From a2a566770655aa4f3ec87b26b7a86cf71cd2025f Mon Sep 17 00:00:00 2001 From: Shanu Nandiraju Date: Mon, 3 Nov 2025 18:23:24 -0800 Subject: [PATCH 1/4] I am adding two new files --- alice.txt | 0 bob.txt | 0 2 files changed, 0 insertions(+), 0 deletions(-) create mode 100644 alice.txt create mode 100644 bob.txt diff --git a/alice.txt b/alice.txt new file mode 100644 index 0000000..e69de29 diff --git a/bob.txt b/bob.txt new file mode 100644 index 0000000..e69de29 From deadccaef4607fd0700ef0cf3883a2273d07f1e0 Mon Sep 17 00:00:00 2001 From: Shanu Nandiraju Date: Mon, 3 Nov 2025 18:30:26 -0800 Subject: [PATCH 2/4] Added experimental txt --- test.txt | 1 + 1 file changed, 1 insertion(+) create mode 100644 test.txt diff --git a/test.txt b/test.txt new file mode 100644 index 0000000..2ef267e --- /dev/null +++ b/test.txt @@ -0,0 +1 @@ +some content From 22908d0cdb7f5eba70c9fd121d57c23421df18ed Mon Sep 17 00:00:00 2001 From: Shanu Nandiraju Date: Mon, 3 Nov 2025 18:51:14 -0800 Subject: [PATCH 3/4] added alpher branches content --- gamow.txt | 8 ++++++-- 1 file changed, 6 insertions(+), 2 deletions(-) diff --git a/gamow.txt b/gamow.txt index 5165600..33f414c 100644 --- a/gamow.txt +++ b/gamow.txt @@ -1,4 +1,6 @@ http://en.wikipedia.org/wiki/Alpher–Bethe–Gamow_paper + + In physical cosmology, the Alpher–Bethe–Gamow paper, or αβγ paper, was created by Ralph Alpher, then a physics PhD student, and his advisor George Gamow. The work, which would become the subject of Alpher's PhD dissertation, argued that the Big Bang would create hydrogen, helium and heavier elements in the correct proportions to explain their abundance in the early universe. While the original theory neglected a number of processes important to the formation of heavy elements, subsequent developments showed that Big Bang nucleosynthesis is consistent with the observed constraints on all primordial elements. Gamow humorously decided to add the name of his friend—the eminent physicist Hans Bethe—to this paper in order to create the whimsical author list of Alpher, Bethe, Gamow, a play on the Greek letters α, β, and γ (alpha, beta, gamma). Bethe was listed in the article as "H. Bethe, Cornell University, Ithaca, New York." In his 1952 book, The Creation of the Universe, Gamow explained Hans Bethe's association with the theory thus: @@ -6,7 +8,9 @@ Gamow humorously decided to add the name of his friend—the eminent physicist H Alpher, at the time only a graduate student, was generally dismayed by the inclusion of Bethe's name on this paper. He felt that the inclusion of another eminent physicist would overshadow his personal contribution to this work and prevent him from receiving proper recognition for such an important discovery. He expressed resentment over Gamow's decision as late as 1999.[ The theory originally proposed that all atomic nuclei are produced by the successive capture of neutrons, one mass unit at a time. However, later study challenged the universality of the successive capture theory. No element was found to have a stable isotope with an atomic mass of five or eight. Physicists soon noticed that these mass gaps would hinder the production of elements beyond helium. Just as it's impossible to climb a staircase one step at a time when one of the steps is missing, this discovery meant that the successive capture theory could not account for higher elements. -It was eventually recognized that most of the heavy elements observed in the present universe are the result of stellar nucleosynthesis (http://en.wikipedia.org/wiki/Stellar_nucleosynthesis) in stars, a theory largely developed by Bethe. + +http://en.wikipedia.org/wiki/Stellar_nucleosynthesis +Stellar nucleosynthesis is the collective term for the nuclear reactions taking place in stars to build the nuclei of the elements heavier than hydrogen. Some small quantity of these reactions also occur on the stellar surface under various circumstances. For the creation of elements during the explosion of a star, the term supernova nucleosynthesis is used. Text is available under the Creative Commons Attribution-ShareAlike License; additional terms may apply. See Terms of Use for details. -http://creativecommons.org/licenses/by-sa/3.0/ +http://creativecommons.org/licenses/by-sa/3.0/ \ No newline at end of file From f52c3352eb793e8b68a64610e717719c0d6165a8 Mon Sep 17 00:00:00 2001 From: Shanu Nandiraju Date: Mon, 3 Nov 2025 18:54:45 -0800 Subject: [PATCH 4/4] fixed bug in the python code --- some_python_code.py | 2 +- 1 file changed, 1 insertion(+), 1 deletion(-) diff --git a/some_python_code.py b/some_python_code.py index 7cad6de..da96ab0 100644 --- a/some_python_code.py +++ b/some_python_code.py @@ -1,3 +1,3 @@ arr = [1, 3, 6, 3, 10, 20] -for i in range(len(arr) + 1): +for i in range(len(arr)): print(arr[i]) \ No newline at end of file