-round multiple-choice questions and their matching official explanations/answer letters are retained. The printed explanations for Questions 2 and 3 stop before a promised formula; Question 26 refers to a following triangle absent from its native solution page. No missing expression or diagram is reconstructed. Native scientific discrepancies and ambiguous formula notation remain literal and are explicitly attributed in local source notes. A separate two-page common USAAAO archive constants/reference table is included with its own source identity; it is undated in the catalogue, and its use as the exact 2025 attachment is not established. No separate dated instructions, answer sheet or constants companion is present in the 2025 archive folder. No point total or time limit is printed in these two exam booklets.
Original first-round date and writers
USAAAO 2025 - First Round
February 8th, 2025
Writers: Abhay Bestrapalli, Sidhant Chaliha, Ferdinand, Ved Gund, Hagan Hensley, Yehong Jiang, Alexander Li, Joe McCarty, Lucas Carrit Delgado Pinheiro, Sahil Pontula.
Common archive reference — Table of Physical Constants
This separate common USAAAO archive reference is undated in the catalogue. Its use as the exact 2025 exam attachment is not established.
| Quantity | Symbol | Value |
|---|---|---|
| Electron rest mass | ||
| Proton rest mass | ||
| Electronic charge | ||
| Speed of light in free space | ||
| Permeability of free space | ||
| Permittivity of free space | ||
| Planck’s constant | ||
| Reduced Planck’s constant | ||
| Boltzmann’s constant | ||
| Gas constant | ||
| Molar gas constant | ||
| Avogadro’s number | ||
| Standard molar volume | ||
| Unified atomic mass unit ( scale) | ||
| Mass of hydrogen atom | ||
| Bohr magneton | or | |
| Nuclear magneton | or | |
| Proton magnetic moment | ||
| Neutron magnetic moment | ||
| Bohr radius | ||
| Fine structure constant | ||
| Compton wavelength of electron | ||
| Rydberg’s constant | ||
| Stefan-Boltzmann constant | ||
| Radiation density constant | ||
| Gravitational constant |
Rest masses of some leptons and hadrons in :
0.5110, 105.66, 1777, 134.98, 139.57, 493.7, 497.7, 547, 1865, 1869, p 938.3, n 939.6, 1115.7, 1189, 1193, 1197, 1315, 1321, 1672, , .
| Quark | Charge | Mass () | |||||
|---|---|---|---|---|---|---|---|
| u | 0 | 0 | 0 | 0 | |||
| d | 0 | 0 | 0 | 0 | |||
| c | 0 | 0 | +1 | 0 | 0 | ||
| s | 0 | -1 | 0 | 0 | 0 | ||
| t | 0 | 0 | 0 | 0 | +1 | 174.3 | |
| b | 0 | 0 | 0 | -1 | 0 | 4.2 |
Common archive reference — Astrophysical Data and identities
Astrophysical Data
| Quantity | Symbol | Value |
|---|---|---|
| 1 astronomical unit | AU | |
| 1 parsec | pc | |
| Luminosity of Sun | ||
| Mass of Sun | ||
| Radius of Sun | ||
| Mass of Earth | ||
| Radius of Earth |
Other data and conversion factors
| Quantity | Symbol | Value |
|---|---|---|
| 1 ångstrom | Å | |
| 1 fermi | fm | |
| 1 barn | b | |
| 1 pascal | Pa | |
| 1 standard atmosphere | ||
| Standard acceleration due to gravity | ||
| 1 electron volt | eV | |
| Wavelength of 1 eV photon |
Trigonometrical identities
In a triangle ABC,
and
Prefixes
| Prefix | Name | Factor |
|---|---|---|
| T | tera | |
| G | giga | |
| M | mega | |
| k | kilo | |
| c | centi | |
| m | milli | |
| micro | ||
| n | nano | |
| p | pico | |
| f | femto |
Source note: The common table prints and . The 2025 question14/key15 use 9.81 and key7 uses 6371 km; those original exam values are preserved separately.
Условие
Cosmologists consider three possible universes: universes dominated by baryonic matter (i.e. ordinary matter), universes dominated by radiation, and universes dominated by dark energy (realistically, we consider some mix of the above). An equation written by Alexander Friedmann implies that for a matter-dominated universe, the Hubble parameter is proportional to the square root of that universe’s matter density. In a matter-dominated universe, how does the size of the universe evolve with time ?
(a) constant
(b)
(c)
(d)
(e)
Отговори
- C
Решение
The Hubble parameter relates proper distance to recessional velocity; equivalently, one can see it as relating the size of the universe to the change in that size . Another thing to notice is that since the amount of matter in the universe doesn’t change, its density is . Thus we can write Friedmann’s equation as
Notice we’re being liberal with constants here, because we’re only interested in the asymptotic behavior of . Thus , so we rearrange to obtain
so that .
Answer: C
Теми и трудност
Оценена трудност: 3/5.
Галактики и космология · Разширение на Вселената · Космология
Предпоставки: Гимназиална подготовка, Разширена олимпиадна подготовка
Оригинал в Архива: exam_2025.pdf · официални решения: sol_2025.pdf · допълнителни данни: physical-constants.pdf