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Generalizations of Holders and some related integral inequalities on   fractal space

Generalizations of Holders and some related integral inequalities on fractal space

: ๋ณธ ์—ฐ๊ตฌ๋Š” ์ˆ˜ํ•™์  ์ด๋ก  ์ค‘ ํ•˜๋‚˜์ธ ํ˜ธ๋”(Hรถlder) ๋ถˆํ‰๋“ฑ์— ์ดˆ์ ์„ ๋งž์ถ”๊ณ , ์ด๋ฅผ ์ง€์—ญ ๋ถ„์ˆ˜ ๋ฏธ์ ๋ถ„ํ•™์ด๋ผ๋Š” ๋ณต์žกํ•œ ์ˆ˜ํ•™ ์˜์—ญ์œผ๋กœ ํ™•์žฅํ•˜๋Š” ๋ฐ ์ฃผ๋ ฅํ•˜๊ณ  ์žˆ๋‹ค. ํ˜ธ๋” ๋ถˆํ‰๋“ฑ์€ ํ•จ์ˆ˜ ๊ณต๊ฐ„์—์„œ์˜ ๋ฒกํ„ฐ ๋‚ด์ ๊ณผ ๊ด€๋ จ๋œ ์ค‘์š”ํ•œ ๊ฒฐ๊ณผ๋กœ, ๋‹ค์–‘ํ•œ ์‘์šฉ ๋ถ„์•ผ์—์„œ ํ™œ์šฉ๋˜๊ณ  ์žˆ๋‹ค. 1. ํ˜ธ๋” ๋ถˆํ‰๋“ฑ์˜ ์ผ๋ฐ˜ํ™” ๋…ผ๋ฌธ์—์„œ๋Š” ๋จผ์ € ๊ธฐ์กด์˜ ํ˜ธ๋” ๋ถˆํ‰๋“ฑ์„ ๋ณต์Šตํ•˜๊ณ  ์ด๋ฅผ ์ง€์—ญ ๋ถ„์ˆ˜ ๋ฏธ์ ๋ถ„ํ•™์— ์ ์šฉํ•˜๊ธฐ ์œ„ํ•œ ์ƒˆ๋กœ์šด ํ˜•ํƒœ์˜ ๋ถˆํ‰๋“ฑ์„ ์ œ์‹œํ•œ๋‹ค. ํŠนํžˆ, pโ‚๊ณผ pโ‚‚๊ฐ€ ์–‘์ˆ˜์ผ ๋•Œ์™€ 0 < pโ‚ < 1์ด๊ณ  pโ‚‚ < 0์ธ ๊ฒฝ์šฐ์— ๋Œ€ํ•ด ๊ฐ๊ฐ ๋‹ค๋ฅธ ์ผ๋ฐ˜ํ™”๋œ ๊ฒฐ๊ณผ๋ฅผ ๋„์ถœํ•œ๋‹ค.

Mathematics
RXTE-ASM light curves of Cen X-3

RXTE-ASM light curves of Cen X-3

Catchy Title KO: Cen X 3์˜ ๊ด‘๋„๊ณก์„  ๋ถˆ์ผ์น˜: ๊ณผ๊ฑฐ์™€ ํ˜„์žฌ์˜ ๋Œ€์กฐ Abstract KO: ์ด ๋…ผ๋ฌธ์€ 2005๋…„์— ๋ฐœํ‘œ๋œ Cen X 3์˜ RXTE ASM ๊ด‘๋„๊ณก์„ ๊ณผ HEASARC ์›น์‚ฌ์ดํŠธ์—์„œ ์ œ๊ณต๋˜๋Š” ์ตœ์‹  ๊ด‘๋„๊ณก์„  ๊ฐ„์˜ ๋ถˆ์ผ์น˜๋ฅผ ๋ณด๊ณ ํ•œ๋‹ค. ์ด๋Ÿฌํ•œ ๋ถˆ์ผ์น˜๋Š” Mรผller ๋“ฑ (2011)์ด RXTE ASM, MAXI, INTEGRAL ๋ฐ SWIFT ๋ฐ์ดํ„ฐ๋ฅผ ํ†ตํ•ด ์œ ์‚ฌํ•œ ํŠน์ง•์„ ๋ฐœ๊ฒฌํ•˜์ง€ ๋ชปํ•œ ๊ฒƒ๊ณผ ์ผ์น˜ํ•œ๋‹ค. ์ €์ž๋“ค์€ ์ด ์ฐจ์ด๊ฐ€ ๋ถ„์„ ์˜ค๋ฅ˜๊ฐ€ ์•„๋‹Œ 2005๋…„์— ์ œ๊ณต๋œ ASM ๊ด‘๋„๊ณก์„ ์˜ ์˜ค๋ฅ˜์—์„œ ๊ธฐ์ธํ•จ์„ ํ™•์ธํ–ˆ๋‹ค. Deep An

Astrophysics
No Image

Transition Radiation by Standard Model Neutrinos at an Interface

1. ์ด๋ก ์  ๋ฐฐ๊ฒฝ ๋ฐ ์—ฐ๊ตฌ ๋ชฉ์  ์ค‘์„ฑ๋ฏธ์ž๋Š” ๋ฌผ๋ฆฌํ•™์—์„œ ๊ฐ€์žฅ ๋ฏธ๋ฌ˜ํ•œ ์ž…์ž ์ค‘ ํ•˜๋‚˜๋กœ, ํ‘œ์ค€ ๋ชจ๋ธ์— ๋”ฐ๋ฅด๋ฉด ๋งค์šฐ ์ž‘์€ ์งˆ๋Ÿ‰์„ ๊ฐ€์ง€๊ณ  ์žˆ์Šต๋‹ˆ๋‹ค. ์ด๋Ÿฌํ•œ ํŠน์„ฑ์ด ์žˆ๊ธฐ ๋•Œ๋ฌธ์—, ์ค‘์„ฑ๋ฏธ์ž์˜ ์ƒํ˜ธ์ž‘์šฉ์€ ์–‘์ž์žฅ ์ด๋ก ์„ ํ†ตํ•ด ์„ค๋ช…๋˜์–ด์•ผ ํ•ฉ๋‹ˆ๋‹ค. ๋ณธ ์—ฐ๊ตฌ์—์„œ๋Š” ์ค‘์„ฑ๋ฏธ์ž๊ฐ€ ๋‘ ๊ฐ€์ง€ ๋‹ค๋ฅธ ๊ตด์ ˆ๋ฅ ์„ ๊ฐ€์ง„ ๋งค์งˆ์˜ ๊ฒฝ๊ณ„๋ฅผ ํ†ต๊ณผํ•  ๋•Œ ๋ฐœ์ƒํ•˜๋Š” ์ „์ด๋ณต์‚ฌ๋ฅผ ํƒ๊ตฌํ•ฉ๋‹ˆ๋‹ค. ์ „์ด๋ณต์‚ฌ๋Š” ์ž…์‚ฌ ์ค‘์„ฑ๋ฏธ์ž๊ฐ€ ์ถœ์‚ฌ ์ค‘์„ฑ๋ฏธ์ž์™€ ๊ด‘์ž๋ฅผ ๋ฐฉ์ถœํ•˜๋ฉด์„œ ๋ฐœ์ƒํ•˜๋Š” ํ˜„์ƒ์ž…๋‹ˆ๋‹ค. ์ด ๊ณผ์ •์€ ์ค‘์„ฑ๋ฏธ์ž์˜ ์šด๋™๋Ÿ‰ ๋ณด์กด์„ ์œ„๋ฐ˜ํ•˜๋ฉฐ, ๋งค์งˆ์˜ ํŠน์„ฑ์ด ์ด๋Ÿฌํ•œ ์ƒํ˜ธ์ž‘์šฉ์— ์ค‘์š”ํ•œ ์—ญํ• ์„ ํ•ฉ๋‹ˆ๋‹ค. 2. ์—ฐ๊ตฌ ๋ฐฉ

Model HEP-PH Astrophysics
Dinamics of HPV Infection among Women with Cervical Lesions

Dinamics of HPV Infection among Women with Cervical Lesions

: ๋ณธ ์—ฐ๊ตฌ๋Š” ์ธ๋ฅ˜ ์œ ๋‘์ข… ๋ฐ”์ด๋Ÿฌ์Šค(HPV)์˜ ์—ญํ•™์„ ๋ถ„์„ํ•˜๊ณ , ํŠนํžˆ ์ž๊ถ๊ฒฝ๋ถ€ ๋ณ‘๋ณ€์„ ๊ฐ€์ง„ ์—ฌ์„ฑ์—์„œ์˜ HPV ๊ฐ์—ผ๊ณผ ๊ด€๋ จ๋œ ๋‹ค์–‘ํ•œ ์ธก๋ฉด์„ ์กฐ์‚ฌํ•˜์˜€๋‹ค. ์—ฐ๊ตฌ๋Š” 293๋ช…์˜ ์—ฌ์„ฑ ํ™˜์ž๋ฅผ ๋Œ€์ƒ์œผ๋กœ ์ง„ํ–‰๋˜์—ˆ์œผ๋ฉฐ, ์ด๋“ค ์ค‘ ์ž๊ถ๊ฒฝ๋ถ€ ์–‘์„ฑ ๋ณ‘๋ณ€์ด ์žˆ๋Š” ํ™˜์ž๋Š” 88๋ช…(30.0%), CIN(Cervical Intraepithelial Neoplasia)์€ 101๋ช…(34.3%), ๊ทธ๋ฆฌ๊ณ  ์ž๊ถ๊ฒฝ๋ถ€์•”์€ 104๋ช…(35.6%)์œผ๋กœ ๊ตฌ์„ฑ๋˜์—ˆ๋‹ค. HPV ๊ฐ์—ผ์˜ ์ผ๋ฐ˜์ ์ธ ํŠน์ง• ๊ฐ์—ผ๋ฅ  : ์ฒซ ๋ฒˆ์งธ ๊ฒ€์‚ฌ์—์„œ, ์ž๊ถ๊ฒฝ๋ถ€ ์–‘์„ฑ ๋ณ‘๋ณ€์ด ์žˆ๋Š” ํ™˜์ž์˜ 61.3%, CIN ํ™˜

Quantitative Biology
Gamma-ray properties of globular clusters and the 'fundamental planes'

Gamma-ray properties of globular clusters and the 'fundamental planes'

์„œ๋ก ๊ณผ ์—ฐ๊ตฌ ๋ฐฐ๊ฒฝ ๋ณธ ๋…ผ๋ฌธ์€ ๊ฐ๋งˆ์„  ์„ฑ์šด์„ ๊ฐ€์ง„ ๊ตฌ์ƒ์„ฑ๋‹จ์— ๋Œ€ํ•œ ์—ฐ๊ตฌ๋ฅผ ํ†ตํ•ด, ํŠนํžˆ ๊ณ ์—๋„ˆ์ง€ ๊ด‘์ž์™€ MSP ์ธ๊ตฌ ์‚ฌ์ด์˜ ์ƒ๊ด€๊ด€๊ณ„๋ฅผ ํƒ์ƒ‰ํ•˜๊ณ  ์žˆ์Šต๋‹ˆ๋‹ค. ๋ผ๋””์˜คํŒŒ์™€ X์„  ๊ด€์ธก์„ ํ†ตํ•ด ์•ฝ 140๊ฐœ์˜ ๋ฐ€๋ฆฌ์ดˆํŒŒ ํŽ„์‚ฌ(MSP)๊ฐ€ 26๊ฐœ์˜ ๊ตฌ์ƒ์„ฑ๋‹จ ๋‚ด์—์„œ ๋ฐœ๊ฒฌ๋˜์—ˆ์ง€๋งŒ, ๋” ๊ฐ•๋ ฅํ•œ X์„  ๋ฐฉ์ถœ์ž๊ฐ€ ๊ด€์ธก์— ์˜ค์—ผ์„ ์ผ์œผํ‚ฌ ์ˆ˜ ์žˆ๋‹ค๋Š” ์ ์ด ์ฃผ๋ชฉ๋ฉ๋‹ˆ๋‹ค. MSP๋Š” ์•Œ๋ ค์ง„ ์œ ์ผํ•œ ๊ตฌ์ƒ์„ฑ๋‹จ ๋‚ด ์•ˆ์ •์ ์ธ ๊ฐ๋งˆ์„  ์›์ฒœ์œผ๋กœ, ์ด ์—ฐ๊ตฌ์—์„œ๋Š” ๋Œ€ํ˜• ์˜์—ญ ๋ง์›๊ฒฝ(LAT)์„ ์‚ฌ์šฉํ•˜์—ฌ 8๊ฐœ์˜ ๊ตฌ์ƒ์„ฑ๋‹จ์—์„œ ๊ฐ๋งˆ์„  ๋ฐฉ์ถœ์„ ๊ด€์ธกํ•˜์˜€์Šต๋‹ˆ๋‹ค. ๊ฐ๋งˆ์„  ๋ฐœ์ƒ ๋ชจ๋ธ ๊ฐ๋งˆ์„ ์˜ ๋ฐœ์ƒ ๊ธฐ์›์€

Astrophysics
Two methods for the light curves extrema determination

Two methods for the light curves extrema determination

๋ณธ ๋…ผ๋ฌธ์€ ๋ณ€๊ด‘์„ฑ ๋ณ„์˜ ๋น› ๊ณก์„ ์—์„œ ๊ทน๋Œ€๊ฐ’๊ณผ ๊ทน์†Œ๊ฐ’์„ ๊ฒฐ์ •ํ•˜๊ธฐ ์œ„ํ•œ ๋‘ ๊ฐ€์ง€ ์ ‘๊ทผ ๋ฐฉ์‹์„ ์ œ์‹œํ•˜๊ณ  ์žˆ๋‹ค. ์ด ์—ฐ๊ตฌ๋Š” ์ฒœ์ฒด๋ฌผ๋ฆฌํ•™ ๋ถ„์•ผ์—์„œ ์ค‘์š”ํ•œ ๋ฌธ์ œ ์ค‘ ํ•˜๋‚˜์ธ ๋ณ€๊ด‘์„ฑ ๋ณ„์˜ ์‹œ๊ฐ„ ์‹œ๋ฆฌ์ฆˆ ๋ฐ์ดํ„ฐ ๋ถ„์„์— ์ดˆ์ ์„ ๋งž์ถ”๊ณ  ์žˆ์œผ๋ฉฐ, ํŠนํžˆ ๋น„์ฃผ๊ธฐ์ ์ธ ๋ณ€๊ด‘ ๋˜๋Š” ์ฃผ๊ธฐ์ ์ธ ๋น› ๊ณก์„ ์„ ๋ณด์ด๋Š” ์ฒœ์ฒด์— ๋Œ€ํ•œ ๊ทน๊ฐ’ ๊ฒฐ์ • ๋ฐฉ๋ฒ•์„ ๋‹ค๋ฃจ๊ณ  ์žˆ๋‹ค. 1. ์„ ํ˜• ํšŒ๊ท€ ๋ถ„์„์„ ์ด์šฉํ•œ ๊ทน๋Œ€๊ฐ’ ๊ฒฐ์ • ์ฒซ ๋ฒˆ์งธ ์ ‘๊ทผ ๋ฐฉ์‹์€ ์„ ํ˜• ํšŒ๊ท€ ๋ชจ๋ธ์„ ์‚ฌ์šฉํ•˜์—ฌ ๊ทน๋Œ€ ๋ฐ ๊ทน์†Œ ์‹œ๊ฐ„์„ ๊ฒฐ์ •ํ•˜๋Š” ๋ฐฉ๋ฒ•์ด๋‹ค. ์ด ๋ฐฉ๋ฒ•์—์„œ๋Š” ๊ด€์ธก๋œ ๋ฐ์ดํ„ฐ๋ฅผ ๋ฒกํ„ฐ Y์™€ t๋กœ ํ‘œํ˜„ํ•˜๊ณ , ๊ฐ๊ฐ์˜ ์ธก์ • ๊ฐ’์— ๊ฐ€์ค‘์น˜ w

