08 September 2023

Cosmic Microwave Background Radiation (CMB), the Observable and Non-Observable Universes, and Their Respective Distances

Soumendra Nath Thakur* Priyanka Samal1 Onwuka Frederick2

Guided by the monumental Big Bang theory, this research paper embarks on a captivating exploration of cosmic vistas, delving into the enigmatic origins of the universe, the enigmatic cosmic microwave background radiation (CMBR), and the intricate interplay between observable and non- observable universes. Intricately woven into this cosmic fabric are the pioneering observations of the Cosmic Background Explorer (COBE), the Wilkinson Microwave Anisotropy Probe (WMAP), and the Planck satellite. These scientific sentinels have charted the CMBR's temperature fluctuations, offering windows into the universe's earliest epochs. COBE's revelation of temperature variations in 1992 solidified the Big Bang theory. WMAP, launched in 2001, delved deeper, unraveling the CMBR's anisotropies and refining cosmic parameter measurements. The Planck satellite, soaring into space in 2009, etched precision onto the cosmic canvas, encapsulating the universe's age, composition, andevolutionary trajectory.This narrative unfolds the epic tale of emergence from a minuscule singularity and the subsequent grand cosmic inflation. At the heart of this cosmic odyssey lies the CMBR, a whispered echo from the universe's primordial dawn that unfolds the saga of its early epochs and the daring journey of the first light. 


The tapestry of time itself is probed, unveiling the temporal intricacies of these realms shaped by phenomena like redshift and the relentless cosmic expansion. Across a 13.8-billion-year narrative, our observational prowess extends to reveal galaxies within a 46.5 billion light-year radius—43% visible, 57% veiled. Anchored by elegant mathematical frameworks like Hubble's Law, this journey through cosmic mechanicsnurtures the growth of understanding and discovery. An expedition both poetic andscientific, this paper unearths the blueprint of the universe, resonating with themes ofcuriosity and evolution that span unfathomable eons. 


07 September 2023

The Significance of Origins in Spacetime (v3). Integrating Local Time with Cosmic Time:

Soumendra Nath Thakur

ORCiD: 0000-0003-1871-7803

07 September 2023

1. Abstract:

In the realm of spacetime, the concept of origin plays a pivotal role, particularly when dealing with the dimensions of space and time. This comprehensive study delves into the critical importance of differentiating between the origins of spatial coordinates (x, y, z) and the temporal dimension 't' within the framework of spacetime.
Furthermore, it illuminates the intriguing relationship between 'local time' (t) and 'cosmic time' (t₀) and their measurements relative to distinct reference points. The research explores how 't' can have its own unique origin, separate from spatial coordinates, and how this 'local time' connects with the overarching concept of 'cosmic time' governing the universe.
This multidimensional analysis enhances our understanding of the profound interplay between space and time, highlighting the fundamental fabric of the universe.

2. Introduction:

Spacetime, a foundational concept in the realm of physics, seamlessly intertwines the dimensions of space and time, forming the fabric of our universe. Within this intricate tapestry, the selection of an origin for the temporal dimension 't' takes on profound significance. 't' is often measured relative to what we might term the "origin of time" or "observer's frame." This origin can be defined by a pivotal event, the commencement of an experiment, or the establishment of a specific coordinate system.

It is imperative to distinguish the origin for time 't' from the origin for spatial coordinates (x, y, z), which is typically represented as 'o.' These origins serve disparate functions. The spatial origin 'o' serves as the foundational reference point for measuring distances within the spatial dimensions, while the temporal origin 't' serves as the reference point for measuring intervals of time.

3. Separate Origins: A Prerequisite:

Within the framework of a comprehensive description of spacetime, the existence of distinct origins for space and time becomes indispensable. Consider a scenario where the origin for spatial coordinates (x, y, z) is 'o,' defined precisely at coordinates (0, 0, 0). Conversely, the origin for time 't' might commence at a specific moment, such as the inception of an experiment or another precisely defined reference time.

4. A complete representation thus entails differentiating these origins:

Imagine an event 'p' positioned at coordinates (x1, y1, z1, t₁) within the spacetime coordinate system. Spatial coordinates (x1, y1, z1) are measured in relation to the origin 'o' in the spatial dimensions, while 't₁' is measured from its own distinct origin in the temporal dimension. This temporal origin could correspond to the initiation of an experiment or any other momentous reference point.

This separation of origins is fundamental for achieving precision in understanding both where an event occurs in space and when it transpires in time.

5. Time ’t₁’ with Cosmic Origin t₀:

Event 'p' is located at coordinates (x₁, y₁, z₁, t₁) within the (x, y, z) system, originating from 'o' in the spatial dimensions. Simultaneously, the time coordinate 't₁' originates from 't₀' within the cosmic dimension.

