Research Paper Undergraduate 1,334 words

Evolution and the Big Bang Theory: Origins Explained

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Abstract

This paper examines the Big Bang theory as a scientific explanation for the origin of the universe, tracing the progression from an initial singularity approximately 13.7 billion years ago to the expanding cosmos observed today. It reviews key supporting evidence, including Hubble's Law, Cosmic Microwave Background radiation, and the abundance of light elements. The paper also addresses notable scientific dissent from researchers such as Robert Gentry and Sir Fred Hoyle, and explores the philosophical and religious dimensions of cosmogony — the study of the universe's origin — concluding that the Big Bang theory remains a compelling, if debated, framework for addressing humanity's deepest metaphysical questions.

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What makes this paper effective

  • The paper moves logically from a foundational definition of the Big Bang to supporting evidence, then to dissent, and finally to philosophical implications — creating a clear, reader-friendly progression.
  • It balances scientific explanation with broader cultural and religious context, making an abstract cosmological topic accessible to a general academic audience.
  • The inclusion of named scientists, specific discoveries (such as Penzias and Wilson's Nobel Prize-winning detection of CMB radiation), and dated evidence lends credibility and specificity to the argument.

Key academic technique demonstrated

The paper demonstrates the technique of presenting a dominant scientific theory, acknowledging legitimate scholarly dissent, and then situating both within a broader philosophical framework. Rather than advocating for one position, it maps the landscape of the debate — a useful strategy in introductory-level science and humanities writing.

Structure breakdown

The paper opens by framing the Big Bang as an answer to metaphysical questions, then dedicates its longest section to the theory's mechanics and supporting evidence. A shorter section addresses alternative scientific models. The penultimate section addresses the religion–science intersection, and the conclusion synthesizes the debate, reaffirming the theory's value while acknowledging its open questions. This five-part structure suits an introductory research paper format.

Introduction to the Big Bang Theory

The metaphysical questions that have haunted humanity since the dawn of civilization are perhaps addressed by the theory of evolution and the Big Bang theory. The Big Bang theory regarding the origin of the universe was formulated approximately 50 years ago and soon became the prevailing framework of the evolutionary establishment, though it has faced considerable opposition.

The Big Bang theory is an effort to explain what happened at the very start of our universe. Research in astronomy and physics has shown that our universe did indeed have a beginning. Before this beginning, there was nothing; after it, our universe came to be. The Big Bang theory attempts to explain what happened during and after the moment that the universe began.

According to the theory, the universe came into existence as a "singularity" approximately 13.7 billion years ago. Singularities are zones that defy our current understanding of physics. They are believed to exist at the core of black holes — areas of intense gravitational pressure so extreme that finite matter is compressed into infinite density. These zones of infinite density are known as singularities. Research suggests that the universe was once an infinitesimally small, infinitely hot, and infinitely dense entity. How it came to be what it is today, however, remains difficult to prove.

After the universe's initial appearance, it appears to have inflated — the "Big Bang" — then expanded and cooled, growing from a very small and very hot point to the size and temperature of the universe we observe today. The universe continues to expand and cool, and humans exist within it, living on a unique planet that circles a star clustered together with several hundred billion other stars in a galaxy. This is the essence of the Big Bang theory.

Research on Evolution and the Big Bang Theory

According to the Big Bang theory, approximately 10 to 20 billion years ago, all of the matter and energy of the universe was compressed into one cosmic egg — a plasma ball consisting of sub-atomic particles and radiation (Gish, 1991). Nobody understands where the cosmic egg came from, or how it got there; it simply appears to have existed. For some inexplicable reason, the cosmic egg exploded. As matter and radiation expanded, so the theory holds, the universe cooled sufficiently for elements to form. Protons and electrons combined to form hydrogen of atomic weight one, and neutrons were captured to form helium of atomic weight four. Most of the gas that formed was hydrogen. These gases are believed to have expanded radially in all directions throughout the universe until they were so highly dispersed that a very low vacuum and temperature existed. No oxygen, nitrogen, phosphorus, carbon, sulfur, copper, iron, nickel, uranium, or other heavier elements were yet present. The universe was composed essentially of hydrogen gas.

Then, somehow, the molecules of gas expanding outward at enormous speed began to collapse inward in localized areas due to gravitational attraction (Gish, 1991). Molecules within a space of roughly six trillion miles in diameter collapsed to form each star; approximately 100 billion stars collected to form each of the roughly 100 billion galaxies in the universe. Our own solar system formed approximately five billion years ago from a cloud of dust and gas made up of the exploded remnants of formerly existing stars.

There has been a great deal of research supporting the Big Bang theory. Most researchers agree that the universe had a beginning. Additionally, galaxies appear to be moving away from us at speeds proportional to their distance — a phenomenon known as Hubble's Law, named after astronomer Edwin Hubble, who discovered it in 1929. This observation supports the expansion of the universe and implies that it was once far more compacted.

Furthermore, if the universe was initially extremely hot, as the Big Bang theory suggests, scientists should be able to find evidence of that primordial heat. In 1965, radio astronomers Arno Penzias and Robert Wilson discovered a 2.725-degree Kelvin (approximately -454.765°F / -270.425°C) Cosmic Microwave Background radiation (CMB) that pervades the observable universe. This is widely regarded as the remnant that scientists had been seeking. Penzias and Wilson shared the 1978 Nobel Prize in Physics for this discovery.

Finally, the abundance of the light elements hydrogen and helium found throughout the observable universe is also considered strong support for the Big Bang model of origins.

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Scientific Dissent and Alternative Models · 110 words

"Researchers who challenge the standard Big Bang theory"

Religion and the Big Bang Theory · 80 words

"Intersection of cosmogony, religion, and science"

Conclusion

There are many misconceptions surrounding the Big Bang theory. For example, we tend to imagine a giant explosion. Experts, however, say that there was no explosion; there was — and continues to be — an expansion. Rather than imagining a balloon popping and releasing its contents, one should imagine a balloon expanding: an infinitesimally small balloon growing to the size of our current universe.

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Key Concepts in This Paper
Big Bang Theory Singularity Hubble's Law CMB Radiation Expanding Universe Cosmic Origins Science and Religion Cosmogony Gravitational Collapse Einstein's Relativity
Cite This Paper
PaperDue. (2026). Evolution and the Big Bang Theory: Origins Explained. PaperDue. https://paperdue.com/study-guide/evolution-big-bang-theory-origins-65359

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