Physics Astrophysics
A Formal Approach for Agent Based Large Concurrent Intelligent Systems

A Formal Approach for Agent Based Large Concurrent Intelligent Systems

: ๋ณธ ๋…ผ๋ฌธ์€ ์—์ด์ „ํŠธ ๊ธฐ๋ฐ˜ ๋ชจ๋ธ๋ง์„ ํ†ตํ•œ ๋ณต์žก ์ง€๋Šฅํ˜• ์‹œ์Šคํ…œ ์„ค๊ณ„์— ์ดˆ์ ์„ ๋งž์ถ”๊ณ  ์žˆ์œผ๋ฉฐ, ์ด๋Š” ํ˜„์žฌ์˜ ํ”„๋กœ์ ํŠธ ๊ด€๋ฆฌ์™€ ์‹œ์Šคํ…œ ๊ฐœ๋ฐœ์—์„œ ์ง๋ฉดํ•˜๋Š” ๋ฌธ์ œ๋ฅผ ํ•ด๊ฒฐํ•˜๊ธฐ ์œ„ํ•œ ์ƒˆ๋กœ์šด ์ ‘๊ทผ๋ฒ•์œผ๋กœ ์ œ์‹œ๋œ๋‹ค. ํŠนํžˆ, ์—์ด์ „ํŠธ ๊ธฐ๋ฐ˜ ๋ชจ๋ธ๋ง์€ ๋ณต์žกํ•œ ์‹œ์Šคํ…œ์„ ํšจ๊ณผ์ ์œผ๋กœ ์„ค๊ณ„ํ•˜๊ณ  ๊ตฌํ˜„ํ•  ์ˆ˜ ์žˆ๋Š” ๋ฐฉ๋ฒ•๋ก  ์ค‘ ํ•˜๋‚˜๋กœ ์ฃผ๋ชฉ๋ฐ›๊ณ  ์žˆ๋‹ค. 1. ์—์ด์ „ํŠธ์˜ ์ž์œจ์„ฑ๊ณผ ๋ฐ˜์‘์„ฑ ๋…ผ๋ฌธ์—์„œ๋Š” ์—์ด์ „ํŠธ์˜ ํ•ต์‹ฌ ํŠน์ง•์œผ๋กœ ์ž์œจ์„ฑ๊ณผ ๋ฐ˜์‘์„ฑ์„ ๊ฐ•์กฐํ•œ๋‹ค. ์ž์œจ์„ฑ์€ ์—์ด์ „ํŠธ๊ฐ€ ์Šค์Šค๋กœ ์ž‘๋™ํ•˜๊ณ , ์‹œ์Šคํ…œ ๋ชฉํ‘œ๋ฅผ ๋‹ฌ์„ฑํ•˜๊ธฐ ์œ„ํ•ด ๋‚ด๋ถ€ ํ•˜์œ„ ๋ชฉํ‘œ๋ฅผ ์„ค์ •ํ•˜๊ณ  ์ด๋ฅผ ์ˆ˜ํ–‰ํ•˜๋Š” ๋Šฅ๋ ฅ์„ ์˜๋ฏธํ•œ๋‹ค. ์ด

System Computer Science Software Engineering
High-Energy Gamma-ray Emission Properties of an Anomalous X-ray Pulsar,   4U 0142+61

High-Energy Gamma-ray Emission Properties of an Anomalous X-ray Pulsar, 4U 0142+61

์ด ์—ฐ๊ตฌ๋Š” Fermi/LAT ๋ฐ์ดํ„ฐ๋ฅผ ํ™œ์šฉํ•˜์—ฌ 4U 0142+61์˜ ๊ณ ์—๋„ˆ์ง€ ๊ฐ๋งˆ์„  ๋ฐฉ์ถœ ํŠน์„ฑ์„ ํƒ๊ตฌํ•œ๋‹ค. AXP๋Š” ๊ฐ•ํ•œ ์ž๊ธฐ์žฅ๊ณผ ํ•จ๊ป˜ ๋†’์€ ๊ด‘๋„๋ฅผ ๋ณด์ด๋Š” X ๋ ˆ์ด ์›์œผ๋กœ, ์ฃผ๋กœ ๋ถ€๊ฐ€ ์›๋ฐ˜์ด๋‚˜ ์ž๊ธฐ์žฅ ๋ถ•๊ดด ๋ชจ๋ธ์„ ํ†ตํ•ด ์„ค๋ช…๋˜์–ด ์™”๋‹ค. ๊ทธ๋Ÿฌ๋‚˜ 4U 0142+61์˜ ๊ฒฝ์šฐ, ๊ณ ์—๋„ˆ์ง€ ๊ฐ๋งˆ์„  ๋ฐฉ์ถœ์— ๋Œ€ํ•œ ์ดํ•ด๋Š” ์—ฌ์ „ํžˆ ๋ถˆ์™„์ „ํ•˜๋‹ค. ์—ฐ๊ตฌํŒ€์€ Fermi/LAT ๋ฐ์ดํ„ฐ๋ฅผ ์‚ฌ์šฉํ•˜์—ฌ 4U 0142+61์˜ ํŽ„์Šค ํ”„๋กœํŒŒ์ผ์„ ์ƒ์„ฑํ•˜๊ณ  ๋ถ„์„ํ•˜์˜€๋‹ค. ์ด ๊ณผ์ •์—์„œ RXTE/PCA ๊ด€์ธก์„ ํ†ตํ•ด ์–ป์€ ์ •๋ฐ€ํ•œ ์Šคํ•€ ์—ํŽ˜๋ฉ”๋ฆฌ์Šค๋ฅผ ํ™œ์šฉํ•˜์—ฌ ๊ณ ์—๋„ˆ์ง€ ๊ฐ๋งˆ์„  ๋ฐฉ์ถœ์„ ๊ฒ€์ƒ‰

Astrophysics
New Zealand pathway towards Asia-Pacific and global e-VLBI research and   development

New Zealand pathway towards Asia-Pacific and global e-VLBI research and development

๋ณธ ๋…ผ๋ฌธ์€ ๋‰ด์งˆ๋žœ๋“œ์˜ ์ฒœ๋ฌธํ•™ ๋ฐœ์ „ ๊ณผ์ •์—์„œ ์ค‘์š”ํ•œ ์ „ํ™˜์ ์ด ๋˜๋Š” ์˜คํด๋žœ๋“œ ๊ณต๊ณผ๋Œ€ํ•™(AUT)์˜ ์—ญํ• ์„ ์ง‘์ค‘์ ์œผ๋กœ ๋ถ„์„ํ•˜๊ณ  ์žˆ์Šต๋‹ˆ๋‹ค. ํŠนํžˆ, 2005๋…„๋ถ€ํ„ฐ ์‹œ์ž‘๋œ AUT์˜ ๋…ธ๋ ฅ์€ ๋‰ด์งˆ๋žœ๋“œ๊ฐ€ ๊ตญ์ œ์ ์ธ VLBI ๋„คํŠธ์›Œํฌ์— ํ•ฉ๋ฅ˜ํ•˜๋Š” ๊ณ„๊ธฐ๊ฐ€ ๋˜์—ˆ์œผ๋ฉฐ, ์ด๋Š” ์•„์‹œ์•„ ํƒœํ‰์–‘ ์ง€์—ญ์—์„œ ์ฒœ๋ฌธํ•™ ์—ฐ๊ตฌ ๊ฐœ๋ฐœ์„ ์ฃผ๋„ํ•˜๋Š” ์ค‘์š”ํ•œ ๋‹จ๊ณ„๋กœ ํ‰๊ฐ€๋ฉ๋‹ˆ๋‹ค. 1. ์—ญ์‚ฌ์  ๋ฐฐ๊ฒฝ ๋ฐ ์ดˆ๊ธฐ ๋ฐœ์ „ ๋…ผ๋ฌธ์€ ๋‰ด์งˆ๋žœ๋“œ์˜ ์ฒœ๋ฌธํ•™ ์—ญ์‚ฌ๋ฅผ ๊ฐ„๋žตํ•˜๊ฒŒ ์†Œ๊ฐœํ•˜๋ฉฐ, ํŠนํžˆ 1948๋…„ ํ˜ธ์ฃผ CSIRO์—์„œ ์ง„ํ–‰๋œ ๋ฐ”๋‹ค๋ฅผ ๊ฑฐ์šธ๋กœ ์‚ฌ์šฉํ•œ ๊ฐ„์„ญ๊ณ„ ์„ค์น˜ ์‹คํ—˜์„ ์–ธ๊ธ‰ํ•ฉ๋‹ˆ๋‹ค. ์ด ์‹คํ—˜์€ ๋ผ๋””์˜คํŒŒ ์›์ฒœ์˜ ์œ„์น˜

Physics Astrophysics
GeV Gamma-ray Emission from the Binary PSR B1259-63/SS2883 During the   2010 Periastron Passage

GeV Gamma-ray Emission from the Binary PSR B1259-63/SS2883 During the 2010 Periastron Passage

PSR B1259 63/SS2883์€ ๊ณ ์—๋„ˆ์ง€ ์ฒœ๋ฌธํ•™์—์„œ ์ค‘์š”ํ•œ ์—ฐ๊ตฌ ๋Œ€์ƒ ์ค‘ ํ•˜๋‚˜๋กœ, ํŽ„์Šค ๋ณ„๊ณผ Be ๋ณ„ ๊ฐ„์˜ ์ƒํ˜ธ์ž‘์šฉ์„ ํ†ตํ•ด ๋‹ค์–‘ํ•œ ์—๋„ˆ์ง€ ๋ฒ”์œ„์˜ ๋ฐฉ์ถœ์„ ๋ณด์—ฌ์ค€๋‹ค. ์ด ์‹œ์Šคํ…œ์€ TeV ๊ฐ๋งˆ์„  ์—๋„ˆ์ง€์—์„œ๋„ ๊ด€์ฐฐ๋˜๋ฉฐ, ํŠนํžˆ 2010๋…„ ๊ทผ์ผ์  ํ†ต๊ณผ ์‹œ ๊ธฐ๊ฐ€์ „์ž๋ณผํŠธ(GeV) ๊ฐ๋งˆ์„  ์‹ ํ˜ธ๋ฅผ ํŽ˜๋ฅด๋ฏธ LAT ๋ฐ์ดํ„ฐ๋ฅผ ํ†ตํ•ด ๊ด€์ธกํ•˜์˜€๋‹ค. ํŽ˜๋ฅด๋ฏธ LAT ๋ฐ์ดํ„ฐ๋Š” 2008๋…„๋ถ€ํ„ฐ 2011๋…„๊นŒ์ง€์˜ ์žฅ๊ธฐ๊ฐ„์— ๊ฑธ์ณ ์ˆ˜์ง‘๋˜์—ˆ์œผ๋ฉฐ, ์ด ์ค‘ ํŠนํžˆ ๊ทผ์ผ์  ํ†ต๊ณผ ํ›„ ํ•œ ๋‹ฌ ๋™์•ˆ TS ๊ฐ’์ด 5 (2ฯƒ ์ˆ˜์ค€)๋กœ ์•”์‹œ์  ํ”์ ์ด ๊ด€์ฐฐ๋˜์—ˆ๋‹ค. ์ดํ›„ ๋‘ ๋‹ฌ ๋™์•ˆ ๊ฐ๋งˆ์„  ์‹ ํ˜ธ

Astrophysics
Inclusion of Unambiguous RE#s is NP-Hard

Inclusion of Unambiguous RE#s is NP-Hard

: ๋ณธ ๋…ผ๋ฌธ์€ ์ •๊ทœํ‘œํ˜„์‹(REs)์˜ ํฌํ•จ์„ฑ ๋ฌธ์ œ์— ๋Œ€ํ•œ ์ค‘์š”ํ•œ ์ด๋ก ์  ๊ฒฐ๊ณผ๋ฅผ ์ œ์‹œํ•˜๋ฉฐ, ํŠนํžˆ ๋ช…ํ™•ํ•œ REs์˜ ๊ฒฝ์šฐ์—๋„ NP ๋‚œ์ œ์ž„์„ ์ฆ๋ช…ํ•œ๋‹ค. ์ด๋Ÿฌํ•œ ๊ฒฐ๊ณผ๋Š” XML ์Šคํ‚ค๋งˆ ์ฝ˜ํ…์ธ  ๋ชจ๋ธ์—์„œ ์š”๊ตฌ๋˜๋Š” ๋ช…ํ™•์„ฑ์„ ๋งŒ์กฑํ•˜๋”๋ผ๋„ ๊ณ„์‚ฐ์ ์œผ๋กœ ํ•ด๊ฒฐํ•˜๊ธฐ ์–ด๋ ค์šด ๋ฌธ์ œ๋ผ๋Š” ๊ฒƒ์„ ์‹œ์‚ฌํ•œ๋‹ค. 1. ์„œ๋ก  ์„œ๋ก ์—์„œ๋Š” ์ด์ „ ์—ฐ๊ตฌ

Computational Complexity Computer Science
Subphotospheric heating in GRBs: analysis and modeling of GRB090902B as   observed by Fermi

Subphotospheric heating in GRBs: analysis and modeling of GRB090902B as observed by Fermi

: ์„œ๋ก  ๋ฐ ์—ฐ๊ตฌ ๋ฐฐ๊ฒฝ ๊ฐ๋งˆ์„  ํญ๋ฐœ(GRB)์€ ์šฐ์ฃผ์—์„œ ๊ฐ€์žฅ ๊ฐ•๋ ฅํ•œ ๋ฐฉ์ถœ ํ˜„์ƒ ์ค‘ ํ•˜๋‚˜๋กœ, ๊ทธ ๋ฐœ์ƒ ๋ฉ”์ปค๋‹ˆ์ฆ˜์— ๋Œ€ํ•œ ์ดํ•ด๋Š” ์—ฌ์ „ํžˆ ๋ฏธ์™„์„ฑ ์ƒํƒœ์ž…๋‹ˆ๋‹ค. ๋ถˆ๋ณผ ๋ชจ๋ธ์€ GRB์˜ ๊ธ‰์„ฑ ๋ฐฉ์ถœ์„ ์„ค๋ช…ํ•˜๋Š” ์ฃผ์š” ์ด๋ก ์œผ๋กœ, ์ƒ๋Œ€์ ์œผ๋กœ ๋น ๋ฅด๊ฒŒ ํŒฝ์ฐฝํ•˜๋Š” ๋ถˆ๋ณผ์—์„œ ๋ฐœ์ƒํ•˜๋Š” ๊ฐ€์—ด์ด ๋ฐฉ์ถœ์„ ์ผ์œผํ‚จ๋‹ค๋Š” ๊ฐœ๋…์„ ์ œ์‹œํ•ฉ๋‹ˆ๋‹ค. ๊ทธ๋Ÿฌ๋‚˜ ๋Œ€๋ถ€๋ถ„์˜ GRB ์ŠคํŽ™ํŠธ๋Ÿผ์€ ํ‘์ฒด ๋ณต์‚ฌ ํŠน์„ฑ์„ ๋ช…ํ™•ํžˆ ๋‚˜ํƒ€๋‚ด์ง€ ์•Š์œผ๋ฉฐ, ์ด๋Š” ๋น„์—ด์  ์„ฑ๋ถ„๊ณผ ํ•จ๊ป˜ ์„œ๋ธŒ๋„๋ฏธ๋‚œํŠธ ์—ด ์„ฑ๋ถ„์˜ ์กด์žฌ๋ฅผ ์‹œ์‚ฌํ•ฉ๋‹ˆ๋‹ค. ๋น„์—ด์  ์„ฑ๋ถ„ ๋ฐ ๊ฐ€์—ด ๋ฉ”์ปค๋‹ˆ์ฆ˜ GRB ์ œํŠธ ๋‚ด์—์„œ ๋ฐœ์ƒํ•˜๋Š” ๊ฐ€์—ด์€ ๊ณ ์—๋„ˆ์ง€ ๊ผฌ๋ฆฌ ๋ถ€๋ถ„์„ ํฌํ•จํ•œ