In this representation, we find an event labeled as 'p' situated within the three-dimensional spatial coordinate system (x, y, z), with 'o' as its foundational reference point for measuring spatial distances and positions.

However, the temporal dimension, as denoted by the time coordinate 't₁,' operates with its own unique reference point. This reference point is identified as 't₀,' which is a reference deeply entwined with the cosmic dimension of time. Effectively, while spatial measurements are anchored in reference to 'o,' temporal measurements find their basis in 't₀,' underlining the fundamental distinction between the origins of space and time.

This presentation serves to underscore the crucial differentiation between the spatial origin 'o' and the cosmic time origin 't₀,' emphasizing the principle that time is not measured from the same reference point as spatial dimensions.

6. Mathematical Presentation:

Spatial Coordinates:

The spatial position of event 'p' in the (x, y, z) coordinate system is represented as follows:

  • x1 represents the displacement along the x-axis.
  • y1 represents the displacement along the y-axis.
  • z1 represents the displacement along the z-axis.

Temporal Coordinate:

The temporal dimension, represented by 't₁,' is measured relative to its own origin, 't₀':

t1  denotes the time coordinate of event 'p' and is measured from 't₀.'

In mathematical notation:

Spatial Coordinates:

(x1,y1,z1) represents the spatial position of event 'p' relative to the spatial origin 'o' in the (x, y, z) coordinate system.

Temporal Coordinate:

t1 represents the time coordinate of event 'p' relative to the cosmic time origin 't₀.'

Spatial Origin on Earth:

Clock 'c₁' is located at coordinates (x1,y1,z1,t1)  in the (x, y, z) system, originating from 'o₁' in spatial dimensions, which is located at mean sea level on Earth, defined with coordinates (0,0,0) = (x1,y1,z1) in the (x, y, z) system with 'o₁.'

Introduction of Elevated System:

Another clock 'c₂' is located at coordinates (x1,y1,z1,t2) in an elevated (x, y, z) system with the present origin 'o₂,' which initially originated in the (x, y, z) system with origin 'o₁' until elevated to a height 'h' meters from 'o₁.'

Spatial Origin at a Height:

Clock 'c₂' is located at coordinates (x2,y2,z2,t2) in the (x, y, z) system, originating at 'o₂' in spatial dimensions, which is located at a height 'h' meters from 'o₁,' defined with coordinates (0,0,h) = (x2,y2,z2) in the (x, y, z) system with 'o₂.' Initially, origin 'o₂' or the clock 'c₂' earlier originated and merged with origin 'o₁,' at an actual distance of (o₂ - o₁) = h meters.

Both temporal origins 'o₁' and 'o₂' of these coordinate systems for the respective clocks 'c₁' and 'c₂' are in a common scale of cosmic time relative to 't₀,' while origins 'o₁' and 'o₂' serve as the reference points for measuring distances and positions within the spatial dimensions.

However, the temporal dimension, represented by the time coordinates 't₁' and 't₂,' operates with a common and distinct reference point. The origin for 't₁' and 't₂' is specified as 't₀,' which is a reference associated with the cosmic dimension of time. In essence, while spatial measurements are made relative to 'o₁' and 'o₂,' temporal measurements are made relative to 't₀,' highlighting the separation between spatial and temporal origins.

7. In Conclusion: 

The exploration of spatial origins on Earth and the introduction of elevated coordinate systems underscore the critical role of distinguishing between spatial and temporal dimensions within the context of spacetime.

The study begins by establishing 'o₁' as the spatial origin at mean sea level on Earth, serving as the reference point for measuring distances in the (x, y, z) system. 'c₁' is located at coordinates (x1,y1,z1,t1) relative to this spatial origin.

The introduction of the elevated system, represented by 'c₂,' introduces the concept of an elevated spatial origin 'o₂.' Initially, 'o₂' originates within the same (x, y, z) system as 'o₁' and is later elevated to a height 'h' meters above 'o₁.' Consequently, 'c₂' is situated at coordinates (x2,y2,z2,t2) in this elevated system, defined relative to 'o₂' and located 'h' meters above 'o₁.'

The critical distinction lies in the temporal dimension, represented by 't₁' and 't₂.' Both 't₁' and 't₂' operate within a common scale of cosmic time relative to 't₀,' emphasizing their shared temporal framework. However, the reference points for measuring distances and positions within the spatial dimensions are 'o₁' and 'o₂,' highlighting the separation between spatial and temporal origins.