Analysis Model Astrophysics
Environment and properties of emitting electrons in blazar jets: Mrk 421   as a laboratory

Environment and properties of emitting electrons in blazar jets: Mrk 421 as a laboratory

๋ณธ ๋…ผ๋ฌธ์€ Mrk 421์ด๋ผ๋Š” ๋ธ”๋ผ์ž๋ฅด์˜ ๊ฐ๋งˆ์„  ๋ฐฉ์ถœ ๋ฉ”์ปค๋‹ˆ์ฆ˜์— ๋Œ€ํ•ด ์‹ฌ๋„ ์žˆ๋Š” ๋ถ„์„์„ ์ œ๊ณตํ•ฉ๋‹ˆ๋‹ค. ๋ธ”๋ผ์ž๋ฅด๋Š” ํ™œ์„ฑ ์€ํ•˜ํ•ต(AGN) ์ค‘์—์„œ ์ œํŠธ๋ฅผ ์ถ• ์†Œ๊ฐํ•˜๋Š” ๊ฐ๋„๊ฐ€ ์ž‘์•„ ๊ด€์ธก๋˜๋Š” ์ฒœ์ฒด๋กœ, ๊ทธ ์ŠคํŽ™ํŠธ๋Ÿผ ์—๋„ˆ์ง€ ๋ถ„ํฌ(SED)๋Š” ๋ผ๋””์˜คํŒŒ์—์„œ ๊ฐ๋งˆ์„ ๊นŒ์ง€์˜ ๋น„์—ด์  ์—ฐ์† ์ŠคํŽ™ํŠธ๋Ÿผ์„ ๋‚˜ํƒ€๋ƒ…๋‹ˆ๋‹ค. ํŠนํžˆ, Mrk 421์€ ๊ณ ์ฃผํŒŒ BL ๋ผํฌ ๊ฐ์ฒด๋กœ์„œ, ๋‹ค์–‘ํ•œ ํ™œ๋™ ์ƒํƒœ์—์„œ์˜ SED๋ฅผ ์—ฐ๊ตฌํ•จ์œผ๋กœ์จ ๋ฐฉ์ถœ ์ „์ž์˜ ํ™˜๊ฒฝ ๋ฐ ํŠน์„ฑ์„ ์ดํ•ดํ•˜๋Š” ์ค‘์š”ํ•œ ์‹คํ—˜ ๋Œ€์ƒ์ž…๋‹ˆ๋‹ค. ๋…ผ๋ฌธ์—์„œ๋Š” SSC(์‹œ๋„ˆํŠธ๋ก  ์ž์ฒด ์ปดํŠผ) ๋ชจ๋ธ์„ ์‚ฌ์šฉํ•˜์—ฌ Mrk 421์˜ ๊ฐ๋งˆ์„  ๋ฐฉ์ถœ ๋ฉ”์ปค๋‹ˆ์ฆ˜

Astrophysics
Using H-alpha as a Tracer of the Emission Region of LS I +61 303

Using H-alpha as a Tracer of the Emission Region of LS I +61 303

1. ์„œ๋ก  LS I +61 303์€ ๊ณ ์งˆ๋Ÿ‰ X์„  ์Œ์„ฑ๊ณ„(HMXB)๋กœ, B0Veํ˜• ๊ด‘ํ•™ ์„ฑ๊ฐ„์„ฑ๊ณผ ์•Œ๋ ค์ง€์ง€ ์•Š์€ ์ปดํŒฉํŠธํ•œ ๋™๋ฐ˜์ž๋กœ ๊ตฌ์„ฑ๋˜์–ด ์žˆ์Šต๋‹ˆ๋‹ค. ์ด ์‹œ์Šคํ…œ์€ ๋†’์€ ํŽธ์‹ฌ ๊ถค๋„๋ฅผ ๋Œ๋ฉฐ, ์ƒ๋Œ€๋ก ์  ํŽ„์‚ฌ ๋ฐ”๋žŒ๊ณผ ๋ฒ  ๋ณ„ ์›๋ฐ˜์˜ ์ƒํ˜ธ์ž‘์šฉ์œผ๋กœ ์ธํ•ด ๋‹ค์–‘ํ•œ ์ „์ž๊ธฐํŒŒ ์ŠคํŽ™ํŠธ๋Ÿผ์„ ๋ฐฉ์ถœํ•ฉ๋‹ˆ๋‹ค. ์ด๋Ÿฌํ•œ ํŠน์„ฑ ๋•Œ๋ฌธ์— LS I +61 303์€ ์ฒœ๋ฌธํ•™์ ์œผ๋กœ ๋งค์šฐ ์ค‘์š”ํ•œ ์—ฐ๊ตฌ ๋Œ€์ƒ์ž…๋‹ˆ๋‹ค. 2. ๊ด€์ธก 2008๋…„ 10์›”๊ณผ 11์›”์— KPNO Coudรฉ ํ”ผ๋“œ ๋ง์›๊ฒฝ์—์„œ Hฮฑ ์ŠคํŽ™ํŠธ๋Ÿผ์„ ์—ฐ์†์œผ๋กœ ํš๋“ํ•˜์—ฌ, ํ•œ ์™„์ „ํ•œ ๊ถค๋„๋ฅผ ํ†ตํ•ด ๋ฐฉ์ถœ์˜ ์ง„ํ™”๋ฅผ ์—ฐ๊ตฌํ–ˆ์Šต๋‹ˆ๋‹ค. ๊ด€์ธก ๊ฒฐ๊ณผ

Astrophysics
GammaLib - A new framework for the analysis of Astronomical Gamma-Ray   Data

GammaLib - A new framework for the analysis of Astronomical Gamma-Ray Data

: GammaLib ํ”„๋ ˆ์ž„์›Œํฌ๋Š” ๊ฐ๋งˆ์„  ์ฒœ๋ฌธํ•™์˜ ๋ฐ์ดํ„ฐ ๋ถ„์„์— ํ˜์‹ ์ ์ธ ์ ‘๊ทผ๋ฒ•์„ ์ œ์‹œํ•˜๊ณ  ์žˆ์Šต๋‹ˆ๋‹ค. ์ด ๋…ผ๋ฌธ์€ GammaLib์ด ์–ด๋–ป๊ฒŒ ๋‹ค์–‘ํ•œ ๊ฐ๋งˆ์„  ๊ด€์ธก ๊ธฐ๊ธฐ์™€ ๋ฐ์ดํ„ฐ ํ˜•์‹์„ ํ†ตํ•ฉํ•˜์—ฌ ๊ณ ๊ธ‰ ๊ณผํ•™์  ๋ถ„์„์„ ๊ฐ€๋Šฅํ•˜๊ฒŒ ํ•˜๋Š”์ง€ ์„ค๋ช…ํ•ฉ๋‹ˆ๋‹ค. 1. ๊ฐ๋งˆ์„  ์ฒœ๋ฌธํ•™์˜ ํ˜„์žฌ ์ƒํƒœ ๊ฐ๋งˆ์„  ์ฒœ๋ฌธํ•™์€ ์—๋„ˆ์ง€ ๋ฒ”์œ„๊ฐ€ ๋„“๊ณ  ๋‹ค์–‘ํ•œ ๊ฐ๋งˆ์„  ๋ง์›๊ฒฝ์œผ๋กœ ๊ตฌ์„ฑ๋˜์–ด ์žˆ์Šต๋‹ˆ๋‹ค. ์ด๋Ÿฌํ•œ ๋‹ค์–‘์„ฑ์—๋„ ๋ถˆ๊ตฌํ•˜๊ณ , ๋ฐ์ดํ„ฐ๋Š” ๋Œ€๋ถ€๋ถ„ ๊ฐœ๋ณ„ ์ด๋ฒคํŠธ๋กœ ๊ตฌ์„ฑ๋˜๋ฉฐ, ๋„์ฐฉ ์‹œ๊ฐ„, ๋ฐฉํ–ฅ, ๊ทธ๋ฆฌ๊ณ  ์—๋„ˆ์ง€๋ฅผ ํฌํ•จํ•ฉ๋‹ˆ๋‹ค. FITS์™€ OGIP ํ‘œ์ค€์€ ๋งŽ์€ ์šฐ์ฃผ ๊ธฐ๋ฐ˜ ๋ง์›๊ฒฝ์— ๊ตฌํ˜„๋˜์—ˆ์ง€๋งŒ, ์ง€์ƒ

Analysis Framework Astrophysics Data
SSC Emission as Explanation of The Gamma Ray Afterglow Observed in GRB   980923

SSC Emission as Explanation of The Gamma Ray Afterglow Observed in GRB 980923

๋งค๋ ฅ์ ์ธ ํ•œ๊ธ€ ์ œ๋ชฉ: GRB 980923์˜ ํ•˜๋“œ ์ปดํฌ๋„ŒํŠธ์— ๋Œ€ํ•œ ์—ญ๋ฐ˜ ์ถฉ๊ฒฉ ํŒŒํ˜• ์—ฐ๊ตฌ ์ดˆ๋ก ์ „์ฒด ๋ฒˆ์—ญ ๋ฐ ์ •๋ฆฌ: ์ด ๋…ผ๋ฌธ์€ ๊ฐ๋งˆ์„  ํญ๋ฐœ(GRB)๊ณผ ๊ทธ ํ›„๊ด‘์„ ์„ค๋ช…ํ•˜๋Š” ํ™”์—ผ๊ตฌ ๋ชจ๋ธ์„ ๊ธฐ๋ฐ˜์œผ๋กœ, GRB 980923์˜ ํ•˜๋“œ ์ปดํฌ๋„ŒํŠธ๋ฅผ ๋ถ„์„ํ•œ๋‹ค. ํŠนํžˆ, ์—ญ๋ฐ˜ ์ถฉ๊ฒฉ ํŒŒํ˜•์—์„œ ๋ฐœ์ƒํ•˜๋Š” ์ž๊ธฐ์กฐํ™” ์‚ฐ๋ž€(SSC) ๊ณผ์ •์ด X์„  ๋Œ€์—ญ์— ๋ฏธ์น˜๋Š” ์˜ํ–ฅ๊ณผ ๊ณ ์—๋„ˆ์ง€ ์ŠคํŽ™ํŠธ๋Ÿผ ๊ตฌ์„ฑ ์š”์†Œ๋ฅผ ์„ค๋ช…ํ•˜๋Š”๋ฐ ์ดˆ์ ์„ ๋งž์ถ˜๋‹ค. ์—ฐ๊ตฌ์—์„œ๋Š” ์ „๋ฐฉ ์ถฉ๊ฒฉ๊ณผ ํ›„๋ฐฉ ์ถฉ๊ฒฉ์˜ ์—ญํ• ์„ ๋ถ„์„ํ•˜๊ณ , ์ด๋“ค ์ถฉ๊ฒฉ์—์„œ ๋ฐœ์ƒํ•˜๋Š” ๋ฐฉ์ถœ ๊ณผ์ •์„ ๊ณ„์‚ฐํ•˜์—ฌ GRB 980923์˜ ๊ด€์ธก ๋ฐ์ดํ„ฐ์™€ ๋น„๊ตํ•œ๋‹ค. ์‹ฌ

Astrophysics
On a property of the $n$-dimensional cube

On a property of the $n$-dimensional cube

๋ณธ ๋…ผ๋ฌธ์€ ๊ณ ์ฐจ์› ๊ทธ๋ž˜ํ”„ ์ด๋ก ์—์„œ ์ค‘์š”ํ•œ ๋ฌธ์ œ ์ค‘ ํ•˜๋‚˜์ธ n์ฐจ์› ํ๋ธŒ์˜ ๋ถ€๋ถ„ ์ง‘ํ•ฉ์— ๋Œ€ํ•œ ์—ฐ๊ตฌ๋ฅผ ์ˆ˜ํ–‰ํ•˜๊ณ  ์žˆ๋‹ค. ํŠนํžˆ, n โ‰ฅ 4์ผ ๋•Œ, |V'| โ‰ฅ 2^(n 1) + 1์ธ ๋ชจ๋“  ๋ถ€๋ถ„ ์ง‘ํ•ฉ V'์— ๋Œ€ํ•ด ํด๋ผ์šฐ ๋˜๋Š” ๋‹จ์ˆœ ์ˆœํ™˜์„ ์œ ๋„ํ•˜๋Š” ์ •์ ๋“ค์˜ ์กด์žฌ๋ฅผ ์ฆ๋ช…ํ•œ๋‹ค. ์„œ๋ก  ๋ฐ ์ •์˜ ๋…ผ๋ฌธ์€ ๊ทธ๋ž˜ํ”„ ์ด๋ก ์—์„œ ์ค‘์š”ํ•œ ๊ฐœ๋…๋“ค์„ ์†Œ๊ฐœํ•˜๊ณ , n์ฐจ์› ํ๋ธŒ Qn๊ณผ ํด๋ผ์šฐ(K1,3)์˜ ์ •์˜๋ฅผ ์ œ๊ณตํ•œ๋‹ค. ํŠนํžˆ, n์ฐจ์› ํ๋ธŒ๋Š” ๊ฐ ์ฐจ์›๋งˆ๋‹ค ๋‘ ๊ฐœ์˜ ๊ฐ’์„ ๊ฐ€์งˆ ์ˆ˜ ์žˆ๋Š” ์ •์  ์ง‘ํ•ฉ์œผ๋กœ ๊ตฌ์„ฑ๋˜๋ฉฐ, ํด๋ผ์šฐ๋Š” ์ค‘์‹ฌ ์ •์ ์„ ํฌํ•จํ•˜๋Š” ์™„์ „ ์ด๋ถ„ ๊ทธ๋ž˜ํ”„ K1,3์„ ์˜๋ฏธํ•œ

Mathematics Computer Science Discrete Mathematics
Quantum Entanglement Phase Transition in Werner State

Quantum Entanglement Phase Transition in Werner State

: ๋ณธ ๋…ผ๋ฌธ์€ ๊ณ„์‚ฐ ์—ญํ•™์„ ๊ธฐ๋ฐ˜์œผ๋กœ ํ•œ ์ƒˆ๋กœ์šด ์ ‘๊ทผ๋ฒ•์„ ํ†ตํ•ด ์–‘์ž ์‹œ์Šคํ…œ์˜ ๋ณต์žก์„ฑ์„ ์ธก์ •ํ•˜๋Š” ๋ฐฉ๋ฒ•์„ ์ œ์•ˆํ•˜๊ณ  ์žˆ์Šต๋‹ˆ๋‹ค. ์ด ์—ฐ๊ตฌ๋Š” ๊ณ ์ „์  ๋ณต์žก์„ฑ ์ธก์ • ์ง€ํ‘œ์™€ ๋‹ฌ๋ฆฌ, ์–ฝํž˜๊ณผ ๊ฐ™์€ ์–‘์ž ํšจ๊ณผ๋ฅผ ํฌ์ฐฉํ•  ์ˆ˜ ์žˆ๋Š” ์ƒˆ๋กœ์šด ์ง€ํ‘œ ๊ฐœ๋ฐœ์— ์ดˆ์ ์„ ๋งž์ถ”๊ณ  ์žˆ์Šต๋‹ˆ๋‹ค. 1. ๊ณ„์‚ฐ ์—ญํ•™์˜ ๊ธฐ์ดˆ ๊ณ„์‚ฐ ์—ญํ•™์€ Crutchfield์™€ Young์ด ์ œ์•ˆํ•œ ๊ฐœ๋…์œผ๋กœ, ๋™์—ญํ•™ ์‹œ์Šคํ…œ์˜ ๋ณต์žก์„ฑ์„ ์ธก์ •ํ•˜๋Š” ๋ฐฉ๋ฒ•์„ ์ œ๊ณตํ•ฉ๋‹ˆ๋‹ค. ์ด ์ ‘๊ทผ๋ฒ•์—์„œ๋Š” ํ™•๋ฅ ์  ์ž๋™๋ฌธ์„ ์ƒ์„ฑํ•˜์—ฌ ๋ถ„์„ ์‹œ์Šคํ…œ์˜ ๊ธฐํ˜ธ ์—ญํ•™์„ ๋ชจ๋ฐฉํ•˜๊ณ , ์ด๋ฅผ ํ†ตํ•ด ๋‚ด์žฌ์ ์ธ ๊ณ„์‚ฐ ๋ฐ ๋ณต์žก์„ฑ์„ ์ •๋Ÿ‰ํ™”ํ•ฉ๋‹ˆ๋‹ค. 2. ์–‘์ž ์ƒ

Physics Nonlinear Sciences Quantum Physics
New Zealand involvement in Radio Astronomical VLBI Image Processing

New Zealand involvement in Radio Astronomical VLBI Image Processing

: ๋ณธ ๋…ผ๋ฌธ์€ ๋‰ด์งˆ๋žœ๋“œ์˜ ์›Œํฌ์›Œ์Šค ๋ผ๋””์˜ค ์ฒœ๋ฌธ๋Œ€(WRAO)์™€ ํ˜ธ์ฃผ ์žฅ๊ฑฐ๋ฆฌ ๋ฐฐ์—ด(LBA) ๊ฐ„์˜ ํ˜‘๋ ฅ์ด ์–ด๋–ป๊ฒŒ ๊ณ ํ•ด์ƒ๋„ ๋ผ๋””์˜ค ์˜์ƒ์„ ์ƒ์„ฑํ•˜๋Š” ๋ฐ ๊ธฐ์—ฌํ•˜๊ณ  ์žˆ๋Š”์ง€๋ฅผ ์‹ฌ์ธต์ ์œผ๋กœ ๋ถ„์„ํ•ฉ๋‹ˆ๋‹ค. WRAO๋Š” AUT ๋Œ€ํ•™๊ต์˜ IRASR์—์„œ ์šด์˜๋˜๋ฉฐ, 12m ๋ผ๋””์˜ค ๋ง์›๊ฒฝ์€ ์„ธ ๊ฐ€์ง€ ์ฃผํŒŒ์ˆ˜ ๋Œ€์—ญ(1.4, 2.3, 8.6 GHz)์—์„œ ์ž‘๋™ํ•ฉ๋‹ˆ๋‹ค. ํ•ต์‹ฌ ๋‚ด์šฉ ๋ถ„์„ VLBI์™€ LBA์˜ ํ˜‘๋ ฅ: WRAO๋Š” 2011๋…„๋ถ€ํ„ฐ LBA์— ์ •๊ธฐ์ ์œผ๋กœ ์ฐธ์—ฌํ•˜๊ณ  ์žˆ์œผ๋ฉฐ, ์ด๋กœ ์ธํ•ด VLBI ์ž‘์—…์˜ ํ•ด์ƒ๋„๊ฐ€ ํฌ๊ฒŒ ํ–ฅ์ƒ๋˜์—ˆ์Šต๋‹ˆ๋‹ค. ํŠนํžˆ WRAO์˜ ์ถ”๊ฐ€๋กœ ๋™์„œ ๊ธฐ์„  ๊ธธ์ด๊ฐ€ ์•ฝ

Graphics Computer Science Astrophysics
Zum 200. Geburtstag von Evariste Galois

Zum 200. Geburtstag von Evariste Galois

: ๊ฐˆ๋ฃจ์•„์˜ ์‚ถ๊ณผ ์‹œ๋Œ€์  ๋ฐฐ๊ฒฝ ์—๋ฐ”๋ฆฌ์Šค ๊ฐˆ๋ฃจ์•„๋Š” ํ”„๋ž‘์Šค ํ˜๋ช… ์ดํ›„์˜ ๋ถˆ์•ˆ์ •ํ•œ ์ •์น˜ ํ™˜๊ฒฝ ์†์—์„œ ํƒœ์–ด๋‚ฌ๋‹ค. ๊ทธ์˜ ์ƒ์• ๋Š” 1820๋…„๋Œ€์™€ 30๋…„๋Œ€, ์ฆ‰ ๋‘ ๋ฒˆ์งธ ํ˜๋ช…์ด ์ผ์–ด๋‚œ ์‹œ๊ธฐ์™€ ๋งž๋ฌผ๋ ค ์žˆ๋‹ค. ์ด๋Ÿฌํ•œ ์‹œ๋Œ€์  ๋ฐฐ๊ฒฝ์€ ๊ฐˆ๋ฃจ์•„์—๊ฒŒ ํฐ ์˜ํ–ฅ์„ ๋ฏธ์ณค์œผ๋ฉฐ, ๊ทธ๋Š” ์ •์น˜์ ์œผ๋กœ ๋งค์šฐ ํ™œ๋™์ ์ด์—ˆ๋‹ค. ๊ทธ๋Ÿฌ๋‚˜ ์ด๋กœ ์ธํ•ด ํ•™๊ต์—์„œ ์ถ”๋ฐฉ๋‹นํ•˜๊ฑฐ๋‚˜ ์‚ฌํšŒ์  ์ œ์•ฝ์„ ๊ฒช๊ฒŒ ๋˜์—ˆ๋‹ค. ์ˆ˜ํ•™์  ์—…์  ๊ฐˆ๋ฃจ์•„์˜ ๊ฐ€์žฅ ์ค‘์š”ํ•œ ์ˆ˜ํ•™์  ์—…์  ์ค‘ ํ•˜๋‚˜๋Š” ๋ฐฉ์ •์‹์˜ ํ•ด๋ฒ•๊ณผ ๊ตฐ๋ก  ์‚ฌ์ด์˜ ๊นŠ์€ ์—ฐ๊ฒฐ์„ ํƒ๊ตฌํ•œ ๊ฒƒ์ด๋‹ค. ๊ทธ๋Š” ๋‹ค์„ฏ ์ฐจ์ˆ˜ ์ด์ƒ์˜ ๋ฐฉ์ •์‹์— ๋Œ€ํ•œ ์ผ๋ฐ˜์ ์ธ ํ•ด๋ฒ•์ด ์กด์žฌํ•˜์ง€ ์•Š๋Š”๋‹ค๋Š” ๊ฒƒ

Mathematics
No Image

Jacobians and Hessians of Mean Value Coordinates for Closed Triangular Meshes

์ด ๋…ผ๋ฌธ์€ ํ์‡„ ์‚ผ๊ฐ๋ง์— ๋Œ€ํ•œ ํ‰๊ท ๊ฐ’ ์ขŒํ‘œ๋ฅผ ๋‹ค๋ฃจ๋Š” ๋ฐ ์ค‘์ ์„ ๋‘๊ณ  ์žˆ์œผ๋ฉฐ, ์ด๋ฅผ ํ†ตํ•ด 3์ฐจ์› ๊ณต๊ฐ„ ๋‚ด์—์„œ ๋ฉ”์‰ฌ ๋ณ€ํ˜• ๋ฐ ๋ณด๊ฐ„ ๊ณผ์ •์„ ๋ถ„์„ํ•ฉ๋‹ˆ๋‹ค. ์ฃผ์š” ๋‚ด์šฉ๊ณผ ๋ถ„์„์€ ๋‹ค์Œ๊ณผ ๊ฐ™์Šต๋‹ˆ๋‹ค. 1. ํ‰๊ท ๊ฐ’ ์ขŒํ‘œ์˜ ์ •์˜์™€ ๊ณ„์‚ฐ ๋…ผ๋ฌธ์—์„œ๋Š” ํ์‡„ ์‚ผ๊ฐ๋ง M์˜ ๊ผญ์ง“์  p i๋ฅผ ์‚ฌ์šฉํ•˜์—ฌ 3์ฐจ์› ๊ณต๊ฐ„ ๋‚ด ์  ฮท๋ฅผ ํ‘œํ˜„ํ•˜๋Š” ๋ฐฉ๋ฒ•์„ ์ œ์‹œํ•ฉ๋‹ˆ๋‹ค. ์ด๋Š” w i๋ผ๋Š” ๊ฐ€์ค‘์น˜๋ฅผ ํ†ตํ•ด ์ด๋ฃจ์–ด์ง€๋ฉฐ, ์ด ๊ฐ€์ค‘์น˜๋“ค์€ ฮป i๋ฅผ ํ†ตํ•ด ์ •์˜๋ฉ๋‹ˆ๋‹ค. ์ด๋Ÿฌํ•œ ๊ฐ€์ค‘์น˜๋“ค์„ ์ด์šฉํ•ด ํ‰๊ท ๊ฐ’ ์ขŒํ‘œ๋ฅผ ๊ณ„์‚ฐํ•  ์ˆ˜ ์žˆ์Šต๋‹ˆ๋‹ค. 2. ํ•จ์ˆ˜ ๋ณด๊ฐ„๊ณผ ์„ ํ˜• ์ •๋ฐ€๋„ ํ‰๊ท ๊ฐ’ ์ขŒํ‘œ๋Š” ์‚ผ๊ฐ๋ง ๋‚ด์—์„œ ๊ฐ ๊ผญ์ง“์ 

Computer Science Graphics
No Image

Markov-Binary Visibility Graph: a new method for analyzing Complex Systems

์ฃ„์†กํ•ฉ๋‹ˆ๋‹ค, ํ•˜์ง€๋งŒ ์ œ๊ณต๋œ ํ…์ŠคํŠธ ์กฐ๊ฐ์—๋Š” ์‹ค์ œ ๋‚ด์šฉ์ด ํฌํ•จ๋˜์–ด ์žˆ์ง€ ์•Š์•„์„œ ๋…ผ๋ฌธ์˜ ์ดˆ๋ก์ด๋‚˜ ์‹ฌ๋„ ๋ถ„์„์„ ์ˆ˜ํ–‰ํ•  ์ˆ˜ ์—†์Šต๋‹ˆ๋‹ค. ๋…ผ๋ฌธ์˜ ๋ณธ๋ฌธ ๋˜๋Š” ์ค‘์š”ํ•œ ๋ถ€๋ถ„์„ ํฌํ•จํ•˜๋Š” ์ถ”๊ฐ€ ์ •๋ณด๊ฐ€ ํ•„์š”ํ•ฉ๋‹ˆ๋‹ค. ๋งŒ์•ฝ ๋…ผ๋ฌธ์˜ ํŠน์ • ์„น์…˜์ด๋‚˜ ์š”์•ฝ, ๊ทธ๋ž˜ํ”„, ํ‘œ ๋“ฑ์„ ์ œ๊ณตํ•ด ์ฃผ์‹ค ๊ฒฝ์šฐ, ๊ทธ์— ๋”ฐ๋ฅธ ๋ถ„์„๊ณผ ๋ฒˆ์—ญ์„ ๋„์™€๋“œ๋ฆด ์ˆ˜ ์žˆ์Šต๋‹ˆ๋‹ค.

Physics Nonlinear Sciences System
ABHIVYAKTI: A Vision Based Intelligent System for Elder and Sick Persons

ABHIVYAKTI: A Vision Based Intelligent System for Elder and Sick Persons

ABHIVYA KTI๋Š” ๋งํ•˜๊ฑฐ๋‚˜ ๊ฑธ์„ ์ˆ˜ ์—†๋Š” ๋…ธ์ธ์ด๋‚˜ ํ™˜์ž๋ฅผ ์œ„ํ•œ ์† ์ œ์Šค์ฒ˜ ์ธ์‹ ์‹œ์Šคํ…œ์œผ๋กœ, ์ปดํ“จํ„ฐ ๋น„์ „ ๊ธฐ์ˆ ์„ ํ™œ์šฉํ•˜์—ฌ ์‚ฌ์šฉ์ž์˜ ์ œ์Šค์ฒ˜๋ฅผ ํ•ด์„ํ•˜๊ณ  ํ•„์š”ํ•œ ๋™์ž‘์„ ์ˆ˜ํ–‰ํ•˜๋Š” ๋ฐ ์ดˆ์ ์„ ๋งž์ถ”๊ณ  ์žˆ์Šต๋‹ˆ๋‹ค. ์ด ์—ฐ๊ตฌ์˜ ํ•ต์‹ฌ์€ ์ธ๊ฐ„๊ณผ ๊ธฐ๊ณ„ ๊ฐ„์˜ ์ƒํ˜ธ์ž‘์šฉ์„ ํ–ฅ์ƒ์‹œํ‚ค๋Š” ๊ฒƒ์ž…๋‹ˆ๋‹ค. 1. ์‹œ์Šคํ…œ ๊ตฌ์„ฑ ๋ฐ ์ž‘๋™ ๋ฐฉ์‹ ABHIVYA KTI๋Š” ์นด๋ฉ”๋ผ๋ฅผ ํ†ตํ•ด ์‚ฌ์šฉ์ž์˜ ์† ์ œ์Šค์ฒ˜๋ฅผ ์บก์ฒ˜ํ•˜๊ณ , ์ด๋ฅผ ํ•ด์„ํ•˜์—ฌ ํ•„์š”ํ•œ ๋™์ž‘์„ ์ˆ˜ํ–‰ํ•ฉ๋‹ˆ๋‹ค. ์ด ์‹œ์Šคํ…œ์€ ๋ฏธ๋ฆฌ ์ •์˜๋œ ์ œ์Šค์ฒ˜ ๋ฌธ๋ฒ•์— ๋”ฐ๋ผ ์ž‘๋™ํ•˜๋ฉฐ, ์œ ํšจํ•œ ์ œ์Šค์ฒ˜๊ฐ€ ์ž…๋ ฅ๋˜๋ฉด ํ•ด๋‹น ๋™์ž‘์„ ์‹คํ–‰ํ•˜๊ณ  ์™„๋ฃŒ ๋ฉ”์‹œ์ง€๋ฅผ ์‚ฌ์šฉ์ž

Computer Science System Computer Vision
Fourier Cosine and Sine Transform on fractal space