This research accentuates the fundamental concept that while spatial measurements are made relative to spatial origins, temporal measurements are made relative to a distinct temporal origin, 't₀,' associated with the cosmic dimension of time. This distinction is paramount in understanding the intricate interplay between space and time within the framework of spacetime.

In essence, the significance of spatial and temporal origins elucidates the complexity of spacetime, enriching our comprehension of the fundamental fabric of our universe. 

8. References:

[1] Einstein, A. (1915). General Theory of Relativity. Annalen der Physik, 354(7), 769-822.

[2] Hawking, S. W. (1988). A Brief History of Time: From the Big Bang to Black Holes. Bantam Books.

[3] Minkowski, H. (1908). Space and Time: An Introduction to the Special Theory of Relativity. Princeton University Press.

[4] Penrose, R. (1965). Gravitational Collapse and Space-Time Singularities. Physical Review Letters, 14(3), 57-59.

[5] Thorne, K. S., & Wheeler, J. A. (1973). Gravitation. W. H. Freeman and Company.


05 September 2023

The Significance of Origins in Spacetime (v2). Integrating Local Time with Cosmic Time:

 Soumendra Nath Thakur

ORCiD: 0000-0003-1871-7803

05 September 2023

1. Abstract:

In the realm of spacetime, the concept of origin takes on a critical role, especially when dealing with the dimensions of space and time. This article explores the importance of distinguishing between the origins of spatial coordinates (x, y, z) and the temporal dimension 't' within the context of a complete spacetime description. It emphasizes the need to recognize that 't' often has its own distinct origin, separate from the spatial coordinates. 

Additionally, this article sheds light on the intriguing relationship between 'local time' (t) and 'cosmic time' (t₀), and how they are measured relative to different reference points. It delves into the idea that 't' can begin at specific moments or events, known as 'local time,' and elucidates how this local time relates to the broader concept of 'cosmic time' that governs the universe.

2. Introduction:

Spacetime, a fundamental concept in the realm of physics, combines the dimensions of space and time into a seamless continuum. In this intricate interplay, the choice of origin for the temporal dimension 't' becomes a pivotal consideration. Often, 't' is measured relative to what we might term the "origin of time" or "observer's frame." This origin could be defined by a significant event, the initiation of an experiment, or the establishment of a specific coordinate system.

It's crucial to distinguish the origin for time 't' from the origin for spatial coordinates (x, y, z), often represented as 'o.' These origins serve distinct purposes. The spatial origin 'o' sets the reference point for measuring distances in the spatial dimensions, while the temporal origin 't' sets the reference point for measuring time intervals.

3. Separate Origins: A Prerequisite:

In the context of a comprehensive spacetime description, separate origins for space and time are practically indispensable. Consider the following scenario: the origin for spatial coordinates (x, y, z) is 'o,' defined with coordinates (0, 0, 0). In contrast, the origin for time 't' may commence at a specific moment, such as the inception of an experiment or another reference time.

4. A complete representation thus entails differentiating these origins:

Event 'p' is positioned at coordinates (x1, y1, z1, t₁) in the spacetime coordinate system. Spatial coordinates (x1, y1, z1) are measured relative to the origin 'o' for spatial dimensions, while 't₁' is measured from its own distinct origin for time. This temporal origin could be the initiation of an experiment or any other significant reference moment.

This separation of origins allows for a precise understanding of where an event occurs in space and when it transpires in time.

5. Time ’t₁’ with Cosmic Origin t₀:

Event 'p' is located at coordinates (x₁, y₁, z₁, t₁) in the (x, y, z) system, originating from 'o' in spatial dimensions, while the time coordinate 't₁' originates from 't₀' in the cosmic dimension.

In this presentation, we have an event denoted as 'p' situated in the three-dimensional spatial coordinate system (x, y, z) with an origin labeled as 'o.' This origin 'o' serves as the reference point for measuring distances and positions within the spatial dimensions.

However, the temporal dimension, represented by the time coordinate 't₁,' operates with a distinct reference point. The origin for 't₁' is specified as 't₀,' which is a reference associated with the cosmic dimension of time. In essence, while spatial measurements are made relative to 'o,' temporal measurements are made relative to 't₀,' highlighting the separation between spatial and temporal origins.

This presentation distinguishes between the spatial origin 'o' and the cosmic time origin 't₀,' underlining the concept that time is not measured from the same reference point as spatial dimensions.

6. Mathematical Presentation:

Spatial Coordinates:

Spatial position of event 'p' in the (x, y, z) coordinate system:

x₁ represents the displacement along the x-axis.

y₁ represents the displacement along the y-axis.

z₁ represents the displacement along the z-axis.