Fourier Cosine and Sine Transform on fractal space

์ด ๋…ผ๋ฌธ์€ ์–‘ ํ‘ธ๋ฆฌ์— ๋ณ€ํ™˜๊ณผ ๊ทธ ์‘์šฉ์„ ์ค‘์‹ฌ์œผ๋กœ ํ”„๋ž™ํƒˆ ๊ณต๊ฐ„์—์„œ์˜ ํ•จ์ˆ˜ ํ•ด์„ ๋ฐฉ๋ฒ•๋ก ์„ ํƒ์ƒ‰ํ•ฉ๋‹ˆ๋‹ค. ํŠนํžˆ, ์ด ์—ฐ๊ตฌ๋Š” ๋ถˆ๊ทœ์น™ํ•œ ์—ฐ์† ํ”„๋ž™ํƒˆ ํ•จ์ˆ˜๋ฅผ ๋‹ค๋ฃจ๋Š”๋ฐ ์ค‘์š”ํ•œ ์—ญํ• ์„ ํ•˜๋Š” ์ง€์—ญ ๋ถ„์‚ฐ ๋ฏธ์ ๋ถ„ํ•™์„ ๊ธฐ๋ฐ˜์œผ๋กœ ํ•œ ์–‘ ํ‘ธ๋ฆฌ์— ๋ณ€ํ™˜์„ ์†Œ๊ฐœํ•˜๊ณ , ์ด๋ฅผ ํ†ตํ•ด ์ฝ”์‚ฌ์ธ๊ณผ ์‚ฌ์ธ ๋ณ€ํ™˜์˜ ์ƒˆ๋กœ์šด ํ˜•ํƒœ๋ฅผ ์ œ์‹œํ•ฉ๋‹ˆ๋‹ค. ์ด๋Ÿฌํ•œ ๋ณ€ํ™˜๋“ค์€ ๊ณตํ•™ ๋ฌธ์ œ ํ•ด๊ฒฐ์—์„œ ์œ ์šฉํ•˜๋ฉฐ, ํŠนํžˆ ํ”„๋ž™ํƒˆ ์ฐจ์› ฮฑ ์— ๋Œ€ํ•œ ํ•จ์ˆ˜๋“ค์˜ ๋ถ„์„์— ์ค‘์š”ํ•œ ๋„๊ตฌ๊ฐ€ ๋ฉ๋‹ˆ๋‹ค. 1. ์–‘ ํ‘ธ๋ฆฌ์— ๋ณ€ํ™˜์˜ ์ •์˜์™€ ์„ฑ์งˆ ์–‘ ํ‘ธ๋ฆฌ์— ๋ณ€ํ™˜์€ ์ง€์—ญ ๋ถ„์‚ฐ ๋ฏธ์ ๋ถ„ํ•™์„ ๊ธฐ๋ฐ˜์œผ๋กœ ํ•˜๋ฉฐ, ์ด๋Š” ํ”„๋ž™ํƒˆ ๊ณต๊ฐ„์—์„œ์˜ ์—ฐ์† ํ•จ์ˆ˜๋ฅผ

Mathematics
Verifying Sierpinski and Riesel Numbers in ACL2

Verifying Sierpinski and Riesel Numbers in ACL2

์ด ๋…ผ๋ฌธ์€ ์‹œ๋ฅดํ”ผ๋‹ˆ(Sierpiล„ski) ์ˆ˜์™€ ๋ ˆ์ ค(Riesel) ์ˆ˜์— ๋Œ€ํ•œ ์‹ฌ๋„ ์žˆ๋Š” ๋ถ„์„๊ณผ ACL2๋ผ๋Š” ์ปดํ“จํ„ฐ ์ฆ๋ช… ๋„๊ตฌ๋ฅผ ํ™œ์šฉํ•œ ๊ทธ๋“ค์˜ ์„ฑ์งˆ ๊ฒ€์ฆ ๋ฐฉ๋ฒ•์„ ๋‹ค๋ฃน๋‹ˆ๋‹ค. ์ด๋“ค ์ˆ˜๋Š” ํŠน์ • ์–‘์˜ ํ™€์ˆ˜ ์ •์ˆ˜๊ฐ€ ๋ฌดํ•œ ๋ฆฌ์ŠคํŠธ์—์„œ ์†Œ์ˆ˜๊ฐ€ ๋ฐœ๊ฒฌ๋˜์ง€ ์•Š๋Š” ๊ฒฝ์šฐ์— ํ•ด๋‹นํ•˜๋ฉฐ, ์ด๋ฅผ ํ†ตํ•ด ์ˆ˜ํ•™์ ์œผ๋กœ ์ค‘์š”ํ•œ ์œ„์น˜๋ฅผ ์ฐจ์ง€ํ•˜๊ณ  ์žˆ์Šต๋‹ˆ๋‹ค. ์‹œ๋ฅดํ”ผ๋‹ˆ์™€ ๋ ˆ์ ค ์ˆ˜์˜ ๊ฐœ๋… ์‹œ๋ฅดํ”ผ๋‹ˆ ์ˆ˜์™€ ๋ ˆ์ ค ์ˆ˜๋Š” ๊ฐ๊ฐ k โ€ข 2^n + 1๊ณผ k โ€ข 2^n 1 ํ˜•ํƒœ์˜ ๋ฌดํ•œ ๋ฆฌ์ŠคํŠธ์—์„œ ์†Œ์ˆ˜๊ฐ€ ๋ฐœ๊ฒฌ๋˜์ง€ ์•Š๋Š” ์–‘์˜ ํ™€์ˆ˜ ์ •์ˆ˜์ž…๋‹ˆ๋‹ค. ์ด๋“ค ์ˆ˜๋ฅผ ์‹๋ณ„ํ•˜๋Š” ๊ฒƒ์€ ์–ด๋ ต์ง€๋งŒ, ํŠน์ • ์กฐ๊ฑด์„ ๋งŒ์กฑํ•˜๋ฉด

Computer Science Discrete Mathematics Logic
Multicanonical entropy like-solution of statistical temperature weighted   histogram analysis method (ST-WHAM)

Multicanonical entropy like-solution of statistical temperature weighted histogram analysis method (ST-WHAM)

๋ณธ ๋…ผ๋ฌธ์€ ST WHAM (ํ†ต๊ณ„์  ์˜จ๋„ ๊ฐ€์ค‘ ํžˆ์Šคํ† ๊ทธ๋žจ ๋ถ„์„ ๋ฐฉ๋ฒ•)์— ์ค‘์ ์„ ๋‘๊ณ , ์ด ๋ฐฉ๋ฒ•์ด ๋ฏธ์„ธ๊ด€์„ฑ ์—”ํŠธ๋กœํ”ผ๋ฅผ ์ถ”์ •ํ•˜๋Š” ๋ฐ ์–ผ๋งˆ๋‚˜ ํšจ๊ณผ์ ์ธ์ง€๋ฅผ ๋ถ„์„ํ•ฉ๋‹ˆ๋‹ค. WHAM ๋ฐฉ์‹์˜ ํ•œ๊ณ„์™€ ST WHAM์˜ ๊ฐœ์„ ์ , ๊ทธ๋ฆฌ๊ณ  ์ด๋ฅผ ํ†ตํ•ด ์–ป์„ ์ˆ˜ ์žˆ๋Š” ์—ด์—ญํ•™์  ์ •๋ณด์˜ ์ค‘์š”์„ฑ์„ ๊ฐ•์กฐํ•˜๊ณ  ์žˆ์Šต๋‹ˆ๋‹ค. 1. WHAM๊ณผ ST WHAM์˜ ๋น„๊ต WHAM์€ ๋‹ค์–‘ํ•œ ์˜จ๋„์—์„œ ์ˆ˜ํ–‰๋œ ๋ชฌํ…Œ์นด๋ฅผ๋กœ ์‹œ๋ฎฌ๋ ˆ์ด์…˜ ๋ฐ์ดํ„ฐ๋ฅผ ๊ฒฐํ•ฉํ•˜์—ฌ ์ƒ˜ํ”Œ๋ง์„ ํ–ฅ์ƒ์‹œํ‚ค๋Š” ๋ฐฉ๋ฒ•์ž…๋‹ˆ๋‹ค. ๊ทธ๋Ÿฌ๋‚˜, ์ด ๋ฐฉ์‹์€ ๋ฐ˜๋ณต์ ์ธ ์ˆ˜์น˜ ๊ณผ์ •์„ ํ•„์š”๋กœ ํ•˜๋ฉฐ, ์ด๋ฅผ ํ†ตํ•ด ์—๋„ˆ์ง€ ๋ฐ์ดํ„ฐ๊ฐ€ ์ €์žฅ๋œ ํžˆ์Šคํ† ๊ทธ๋žจ์—์„œ ์ž์œ 

Analysis Physics Condensed Matter
Goonhilly Sparklers

Goonhilly Sparklers

: ์ด ๋…ผ๋ฌธ์€ ๊ณ ์šดํž๋ฆฌ ์ง€๊ตฌ๊ด€์ธก์†Œ๋ฅผ ํ™œ์šฉํ•œ ๊ทน๋‹จ ์‚ฐ๋ž€ ์‚ฌ๊ฑด(ESEs) ์—ฐ๊ตฌ์— ๋Œ€ํ•œ ์‹ฌ๋„ ์žˆ๋Š” ๋ถ„์„์„ ์ œ๊ณตํ•ฉ๋‹ˆ๋‹ค. ESEs๋Š” ์ด์˜จํ™”๋œ ๊ธฐ์ฒด์—์„œ ๋ฐœ์ƒํ•˜๋Š” ์ „ํŒŒ ๊ตด์ ˆ ํ˜„์ƒ์œผ๋กœ, ISM์˜ ์••๋ ฅ์ด ์ฒœ ๋ฐฐ ์ด์ƒ ๋†’์•„์•ผ ํ•˜๋ฉฐ AU ํฌ๊ธฐ์˜ ์˜์—ญ์—์„œ ์ผ์–ด๋‚˜๋Š” ๋งค์šฐ ๋“œ๋ฌธ ์‚ฌ๊ฑด์ž…๋‹ˆ๋‹ค. ์ด๋Ÿฌํ•œ ํ˜„์ƒ์€ ISM์˜ ๊ธฐ๋ณธ ๋ฌผ๋ฆฌํ•™์— ๋Œ€ํ•œ ์šฐ๋ฆฌ์˜ ์ดํ•ด๋ฅผ ๋„์ „ํ•˜๊ณ  ์žˆ์œผ๋ฉฐ, ์ด์ „ ์—ฐ๊ตฌ์—์„œ๋Š” ๋ฐ”๋ฆฌ์˜จ ์•”ํ‘ ๋ฌผ์งˆ์ด ESEs์˜ ์›์ธ์ผ ์ˆ˜ ์žˆ๋‹ค๊ณ  ์ œ์•ˆ๋˜์—ˆ์Šต๋‹ˆ๋‹ค. ๋…ผ๋ฌธ์€ ๊ณ ์šดํž๋ฆฌ ์ง€๊ตฌ๊ด€์ธก์†Œ๊ฐ€ ESEs ์—ฐ๊ตฌ์— ์–ด๋–ป๊ฒŒ ๊ธฐ์—ฌํ•  ์ˆ˜ ์žˆ๋Š”์ง€ ์„ค๋ช…ํ•ฉ๋‹ˆ๋‹ค. ๊ณ ์šดํž๋ฆฌ๋Š” ์˜๊ตญ ์ฝ˜์›”์— ์œ„์น˜ํ•œ ์ „

Astrophysics
Marching of Freely Falling Plates

Marching of Freely Falling Plates

'์ž์œ  ๋‚™ํ•˜ํ•˜๋Š” ํŒ์˜ ํ–‰์ง„: ์ˆ˜์น˜ ์‹œ๋ฎฌ๋ ˆ์ด์…˜ ๋ถ„์„'์€ ์œ ์ฒด ์—ญํ•™๊ณผ ๋น„์„ ํ˜• ๋™์—ญํ•™ ๋ถ„์•ผ์—์„œ ์ค‘์š”ํ•œ ๋ฌธ์ œ์ธ ์ž์œ  ๋‚™ํ•˜ํ•˜๋Š” ํŒ์˜ ์šด๋™์— ๋Œ€ํ•œ ์‹ฌ์ธต์ ์ธ ์—ฐ๊ตฌ๋ฅผ ์ œ๊ณตํ•ฉ๋‹ˆ๋‹ค. ์ด ์—ฐ๊ตฌ๋Š” ๋‹ค์–‘ํ•œ ๋ฌผ๋ฆฌ์  ์กฐ๊ฑด ํ•˜์—์„œ ํŒ์ด ์–ด๋–ป๊ฒŒ ํ–‰๋™ํ•˜๋Š”์ง€, ๊ทธ๋ฆฌ๊ณ  ์ด๋Ÿฌํ•œ ํ–‰๋™์ด ์ฃผ๋ณ€ ์œ ์ฒด์™€ ์–ด๋–ค ์ƒํ˜ธ์ž‘์šฉ์„ ํ•˜๋Š”์ง€๋ฅผ ํƒ๊ตฌํ•˜๊ณ  ์žˆ์Šต๋‹ˆ๋‹ค. 1. ํŒ์˜ ๊ถค์ ๊ณผ ์šด๋™ ์ž์œ  ๋‚™ํ•˜ํ•˜๋Š” ํŒ์˜ ๊ถค์ ์€ ๋งค์šฐ ๋ณต์žกํ•˜๋ฉฐ, ์ด๋Š” ๋ ˆ์ด๋†€์ฆˆ ์ˆ˜์น˜(Reynolds number)์™€ ํ”„๋ผ์šฐ๋“œ ์ˆ˜(Froude number)์— ํฌ๊ฒŒ ์˜์กดํ•ฉ๋‹ˆ๋‹ค. ๋†’์€ ๋ ˆ์ด๋†€์ฆˆ ์ˆ˜์—์„œ ์†Œํ˜• ํ”„๋ผ์šฐ๋“œ ์ˆ˜๋ฅผ ๊ฐ€์ง„ ํŒ์€ ์ง„

Physics
Search for high-energy gamma-ray emission from galaxies of the Local   Group with Fermi/LAT

Search for high-energy gamma-ray emission from galaxies of the Local Group with Fermi/LAT

) ์‹ฌ๋„ ๋ถ„์„: ๋ณธ ์—ฐ๊ตฌ๋Š” ๊ณ ์—๋„ˆ์ง€ ๊ฐ๋งˆ์„  ๋ฐฉ์ถœ์˜ ์›์ฒœ์— ๋Œ€ํ•œ ์ดํ•ด๋ฅผ ํ™•์žฅํ•˜๋Š” ๋ฐ ์ค‘์š”ํ•œ ์—ญํ• ์„ ์ˆ˜ํ–‰ํ•œ๋‹ค. ํŠนํžˆ, Local Group ๋‚ด ์ผ๋ฐ˜ ์€ํ•˜์—์„œ ์ด๋Ÿฌํ•œ ๋ฐฉ์ถœ์ด ๋ฐœ์ƒํ•  ์ˆ˜ ์žˆ๋Š” ๊ฐ€๋Šฅ์„ฑ์„ ํƒ์ƒ‰ํ•จ์œผ๋กœ์จ, ์šฐ์ฃผ์„  ์ƒํ˜ธ์ž‘์šฉ๊ณผ ๊ด€๋ จ๋œ ํ˜„์ƒ์— ๋Œ€ํ•ด ๋” ๊นŠ์€ ํ†ต์ฐฐ๋ ฅ์„ ์ œ๊ณตํ•œ๋‹ค. 1. ์—ฐ๊ตฌ ๋ฐฐ๊ฒฝ ๋ฐ ๋ชฉ์ : ๊ณ ์—๋„ˆ์ง€ ๊ฐ๋งˆ์„ ์˜ ์›์ฒœ์€ ์ฃผ๋กœ ํ™œ๋™์„ฑ ์€ํ•˜ํ•ต(AGN)์ด๋‚˜ ์Šคํƒ€๋ฒ„์ŠคํŠธ ์€ํ•˜์—์„œ ๋ฐœ๊ฒฌ๋˜์–ด ์™”๋‹ค. ๊ทธ๋Ÿฌ๋‚˜ ์ตœ๊ทผ์—๋Š” ์ผ๋ฐ˜์ ์ธ ์€ํ•˜์—์„œ๋„ ์ด๋Ÿฌํ•œ ๋ฐฉ์ถœ์ด ๊ฐ€๋Šฅํ•˜๋‹ค๋Š” ๊ฐ€์„ค์ด ์ œ๊ธฐ๋˜์—ˆ๋‹ค. ์ด ์—ฐ๊ตฌ์—์„œ๋Š” Local Group ๋‚ด ์ผ๋ฐ˜ ์€ํ•˜๋“ค, ํŠนํžˆ M8

Astrophysics
A conjecture on independent sets and graph covers

A conjecture on independent sets and graph covers

๋ณธ ๋…ผ๋ฌธ์€ ๊ทธ๋ž˜ํ”„ ์ด๋ก ์˜ ํ•ต์‹ฌ ๊ฐœ๋…์ธ ๋…๋ฆฝ ์ง‘ํ•ฉ๊ณผ ์ปค๋ฒ„๋ฅผ ๋‹ค๋ฃจ๋ฉฐ, ํŠนํžˆ M ์ปค๋ฒ„์™€ ๋ฒ ํ…Œ ๊ทผ์‚ฌ(Bethe approximation) ์‚ฌ์ด์˜ ๊ด€๊ณ„๋ฅผ ํƒ๊ตฌํ•œ๋‹ค. ์ด๋Ÿฌํ•œ ์—ฐ๊ตฌ๋Š” ํ†ต๊ณ„ ๋ฌผ๋ฆฌํ•™์—์„œ ์ค‘์š”ํ•œ ์—ญํ• ์„ ํ•˜๋Š” ๋ถ„ํ•  ํ•จ์ˆ˜(partition function)์™€ ์ž์œ  ์—๋„ˆ์ง€(free energy)์— ๋Œ€ํ•œ ์ดํ•ด๋ฅผ ํ™•์žฅํ•˜๋Š” ๋ฐ ๊ธฐ์—ฌํ•œ๋‹ค. 1. ๋‹ค๋ณ€์ˆ˜ ๋…๋ฆฝ ์ง‘ํ•ฉ ๋‹คํ•ญ์‹๊ณผ M ์ปค๋ฒ„ ๋…ผ๋ฌธ์€ ๊ทธ๋ž˜ํ”„ G์˜ ๋‹ค๋ณ€์ˆ˜ ๋…๋ฆฝ ์ง‘ํ•ฉ ๋‹คํ•ญ์‹์„ ์ •์˜ํ•˜๊ณ , ์ด๋ฅผ ํ†ตํ•ด ๋…๋ฆฝ ์ง‘ํ•ฉ์˜ ํฌ๊ธฐ์— ๋”ฐ๋ฅธ ๊ฐ€์ค‘์น˜๋ฅผ ํ‘œํ˜„ํ•œ๋‹ค. ์ด ๋‹คํ•ญ์‹์€ G์˜ ๋ชจ๋“  ๋…๋ฆฝ ์ง‘ํ•ฉ I์— ๋Œ€ํ•ด x^{|I|

Mathematics Computer Science Discrete Mathematics
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Lunar Eclipse of June, 15, 2011: Three-color umbra surface photometry

์ด ๋…ผ๋ฌธ์€ 2011๋…„ 6์›” 15์ผ์— ๋ฐœ์ƒํ•œ ์ด ๋‹ฌ ์‹์„ ๊ด€์ธกํ•˜์—ฌ ์ง€๊ตฌ ๋Œ€๊ธฐ์˜ ๊ด‘ํ•™์  ์„ฑ๋ถ„๊ณผ ๊ทธ ๋ณ€ํ™”๋ฅผ ๋ถ„์„ํ•˜๋Š” ๋ฐ ์ดˆ์ ์„ ๋งž์ถ”๊ณ  ์žˆ๋‹ค. ๋‹ฌ ์‹์€ ํƒœ์–‘์—์„œ ๋ฐœ์‚ฐ๋œ ๋ฐฉ์‚ฌ์„ ์ด ์ง€๊ตฌ ๋Œ€๊ธฐ๋ฅผ ํ†ต๊ณผํ•˜๋ฉด์„œ ๊ตด์ ˆ, ์‚ฐ๋ž€ ๋ฐ ํก์ˆ˜๋˜๋Š” ๊ณผ์ •์„ ๊ด€์ฐฐํ•  ์ˆ˜ ์žˆ๋Š” ์ค‘์š”ํ•œ ๊ธฐํšŒ๋กœ, ์ด๋Š” ๋Œ€๊ธฐ ์กฐ๊ฑด์— ํฌ๊ฒŒ ์˜์กดํ•œ๋‹ค. ๋…ผ๋ฌธ์˜ ํ•ต์‹ฌ ๋‚ด์šฉ์€ ๋‹ค์Œ๊ณผ ๊ฐ™๋‹ค: 1. ๋‹ฌ ์‹์˜ ๊ด‘๋„ ์ธก์ • : ๋‹ฌ ํ‘œ๋ฉด์˜ ๊ด‘๋„๋ฅผ ์ธก์ •ํ•จ์œผ๋กœ์จ ์ง€๊ตฌ ๋Œ€๊ธฐ์˜ ๋‹ค์–‘ํ•œ ๊ณ ๋„์™€ ๊ฒฝ๊ณ„์—์„œ ๋ฐœ์ƒํ•˜๋Š” ๊ตด์ ˆ์„ ํฌ๊ด„ํ•œ๋‹ค. ํŠนํžˆ, 2011๋…„ 6์›” 15์ผ์˜ ์ด ๋‹ฌ ์‹์€ ์ ๋„ ๋ฐ ์—ด๋Œ€ ์ง€์—ญ์˜ ๋Œ€๊ธฐ๋ฅผ ๊ด€์ฐฐํ•  ์ˆ˜ ์žˆ๋Š”

Physics Astrophysics
Performance Measurement of the Heterogeneous Network

Performance Measurement of the Heterogeneous Network

์ด ๋…ผ๋ฌธ์€ M/M/2 ํ ์‹œ์Šคํ…œ์„ ํ™œ์šฉํ•˜์—ฌ ๋„คํŠธ์›Œํฌ ์ง€์—ฐ ๋ฌธ์ œ๋ฅผ ๋ถ„์„ํ•˜๊ณ  ์žˆ์Šต๋‹ˆ๋‹ค. ์ด ๋ชจ๋ธ์€ ๋‘ ๊ฐœ์˜ ์„œ๋ฒ„๋กœ ๊ตฌ์„ฑ๋˜๋ฉฐ, ๊ฐ ์„œ๋ฒ„๋Š” ์„œ๋กœ ๋‹ค๋ฅธ ์ฒ˜๋ฆฌ ๋Šฅ๋ ฅ์„ ๊ฐ€์ง€๊ณ  ์žˆ์–ด ์ž‘์—… ์Šค์ผ€์ค„๋ง ๋ฐฉ์‹์€ FCFS(First Come First Served)์ž…๋‹ˆ๋‹ค. 1. M/M/2 ํ ์‹œ์Šคํ…œ M/M/2 ํ ์‹œ์Šคํ…œ์€ ๋„คํŠธ์›Œํฌ ์ง€์—ฐ ๋ฌธ์ œ๋ฅผ ํšจ๊ณผ์ ์œผ๋กœ ๋ชจ๋ธ๋งํ•˜๊ธฐ ์œ„ํ•œ ๋„๊ตฌ๋กœ, ์ด ์‹œ์Šคํ…œ์˜ ์ฃผ์š” ํŠน์ง• ์ค‘ ํ•˜๋‚˜๋Š” ๋‘ ๊ฐœ์˜ ์„œ๋ฒ„๊ฐ€ ์„œ๋กœ ๋‹ค๋ฅธ ์ฒ˜๋ฆฌ ๋Šฅ๋ ฅ์„ ๊ฐ€์ง€๊ณ  ์žˆ๋‹ค๋Š” ์ ์ž…๋‹ˆ๋‹ค. ์ž‘์—… ์Šค์ผ€์ค„๋ง ๋ฐฉ์‹์€ FCFS๋กœ, ์ž‘์—…์ด ๋„์ฐฉํ•œ ์ˆœ์„œ๋Œ€๋กœ ์ฒ˜๋ฆฌ๋ฉ๋‹ˆ๋‹ค. 2. ์ƒํƒœ

Networking Network Computer Science
X-ray view on a Class using Conceptual Analysis in Java Environment

X-ray view on a Class using Conceptual Analysis in Java Environment

์ด ๋…ผ๋ฌธ์€ ๊ฐœ๋… ๋ถ„์„(Conceptual Analysis, CA)์„ ํ™œ์šฉํ•˜์—ฌ ์†Œํ”„ํŠธ์›จ์–ด ์žฌ๊ณตํ•™์—์„œ์˜ ๋ชจ๋“ˆํ™”์™€ ํด๋ž˜์Šค ๋‚ด๋ถ€ ๊ตฌ์กฐ๋ฅผ ๋ถ„์„ํ•˜๋Š” ๋ฐฉ๋ฒ•์„ ์ œ์‹œํ•˜๊ณ  ์žˆ๋‹ค. ํŠนํžˆ ์ž๋ฐ” ํ™˜๊ฒฝ์—์„œ ์ด๋Ÿฌํ•œ ์ ‘๊ทผ๋ฒ•์„ ์ ์šฉํ•จ์œผ๋กœ์จ, ๊ฐœ๋ฐœ์ž๋“ค์ด ์ฝ”๋“œ์˜ ๋ณต์žก์„ฑ์„ ์ค„์ด๊ณ  ์œ ์ง€๋ณด์ˆ˜์„ฑ์„ ํ–ฅ์ƒ์‹œํ‚ค๋Š” ๋ฐ ๋„์›€์ด ๋˜๋„๋ก ์„ค๊ณ„๋˜์—ˆ๋‹ค. ๊ฐœ๋… ๋ถ„์„๊ณผ X Ray ๋ทฐ ๊ฐœ๋… ๋ถ„์„์€ ์š”์†Œ๋“ค ๊ฐ„์˜ ๊ณตํ†ต ์†์„ฑ์— ๊ธฐ๋ฐ˜ํ•˜์—ฌ ์˜๋ฏธ ์žˆ๋Š” ์ง‘๋‹จ์„ ์‹๋ณ„ํ•˜๋Š” ์ด๋ก ์  ์ ‘๊ทผ๋ฒ•์ด๋‹ค. ์ด๋Ÿฌํ•œ ์ง‘๋‹จ์€ '๊ฐœ๋…'์œผ๋กœ ๋ถˆ๋ฆฌ๋ฉฐ, ๊ฐ๊ฐ์˜ ๊ฐœ๋…์€ ํŠน์ • ์†์„ฑ์„ ๊ณต์œ ํ•œ๋‹ค. ๋…ผ๋ฌธ์—์„œ๋Š” X Ray ๋ทฐ๋ผ๋Š” ๊ธฐ๋ฒ•์„ ์†Œ๊ฐœํ•˜๋Š”๋ฐ

Analysis Software Engineering Computer Science
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Structure of lexicographic Groebner bases in three variables of ideals of dimension zero

: ์„œ๋ก  ๋ฐ ์—ฐ๊ตฌ ๋ฐฐ๊ฒฝ ๋…ผ๋ฌธ์€ ๋‹ค๋ณ€์ˆ˜ ๋‹คํ•ญ์‹ ๋ฐ˜ํ™˜์˜ ์ œ๋กœ ์ฐจ์› ์ด์ƒ์ ๊ณผ ๊ทธ๋กœ๋ธŒ๋„ˆ ๊ธฐ์ €์— ์ดˆ์ ์„ ๋งž์ถ”๊ณ  ์žˆ๋‹ค. ํŠนํžˆ, 3๊ฐœ ๋ณ€์ˆ˜ x , y , z ๋ฅผ ์‚ฌ์šฉํ•˜๋Š” ๋‹คํ•ญ์‹ ๋ฐ˜ํ™˜ R

Symbolic Computation Computer Science
A Variant of Azumas Inequality for Martingales with Subgaussian Tails

A Variant of Azumas Inequality for Martingales with Subgaussian Tails

๋ณธ ๋…ผ๋ฌธ์€ Azuma ๋ถ€๋“ฑ์‹์˜ ๋ณ€ํ˜•์— ๋Œ€ํ•ด ๊นŠ์ด ์žˆ๊ฒŒ ๋ถ„์„ํ•˜๊ณ  ์žˆ๋‹ค. ๊ธฐ์กด Azuma ๋ถ€๋“ฑ์‹์€ ํ™•๋ฅ ์  ๊ณผ์ •์—์„œ ์ค‘์š”ํ•œ ์—ญํ• ์„ ํ•˜๋Š”๋ฐ, ํŠนํžˆ ๋งˆ๋ฅดํŒ…์•Œ์˜ ์ˆ˜๋ ด์„ฑ์„ ๋ณด์žฅํ•˜๋Š” ๊ฐ•๋ ฅํ•œ ๋„๊ตฌ์ด๋‹ค. ๊ทธ๋Ÿฌ๋‚˜ ์ด ๋ถ€๋“ฑ์‹์€ ๋ชจ๋“  ์‹œ๊ฐ„ t์— ๋Œ€ํ•ด |Zt|๊ฐ€ ์ƒ์ˆ˜ b ์ด๋‚ด๋กœ ์ œํ•œ๋˜์–ด์•ผ ํ•œ๋‹ค๋Š” ์—„๊ฒฉํ•œ ๊ฐ€์ •์„ ํ•„์š”๋กœ ํ•˜๋ฉฐ, ์ด๋Š” ์‹ค์ œ ๋ฌธ์ œ์—์„œ ์ ์šฉํ•˜๊ธฐ ์–ด๋ ค์šด ๊ฒฝ์šฐ๊ฐ€ ๋งŽ๋‹ค. ๋ณธ ๋…ผ๋ฌธ์—์„œ๋Š” ์ด๋Ÿฌํ•œ ํ•œ๊ณ„๋ฅผ ๊ทน๋ณตํ•˜๊ณ ์ž ๋งˆ๋ฅดํŒ…์•Œ์˜ ๊ฐ ํ•ญ์ด ๊ณ ํ™•๋ฅ ๋กœ ํฐ ๊ฐ’์„ ๊ฐ€์ง€๋”๋ผ๋„ Azuma ๋ถ€๋“ฑ์‹์„ ์ผ๋ฐ˜ํ™”ํ•˜๋Š” ์ƒˆ๋กœ์šด ๋ณ€ํ˜•์„ ์ œ์‹œํ•œ๋‹ค. ์ด๋ฅผ ํ†ตํ•ด, '๊ฑฐ์˜ ๊ฒฝ๊ณ„๊ฐ€ ์žˆ๋Š”' ๋งˆ๋ฅดํŒ…์•Œ์—

Mathematics Machine Learning Computer Science
Comment on 'The separation of variables and bifurcations of first   integrals in one problem of D.N.Goryachev' by Pavel E. Ryabov   (Archive:1102.2588v1)

Comment on 'The separation of variables and bifurcations of first integrals in one problem of D.N.Goryachev' by Pavel E. Ryabov (Archive:1102.2588v1)