Temporal Coordinate:

The temporal dimension, represented by 't₁,' is measured relative to its own origin, 't₀':

t₁ denotes the time coordinate of event 'p' and is measured from 't₀.'

In mathematical notation:

Spatial Coordinates:

(x1, y1, z1) represents the spatial position of event 'p' relative to the spatial origin 'o' in the (x, y, z) coordinate system.

Temporal Coordinate:

t₁ represents the time coordinate of event 'p' relative to the cosmic time origin 't₀.'

7. Conclusion:

The choice of origin in spacetime is a fundamental consideration, distinguishing the reference points for spatial coordinates from the temporal dimension 't.' A comprehensive spacetime description necessitates separate origins for space and time, ensuring precision in locating events in both dimensions.

This mathematical representation captures the separation of origins between spatial and temporal dimensions, as described in the presentation.

The relationship between 'local time' and 'cosmic time' underscores the nuanced nature of temporal measurement. 'Local time' serves as a dynamic, observer-dependent component, while 'cosmic time' remains an unchanging, universal entity. Recognizing the significance of origins in spacetime elucidates the intricate interplay between space and time and deepens our understanding of the fundamental fabric of the universe.

8. References:

[1] Einstein, A. (1915). General Theory of Relativity. Annalen der Physik, 354(7), 769-822.

[2] Hawking, S. W. (1988). A Brief History of Time: From the Big Bang to Black Holes. Bantam Books.

[3] Minkowski, H. (1908). Space and Time: An Introduction to the Special Theory of Relativity. Princeton University Press.

[4] Penrose, R. (1965). Gravitational Collapse and Space-Time Singularities. Physical Review Letters, 14(3), 57-59.

[5] Thorne, K. S., & Wheeler, J. A. (1973). Gravitation. W. H. Freeman and Company.

GPS and Relativity, Relativistic Error Effect on the GPS Time...,

explain in detail the formulas for the relativistic corrections to be implemented in high-speed aircraft, or when using other

Analysis of Relativistic Error Effect on the GPS Time and the Receiver Position Accuracy

The Significance of Origins in Spacetime (v1). Integrating Local Time with Cosmic Time:

Soumendra Nath Thakur

ORCiD: 0000-0003-1871-7803

05 September 2023

1. Abstract:

In the realm of spacetime, the concept of origin takes on a critical role, especially when dealing with the dimensions of space and time. This article explores the importance of distinguishing between the origins of spatial coordinates (x, y, z) and the temporal dimension 't' within the context of a complete spacetime description. It emphasizes the need to recognize that 't' often has its own distinct origin, separate from the spatial coordinates.

Additionally, this article sheds light on the intriguing relationship between 'local time' (t) and 'cosmic time' (t), and how they are measured relative to different reference points. It delves into the idea that 't' can begin at specific moments or events, known as 'local time,' and elucidates how this local time relates to the broader concept of 'cosmic time' that governs the universe.

2. Introduction:

Spacetime, a fundamental concept in the realm of physics, combines the dimensions of space and time into a seamless continuum. In this intricate interplay, the choice of origin for the temporal dimension 't' becomes a pivotal consideration. Often, 't' is measured relative to what we might term the "origin of time" or "observer's frame." This origin could be defined by a significant event, the initiation of an experiment, or the establishment of a specific coordinate system.

It's crucial to distinguish the origin for time 't' from the origin for spatial coordinates (x, y, z), often represented as 'o.' These origins serve distinct purposes. The spatial origin 'o' sets the reference point for measuring distances in the spatial dimensions, while the temporal origin 't' sets the reference point for measuring time intervals.

3. Separate Origins: A Prerequisite:

In the context of a comprehensive spacetime description, separate origins for space and time are practically indispensable. Consider the following scenario: the origin for spatial coordinates (x, y, z) is 'o,' defined with coordinates (0, 0, 0). In contrast, the origin for time 't' may commence at a specific moment, such as the inception of an experiment or another reference time.

4. A complete representation thus entails differentiating these origins:

Event 'p' is positioned at coordinates (x1, y1, z1, t) in the spacetime coordinate system. Spatial coordinates (x1, y1, z1) are measured relative to the origin 'o' for spatial dimensions, while 't' is measured from its own distinct origin for time. This temporal origin could be the initiation of an experiment or any other significant reference moment.

This separation of origins allows for a precise understanding of where an event occurs in space and when it transpires in time.

5. Local Time vs. Cosmic Time:

An intriguing facet of spacetime is the duality between 'local time' (t) and 'cosmic time' (t). 'Local time' refers to the temporal dimension that originates at specific moments or events. It progresses from these local origins and marks the duration of events within specific frames of reference.