: ๋ณธ ๋…ผ๋ฌธ์€ Goryachev ์‹œ์Šคํ…œ์— ๋Œ€ํ•œ ๋ณ€์ˆ˜ ๋ถ„๋ฆฌ์™€ ์ฒซ ๋ฒˆ์งธ ํ†ตํ•ฉ์˜ ๋ถ„๊ธฐ๋ฅผ ๋‹ค๋ฃจ๋ฉฐ, ํŠนํžˆ ๊ฒŒ์˜ค๋ฉ”ํŠธ๋ฆญ ์นผ๋ผ๋ชจํ”„ ๋ฐฉ๋ฒ•์ด ์ ์šฉ๋  ๋•Œ ๋น„์ปค๋„ '์ƒˆ๋กœ์šด ๋ณ€์ˆ˜ ๋ถ„๋ฆฌ'๊ฐ€ ๋ฐœ์ƒํ•œ๋‹ค๋Š” ๊ฒƒ์„ ์ฆ๋ช…ํ•œ๋‹ค. ์ด ์—ฐ๊ตฌ๋Š” Goryachev ์‹œ์Šคํ…œ์„ ์„ค๋ช…ํ•˜๊ธฐ ์œ„ํ•ด ๊ฐ์šด๋™๋Ÿ‰ ๋ฒกํ„ฐ M๊ณผ ํฌ์•„์†ก ๋ฒกํ„ฐ ฮฑ๋ฅผ ์‚ฌ์šฉํ•˜๋ฉฐ, ์ด๋ฅผ ํ†ตํ•ด eโˆ—(3) ๋ฆฌ ํฌ์•„์†ก ๋ธŒ๋ž˜ํ‚ท๊ณผ ์—ฐ๊ด€๋œ ํฌ์•„์†ก ๋ธŒ๋ž˜ํ‚ท์„ ์ •์˜ํ•œ๋‹ค. ์ด๋Ÿฌํ•œ ์ ‘๊ทผ๋ฒ•์€ Goryachev ์‹œ์Šคํ…œ์˜ ๋™์—ญํ•™์  ํŠน์„ฑ์„ ์ดํ•ดํ•˜๋Š” ๋ฐ ์ค‘์š”ํ•œ ์—ญํ• ์„ ํ•œ๋‹ค. ๋…ผ๋ฌธ์—์„œ ์ €์ž๋Š” ๋‘ ๋ณด์กด๋Ÿ‰ H์™€ K ์‚ฌ์ด์˜ ์ƒํ˜ธ์ž‘์šฉ์„ ๋ถ„์„ํ•˜๊ณ , ์ด๋“ค ๊ฐ„์˜ ๊ด€

Nonlinear Sciences
Massive non-thermal radio emitters: new data and their modelling

Massive non-thermal radio emitters: new data and their modelling

๋ณธ ๋…ผ๋ฌธ์€ ๋Œ€์งˆ๋Ÿ‰ ๋ณ„, ํŠนํžˆ Wolf Rayet ๋ฐ OB ์œ ํ˜•์˜ ๋ณ„๋“ค์ด ๋น„์—ด์  ๋ผ๋””์˜ค ๋ฐฉ์ถœ์„ ๋‚˜ํƒ€๋‚ด๋Š” ํ˜„์ƒ์„ ๋‹ค๋ฃจ๊ณ  ์žˆ๋‹ค. ์ด ๋น„์—ด์  ๋ณต์‚ฌ๋Š” ์ถฉ๋Œ ์—†๋Š” ์ถฉ๊ฒฉ์—์„œ ์ƒ๋Œ€๋ก ์  ์ „์ž๊ฐ€ ๊ฐ€์†๋˜์–ด ์ƒ์„ฑ๋˜๋Š” ํŽ˜๋ฅด๋ฏธ ๋ฉ”์ปค๋‹ˆ์ฆ˜์— ์˜ํ•ด ๋ฐœ์ƒํ•œ๋‹ค. ์ด๋ก  ๋ชจ๋ธ(Eichler & Usov, 1993)์€ ์ด๋Ÿฌํ•œ ์ถฉ๊ฒฉ์ด ๋ฐฉ์‚ฌ๋ ฅ์ ์œผ๋กœ ์ฃผ๋„๋˜๋Š” ๋ฐ”๋žŒ์ด ์Œ์„ฑ ๋˜๋Š” ๋‹ค์ค‘ ์‹œ์Šคํ…œ์—์„œ ์ถฉ๋Œํ•˜์—ฌ ๋ฐœ์ƒํ•œ๋‹ค๋Š” ๊ฒƒ์„ ์ œ์‹œํ•˜๊ณ  ์žˆ๋‹ค. Cyg OB2 No. 9๋Š” O5 + O6 7 ์Œ์„ฑ์œผ๋กœ, Van Loo ๋“ฑ (2008)์€ ์ด ๋ณ„์˜ ๋ผ๋””์˜ค ๋ณต์‚ฌ ๋ฐ์ดํ„ฐ๊ฐ€ ์•ฝ 2.355๋…„์˜ ์ฃผ๊ธฐ๋กœ ๋ณ€

Model Astrophysics Data
Can Mathisson-Papapetrou equations give clue to some problems in   astrophysics?

Can Mathisson-Papapetrou equations give clue to some problems in astrophysics?

๋งค๋ ฅ์ ์ธ ํ•œ๊ธ€ ์ œ๋ชฉ: ํŽ˜๋ฅด๋ฏธ ์šด์†ก๊ณผ ๋งˆ์‹œ๋ชฌ ํŒŒํŒŒํŽ˜ํŠธ๋กœ ๋ฐฉ์ •์‹: ์ฒœ์ฒด๋ฌผ๋ฆฌํ•™์  ํ•จ์˜ ์ดˆ๋ก ์ „์ฒด ๋ฒˆ์—ญ ๋ฐ ์ •๋ฆฌ: ๋ณธ ๋…ผ๋ฌธ์€ Mathisson Papapetrou (MPD) ๋ฐฉ์ •์‹์ด ํšŒ์ „ํ•˜๋Š” ์ž…์ž์˜ ์ผ๋ฐ˜ ์ƒ๋Œ€์„ฑ ์ด๋ก ์  ์šด๋™์„ ์„ค๋ช…ํ•˜๋ฉฐ, ํŠนํžˆ ๊ณ ์†์œผ๋กœ ํšŒ์ „ํ•˜๋Š” ์ž…์ž์—์„œ ๋‚˜ํƒ€๋‚˜๋Š” ๊ฐ•ํ•œ ํ•ญ์ค‘๋ ฅ ํšจ๊ณผ๋ฅผ ๋ถ„์„ํ•ฉ๋‹ˆ๋‹ค. ์ด๋Ÿฌํ•œ ํŠน์„ฑ์ด ์ฒœ์ฒด๋ฌผ๋ฆฌํ•™์  ํ˜„์ƒ, ์˜ˆ๋ฅผ ๋“ค์–ด OPERA ์‹คํ—˜ ๊ฒฐ๊ณผ์™€ ์—ฐ๊ด€๋  ์ˆ˜ ์žˆ๋‹ค๋Š” ๊ฐ€๋Šฅ์„ฑ์„ ์ œ์•ˆํ•˜๊ณ  ์žˆ์Šต๋‹ˆ๋‹ค. ๋…ผ๋ฌธ์€ MPD ๋ฐฉ์ •์‹์ด ์ผ๋ฐ˜ ์ƒ๋Œ€์„ฑ ์ด๋ก ์  ๋””๋ž™ ๋ฐฉ์ •์‹์˜ ๊ณ ์ „์  ๊ทผ์‚ฌ์น˜์ž„์„ ๊ฐ•์กฐํ•˜๋ฉฐ, ํŽ˜๋ฅด๋ฏธ ์šด๋ฐ˜ ๊ฐœ๋…์„ ํ†ตํ•ด ์ •ํ™•ํ•œ ์ผ

HEP-TH General Relativity Astrophysics
Could Dense Quark Matter be a Source of Super High Energy Cosmic Rays?

Could Dense Quark Matter be a Source of Super High Energy Cosmic Rays?

1. ์ดˆ๊ณ ์—๋„ˆ์ง€ ์šฐ์ฃผ์„ ์˜ ์›์ฒœ ๋ฌธ์ œ ์ดˆ๊ณ ์—๋„ˆ์ง€ ์šฐ์ฃผ์„ ์€ ์šฐ์ฃผ์˜ ๋ฐœ์ƒ๊ณผ ์ง„ํ™”์— ๋Œ€ํ•œ ์ค‘์š”ํ•œ ์ •๋ณด๋ฅผ ์ œ๊ณตํ•  ์ˆ˜ ์žˆ์ง€๋งŒ, ๊ทธ ์ถœ์ฒ˜๋Š” ์—ฌ์ „ํžˆ ๋ฏธ์Šคํ„ฐ๋ฆฌ๋กœ ๋‚จ์•„ ์žˆ์Šต๋‹ˆ๋‹ค. ์ง€์ƒ ์‹คํ—˜์‹ค์—์„œ๋Š” ์ด๋Ÿฌํ•œ ์—๋„ˆ์ง€ ๋ฒ”์œ„(10^17 18 eV ์ด์ƒ)์˜ ์ž…์ž ๋น”์„ ์žฌํ˜„ํ•˜๋Š” ๊ฒƒ์ด ๋ถˆ๊ฐ€๋Šฅํ•˜๊ธฐ ๋•Œ๋ฌธ์—, ์ดˆ๊ณ ์—๋„ˆ์ง€ ์šฐ์ฃผ์„ ์€ ์ด๋“ค ์ž…์ž์˜ ์ƒํ˜ธ์ž‘์šฉ์„ ์—ฐ๊ตฌํ•  ์ˆ˜ ์žˆ๋Š” ์œ ์ผํ•œ ์ž์›์ž…๋‹ˆ๋‹ค. ๊ทธ๋Ÿฌ๋‚˜ ํ˜„์žฌ๊นŒ์ง€ ์ œ์‹œ๋œ ๋ณ„ ์ƒ์„ฑ ๋ชจ๋ธ๋“ค์€ ์ด๋Ÿฌํ•œ ์—๋„ˆ์ง€ ๋ฒ”์œ„๋ฅผ ๊ฐ€์†ํ™”ํ•˜๋Š” ๋ฐ ํ•„์š”ํ•œ ๊ฐ•๋ ฅํ•œ ์ „์ž๊ธฐ์žฅ์ด ๋ถ€์กฑํ•˜๋‹ค๋Š” ์ด๋ก ์  ์˜ˆ์ธก์ด ์žˆ์Šต๋‹ˆ๋‹ค. 2. ๋ฐ€๋„ ๋†’์€ ์ฟผํฌ ๋ฌผ์งˆ์˜ ๊ฐ€๋Šฅ์„ฑ ๋…ผ๋ฌธ์—์„œ๋Š”

Physics Astrophysics
Maximizing the Cohesion is NP-hard

Maximizing the Cohesion is NP-hard

๋ณธ ๋…ผ๋ฌธ์˜ ์ฃผ์š” ๋ชฉํ‘œ๋Š” ์‚ฌํšŒ ๋„คํŠธ์›Œํฌ ๋ถ„์„์—์„œ ์ค‘์š”ํ•œ ์—ญํ• ์„ ํ•˜๋Š” '๊ฒฐ์†์„ฑ'์ด๋ผ๋Š” ์ƒˆ๋กœ์šด ์ง€ํ‘œ๋ฅผ ๋„์ž…ํ•˜๊ณ , ์ด ์ง€ํ‘œ๋ฅผ ์‚ฌ์šฉํ•˜์—ฌ ๊ทธ๋ž˜ํ”„ ๋‚ด์—์„œ ์ตœ๋Œ€ ๊ฒฐ์†์„ฑ์„ ๊ฐ–๋Š” ์ง‘ํ•ฉ์„ ์ฐพ๋Š” ๋ฌธ์ œ๊ฐ€ NP ํ•˜๋“œ์ž„์„ ์ฆ๋ช…ํ•˜๋Š” ๊ฒƒ์ด๋‹ค. ์ด๋ฅผ ํ†ตํ•ด ์‚ฌํšŒ ๋„คํŠธ์›Œํฌ ๋ถ„์„์˜ ๋ณต์žก์„ฑ์„ ์ดํ•ดํ•˜๊ณ , ํšจ์œจ์ ์ธ ์•Œ๊ณ ๋ฆฌ์ฆ˜ ๊ฐœ๋ฐœ์— ๋Œ€ํ•œ ํ•„์š”์„ฑ๊ณผ ํ•œ๊ณ„๋ฅผ ํŒŒ์•…ํ•  ์ˆ˜ ์žˆ๋‹ค. 1. ๊ฒฐ์†์„ฑ ์ง€ํ‘œ์˜ ๋„์ž… ๋ฐ ์‹คํ—˜์  ๊ฒ€์ฆ ๊ฒฐ์†์„ฑ์€ ์‚ฌํšŒ ๋„คํŠธ์›Œํฌ ๋‚ด์—์„œ ์ง‘๋‹จ์˜ ์ผ์ฒด๊ฐ์„ ์ธก์ •ํ•˜๋Š” ์ƒˆ๋กœ์šด ์ง€ํ‘œ๋กœ, ์ด๋Š” ์‚ฌ์šฉ์ž ์ฃผ๊ด€์  ์ปค๋ฎค๋‹ˆํ‹ฐ ์ธ์‹๊ณผ ๋†’์€ ์ƒ๊ด€๊ด€๊ณ„๋ฅผ ๊ฐ€์ง์„ ํŽ˜์ด์Šค๋ถ ์‹คํ—˜์„ ํ†ตํ•ด ํ™•์ธํ•˜์˜€๋‹ค. ์ด

Networking Computational Complexity Computer Science
Restricted Parameter Range Promise Set Cover Problems Are Easy

Restricted Parameter Range Promise Set Cover Problems Are Easy

: ๋ณธ ๋…ผ๋ฌธ์€ ์„ธํŠธ ์ปค๋ฒ„ ๋ฌธ์ œ์˜ ๋ณ€ํ˜• ์ค‘ ํ•˜๋‚˜์ธ k ๊ท ์ผ ํ•˜์ดํผ๊ทธ๋ž˜ํ”„์—์„œ์˜ ์ •์  ๋ฎ๊ฐœ ๋ฌธ์ œ์— ์ดˆ์ ์„ ๋งž์ถ”๊ณ  ์žˆ์Šต๋‹ˆ๋‹ค. ์ด ๋ฌธ์ œ๋Š” ๊ณ ์ „์ ์ธ ์„ธํŠธ ์ปค๋ฒ„ ๋ฌธ์ œ์™€ ์œ ์‚ฌํ•˜์ง€๋งŒ, ๊ฐ ์—ฃ์ง€๊ฐ€ ์ •ํ™•ํžˆ k๊ฐœ์˜ ์›์†Œ๋ฅผ ํฌํ•จํ•˜๋Š” ํŠน์„ฑ์„ ๊ฐ€์ง‘๋‹ˆ๋‹ค. ๋…ผ๋ฌธ์€ ๋‘ ๊ฐ€์ง€ ์ฃผ์š” ๊ฒฐ๊ณผ๋ฅผ ์ œ์‹œํ•ฉ๋‹ˆ๋‹ค: ์ฒซ์งธ๋กœ, YES ์ธ์Šคํ„ด์Šค์—์„œ ์ •์ˆ˜ ๋ฒกํ„ฐ L(B)๋Š” n๊ฐœ์˜ ๋น„์˜ ์š”์†Œ๋ฅผ ๊ฐ–๋Š”๋‹ค๋Š” ๊ฒƒ์ž…๋‹ˆ๋‹ค. ์ด๋Š” ์ •ํ™•ํ•œ ๋ฎ๊ฐœ๊ฐ€ ์กด์žฌํ•จ์„ ์˜๋ฏธํ•˜๋ฉฐ, ์ด๋ฅผ ํ†ตํ•ด ๋ฌธ์ œ์˜ ํ•ด๊ฒฐ ๊ฐ€๋Šฅ์„ฑ์„ ํ™•์ธํ•  ์ˆ˜ ์žˆ์Šต๋‹ˆ๋‹ค. ๋‘˜์งธ๋กœ, NO ์ธ์Šคํ„ด์Šค์—์„œ๋Š” L(B)๊ฐ€ ์ตœ๋Œ€ 2(nฮท(m)d)๊ฐœ์˜ ๋น„์˜ ์š”์†Œ๋งŒ ๊ฐ€์ง‘๋‹ˆ๋‹ค