On the other hand, 'cosmic time' represents the broader temporal fabric governing the entire universe. It is akin to a cosmic clock that ticks uniformly, independent of local variations. 'Cosmic time' permeates all of spacetime, providing a universal reference for temporal measurement.

6. Relationship between 'Local Time' and 'Cosmic Time':

The relationship between 'local time' and 'cosmic time' is a crucial aspect of spacetime. 'Local time' (t) is inherently tied to the observer's.

Conversely, 'cosmic time' (t) remains constant across the universe. It serves as the ultimate arbiter of temporal progression, unifying disparate regions of spacetime under a single temporal framework.

In summary, 'local time' and 'cosmic time' are intimately connected yet distinct in their origins and implications. 'Local time' emerges from specific events or reference points, while 'cosmic time' transcends local variations, providing a universal timekeeping system for the cosmos.

7. Mathematical Presentation:

In the context of spacetime, the choice of origin for the time dimension ’t’ is an important consideration, and it's not necessarily the same as the origin 'o' for the spatial coordinates (x, y, z).

Origin of Time ’t’:

The origin or reference point for the time dimension ’t’ is typically not explicitly mentioned. In physics, time is often measured relative to a different reference point, often referred to as the "origin of time." This reference point could be the moment of an event, such as the start of an experiment or the origin of a particular coordinate system.

Separate Origins:

In practice, the origin for time ’t’ is distinct from the origin 'o' for spatial coordinates (x, y, z). These origins serve different purposes. The origin for spatial coordinates defines the reference point for measuring distances in space, while the origin for time defines the reference point for measuring time intervals.

So, in the context of a complete spacetime description, one would typically have separate origins for space and time.

For example:

Origin for spatial coordinates (x, y, z) is 'o' with coordinates (0, 0, 0).

Origin for time ’t’ may be a specific moment (e.g., the start of an experiment) or another reference time.

In the statement, it's important to clarify that 'o' represents the origin for spatial coordinates (x, y, z), and if 't' is included as the fourth coordinate, it should be measured relative to its own distinct origin for time.

So, the complete representation might be something like:

Event 'p' is located at coordinates (x1, y1, z1, t) in the spacetime coordinate system. The spatial coordinates (x1, y1, z1) are measured relative to the origin 'o' for spatial coordinates, and 't' is measured relative to its own origin for time, which could be the start of an experiment or another reference moment.

This way, it is clearly differentiated between the origins for spatial and temporal dimensions.

While in scientific representations:

In the context of scientific representations, it's important to clarify the reference frame and assumptions being made. If the reference to time ’t’ in a scenario where one wants to consider its origin as the starting point of an event or measurement, he can make that explicit in his representation.

Here's how one can represent time ’t’ with its axial position in the (x, y, z) coordinate system with an origin at its beginning:

Spatial Coordinates of 'p': 

The spatial position of point 'p' is represented by its coordinates (x1, y1, z1) with respect to the origin 'o' in the (x, y, z) coordinate system. These coordinates describe where 'p' is located in space.

Time ’t’ with an Origin:

To represent time ’t’ with its axial position, one can specify that ’t’ starts at a particular moment or event, and it increases as time progresses. One should include this information as part of his representation:

The x-coordinate (x1) tells how far 'p' is from the origin 'o' along the x-axis.

The y-coordinate (y1) tells how far 'p' is from 'o' along the y-axis.

The z-coordinate (z1) tells how far 'p' is from 'o' along the z-axis.

The time ’t’ is measured from a specified origin or starting point and indicates when the event associated with 'p' occurs.

The representation might look like this:

Event 'p' is located at coordinates (x1, y1, z1) in the (x, y, z) coordinate system, with time ’t’ starting at a specific origin and increasing from that point. 

By specifying that ’t’ starts at a particular origin; one emphasizes the reference point for time measurement within his chosen coordinate system. This approach aligns with the concept of time as a progression from a defined starting moment.

8. Conclusion:

The choice of origin in spacetime is a fundamental consideration, distinguishing the reference points for spatial coordinates from the temporal dimension 't.' A comprehensive spacetime description necessitates separate origins for space and time, ensuring precision in locating events in both dimensions.

The relationship between 'local time' and 'cosmic time' underscores the nuanced nature of temporal measurement. 'Local time' serves as a dynamic, observer-dependent component, while 'cosmic time' remains an unchanging, universal entity. . 'Local time' and 'cosmic time' are intimately connected yet distinct in their origins and implications

Recognizing the significance of origins in spacetime elucidates the intricate interplay between space and time and deepens our understanding of the fundamental fabric of the universe.