Computational Complexity Computer Science
The quadratic WDVV solution $E_8(a_1)$

The quadratic WDVV solution $E_8(a_1)$

์ด ๋…ผ๋ฌธ์€ ๊ณ ์ฐจ์› ๋ฆฌ ๋Œ€์ˆ˜์™€ ํ”„๋กœ๋ฒค๋ฆฌ์šฐ์Šค ๋งŒ๋Œ(Frobenius Manifold) ์‚ฌ์ด์˜ ๊นŠ์€ ๊ด€๊ณ„๋ฅผ ํƒ๊ตฌํ•ฉ๋‹ˆ๋‹ค. ํŠนํžˆ, Eโ‚ˆ(aโ‚)๋ผ๋Š” ํŠน์ •ํ•œ ๊ฒฝ์šฐ์— ์ดˆ์ ์„ ๋งž์ถ”๊ณ  ์žˆ์Šต๋‹ˆ๋‹ค. ์ด ์—ฐ๊ตฌ๋Š” Witten Dijkgraaf Verlinde Verlinde (WDVV) ๋ฐฉ์ •์‹์ด๋ผ๋Š” ์ค‘์š”ํ•œ ํŽธ๋ฏธ๋ถ„ ๋ฐฉ์ •์‹ ์‹œ์Šคํ…œ์˜ ํ•ด๋ฅผ ๊ตฌ์„ฑํ•˜๋Š” ๋ฐฉ๋ฒ•์„ ํƒ๊ตฌํ•ฉ๋‹ˆ๋‹ค. ํ”„๋กœ๋ฒค๋ฆฌ์šฐ์Šค ๋งŒ๋Œ์€ ๋Œ€์ˆ˜์  ๊ตฌ์กฐ์™€ ๊ธฐํ•˜ํ•™์  ๊ตฌ์กฐ๊ฐ€ ๊ฒฐํ•ฉ๋œ ๋ณต์žกํ•œ ์ˆ˜ํ•™์  ๊ฐ์ฒด์ž…๋‹ˆ๋‹ค. ์ด ๋…ผ๋ฌธ์—์„œ๋Š” ์ด๋Ÿฌํ•œ ๊ตฌ์กฐ๊ฐ€ ์–ด๋–ป๊ฒŒ Eโ‚ˆ ๋ฆฌ ๋Œ€์ˆ˜์™€ ์—ฐ๊ฒฐ๋˜๋Š”์ง€, ๊ทธ๋ฆฌ๊ณ  ๊ทธ ์ž ์žฌ ํ•จ์ˆ˜๋Š” ์–ด๋–ค ํ˜•ํƒœ๋ฅผ ๊ฐ€์ง€๋Š”์ง€๋ฅผ ๋ถ„

MATH-PH Mathematics Nonlinear Sciences
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Partition function of 1-, 2-, and 3-D monatomic ideal gas: A simple and comprehensive review

๋ณธ ๋…ผ๋ฌธ์€ ์›์ž ๊ธฐ์ฒด์˜ ๋ถ„ํ•  ํ•จ์ˆ˜๋ฅผ 1์ฐจ์›, 2์ฐจ์›, ๊ทธ๋ฆฌ๊ณ  3์ฐจ์›์—์„œ ๊ฐ๊ฐ ํƒ๊ตฌํ•˜๊ณ  ์ด๋ฅผ ํ†ตํ•ด ์ฐจ์›์— ๋”ฐ๋ฅธ ๊ณตํ†ต์ ๊ณผ ์ฐจ์ด์ ์„ ๋ถ„์„ํ•œ๋‹ค. ์ด ์—ฐ๊ตฌ๋Š” ๊ณ ์ „์ ์ธ ๋ฌผ๋ฆฌํ•™์  ์ ‘๊ทผ ๋ฐฉ์‹์„ ๋ฐ”ํƒ•์œผ๋กœ ํ•˜๋ฉฐ, ํŠนํžˆ ๋งฅ์Šค์›ฐ ๋ณผ์ธ ๋งŒ ํ†ต๊ณ„ํ•™์˜ ์›๋ฆฌ๋ฅผ ํ™œ์šฉํ•˜์—ฌ ์ž…์ž์˜ ์ƒํƒœ ์ˆ˜์™€ ์—๋„ˆ์ง€ ๊ฐ„์˜ ๊ด€๊ณ„๋ฅผ ์ •๋ฆฝํ•˜๊ณ  ์ด๋ฅผ ํ†ตํ•ด ๋ถ„ํ•  ํ•จ์ˆ˜๋ฅผ ๋„์ถœํ•˜๋Š” ๋ฐฉ๋ฒ•๋ก ์„ ์ œ์‹œํ•œ๋‹ค. 1. ์ด๋ก ์  ๋ฐฐ๊ฒฝ ๋…ผ๋ฌธ์€ ฮ“ ํ†ตํ•ฉ๊ณผ ๋งฅ์Šค์›ฐ ๋ณผ์ธ ๋งŒ ํ†ต๊ณ„ํ•™์— ๋Œ€ํ•œ ์ดํ•ด๊ฐ€ ํ•„์š”ํ•˜๋‹ค๋Š” ์ ์—์„œ ์ถœ๋ฐœํ•œ๋‹ค. ์ด๋Ÿฌํ•œ ์ˆ˜ํ•™์  ๊ธฐ๋ฐ˜ ์œ„์—์„œ, ์›์ž ๊ธฐ์ฒด์˜ ๋ถ„ํ•  ํ•จ์ˆ˜๋ฅผ ๊ณ„์‚ฐํ•˜๋Š” ๋ฐฉ๋ฒ•์„ ํƒ๊ตฌํ•œ๋‹ค. ์ด๋ก ์ ์œผ๋กœ, ๋ถ„ํ• 

Condensed Matter Physics
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Returns in futures markets and $nu=3$ t-distribution

๋ณธ ๋…ผ๋ฌธ์€ ๊ณ ์ฃผํŒŒ๋กœ ์ƒ˜ํ”Œ๋ง๋œ ๊ธˆ์œต ์‹œ๊ฐ„ ์‹œ๋ฆฌ์ฆˆ์˜ ๋กœ๊ทธ ๋ฐ˜ํ™˜ ํ™•๋ฅ  ๋ถ„ํฌ๋ฅผ ๋ถ„์„ํ•˜๊ณ , ์ด๋ฅผ ํ†ตํ•ด t ๋ถ„ํฌ๊ฐ€ ์‹ค์ œ ๋ฐ์ดํ„ฐ์™€ ์–ผ๋งˆ๋‚˜ ์ž˜ ์ผ์น˜ํ•˜๋Š”์ง€ ๊ฒ€์ฆํ•ฉ๋‹ˆ๋‹ค. ์ด ์—ฐ๊ตฌ๋Š” ์–‘์  ๊ธˆ์œต์—์„œ ์ค‘์š”ํ•œ ์—ญํ• ์„ ํ•˜๋Š” ๋กœ๊ทธ ๋ฐ˜ํ™˜ ๋ถ„ํฌ์— ๋Œ€ํ•œ ๊นŠ์ด ์žˆ๋Š” ์ดํ•ด๋ฅผ ์ œ๊ณตํ•˜๋ฉฐ, ํŠนํžˆ ฮฝ โ‰ˆ 3์ธ t ๋ถ„ํฌ์˜ ์ค‘์š”์„ฑ์„ ๊ฐ•์กฐํ•ฉ๋‹ˆ๋‹ค. 1. ๊ธˆ์œต ์‹œ๊ฐ„ ์‹œ๋ฆฌ์ฆˆ์™€ ๋กœ๊ทธ ๋ฐ˜ํ™˜ ๊ธˆ์œต ์‹œ๊ฐ„ ์‹œ๋ฆฌ์ฆˆ๋Š” ๊ฐ€๊ฒฉ ๋ณ€๋™์„ ๋‚˜ํƒ€๋‚ด๋ฉฐ, ์ด ๋ณ€๋™์€ ๋กœ๊ทธ ๋ฐ˜ํ™˜ x(t) log

Quantitative Finance
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Next-to-next-to-leading order post-Newtonian spin(1)-spin(2) Hamiltonian for self-gravitating binaries

: ๋ณธ ๋…ผ๋ฌธ์€ ๊ณ ์† ์ž์ „ํ•˜๋Š” ๋ฐ€๋„ ๋†’์€ ๋ฌผ์ฒด ๊ฐ„์˜ ์ƒํ˜ธ์ž‘์šฉ์— ๋Œ€ํ•œ ํฌ์ŠคํŠธ๋‰ดํ„ด(PN) ์Šคํ•€(1) ์Šคํ•€(2) ํ•ด๋ฐ€ํ† ๋‹ˆ์•ˆ์„ ์œ ๋„ํ•˜๊ณ  ๋ถ„์„ํ•ฉ๋‹ˆ๋‹ค. ์ด ์—ฐ๊ตฌ๋Š” ์ผ๋ฐ˜ ์ƒ๋Œ€์„ฑ ์ด๋ก ์—์„œ ๋‘ ๋ฌผ์ฒด๊ฐ€ ๊ณ ์†์œผ๋กœ ํšŒ์ „ํ•  ๋•Œ์˜ ๋™์—ญํ•™์  ํ–‰๋™์„ ์ดํ•ดํ•˜๋Š” ๋ฐ ์ค‘์š”ํ•œ ์—ญํ• ์„ ํ•ฉ๋‹ˆ๋‹ค. 1. ์—ฐ๊ตฌ ๋ฐฐ๊ฒฝ ๋ฐ ๋ชฉ์  ๋ณธ ๋…ผ๋ฌธ์€ ๊ธฐ์กด์˜ ์Šคํ•€ ์ƒํ˜ธ์ž‘์šฉ์— ๋Œ€ํ•œ ์—ฐ๊ตฌ๋ฅผ ํ™•์žฅํ•˜๊ณ , ํŠนํžˆ 4PN ์ˆœ์„œ๊นŒ์ง€ ๊ณ„์‚ฐ๋œ ํ•ด๋ฐ€ํ† ๋‹ˆ์•ˆ์„ ์ œ์‹œํ•ฉ๋‹ˆ๋‹ค. ์ด๋Š” ๋‘ ๋ฌผ์ฒด๊ฐ€ ๊ณ ์†์œผ๋กœ ํšŒ์ „ํ•˜๋Š” ๊ฒฝ์šฐ์— ์ ์šฉ๋˜๋ฉฐ, ์ผ๋ฐ˜ ์ƒ๋Œ€์„ฑ ์ด๋ก ์—์„œ์˜ ๊ทผ์‚ฌ์น˜์ธ ํฌ์ŠคํŠธ๋‰ดํ„ด(PN) ์ ‘๊ทผ๋ฒ•์„ ์‚ฌ์šฉํ•˜์—ฌ ์œ ๋„๋ฉ๋‹ˆ๋‹ค. 2. ์—ฐ๊ตฌ ๋ฐฉ

HEP-TH General Relativity Astrophysics
A Novel comprehensive method for real time Video Motion Detection   Surveillance

A Novel comprehensive method for real time Video Motion Detection Surveillance

๋ณธ ๋…ผ๋ฌธ์€ ์ €๋ ดํ•˜๊ณ  ํšจ์œจ์ ์ธ ์‹ค์‹œ๊ฐ„ ๋น„๋””์˜ค ๋ชจ์…˜ ๊ฐ์ง€ ๋ณด์•ˆ ์‹œ์Šคํ…œ(VMDss)์˜ ์„ค๊ณ„์™€ ๊ตฌํ˜„์„ ๋‹ค๋ฃจ๊ณ  ์žˆ๋‹ค. ์ด ์‹œ์Šคํ…œ์€ ์‚ฌ์šฉ์ž ์นœํ™”์ ์ด๊ณ  ์›๊ฒฉ ์ œ์–ด๊ฐ€ ๊ฐ€๋Šฅํ•˜๋ฉฐ, ๋ฏธ๋ฆฌ ์ •์˜๋œ ์ƒ‰์ƒ ๊ฐ์ฒด ์ถ”์  ๊ธฐ๋Šฅ์„ ํฌํ•จํ•˜๊ณ  ์žˆ์–ด ๋‹ค์–‘ํ•œ ํ™˜๊ฒฝ์—์„œ ์œ ์šฉํ•˜๊ฒŒ ํ™œ์šฉ๋  ์ˆ˜ ์žˆ๋‹ค. 1. ์‹œ์Šคํ…œ ๊ตฌ์„ฑ ์ „์†ก ์„น์…˜ : ์ปดํ“จํ„ฐ, RS232 ์ธํ„ฐํŽ˜์ด์Šค, ๋งˆ์ดํฌ๋กœ์ปจํŠธ๋กค๋Ÿฌ, RF ์†ก์‹ ๊ธฐ, RF ๋น„๋””์˜ค ์ˆ˜์‹ ๊ธฐ๋กœ ๊ตฌ์„ฑ๋˜์–ด ์žˆ์œผ๋ฉฐ, ์ด๋“ค ์š”์†Œ๋Š” ์‹œ๊ฐ ์ •๋ณด๋ฅผ ์ˆ˜์ง‘ํ•˜๊ณ  ์ œ์–ด ์‹ ํ˜ธ๋ฅผ ์ „์†กํ•˜๋Š” ์—ญํ• ์„ ์ˆ˜ํ–‰ํ•œ๋‹ค. ์ˆ˜์‹  ์„น์…˜ : ๋ชจ๋ฐ”์ผ ํ”Œ๋žซํผ, RF ์ˆ˜์‹ ๊ธฐ, ๋งˆ์ดํฌ๋กœ์ปจํŠธ๋กค๋Ÿฌ, RF ์นด๋ฉ”

Detection Computer Science Computer Vision
Education and Outreach in Particle Physics

Education and Outreach in Particle Physics

๋ณธ ๋…ผ๋ฌธ์€ ๊ณผํ•™, ํŠนํžˆ ์ž…์ž ๋ฌผ๋ฆฌํ•™ ๋ถ„์•ผ์—์„œ ๊ต์œก ๋ฐ ํ™๋ณด ํ™œ๋™์˜ ์ค‘์š”์„ฑ์„ ๊ฐ•์กฐํ•˜๋ฉฐ, ์ด๋ฅผ ํ†ตํ•ด ๋Œ€์ค‘์—๊ฒŒ ๊ณผํ•™์˜ ์•„๋ฆ„๋‹ค์›€๊ณผ ๊ฒฝ์ด๋กœ์›€์„ ์ „๋‹ฌํ•˜๋Š” ๋ฐฉ๋ฒ•์— ๋Œ€ํ•ด ์‹ฌ๋„ ์žˆ๊ฒŒ ๋‹ค๋ฃจ๊ณ  ์žˆ๋‹ค. ๋…ผ๋ฌธ์€ ๋‹ค์–‘ํ•œ ํ”„๋กœ๊ทธ๋žจ๊ณผ ์‚ฌ๋ก€๋ฅผ ํ†ตํ•ด ์ž…์ž ๋ฌผ๋ฆฌํ•™์˜ ๊ต์œก ๋ฐ ํ™๋ณด ํ™œ๋™์˜ ํšจ๊ณผ์„ฑ์„ ๊ฒ€์ฆํ•˜๊ณ , ์ด๋ฅผ ํ†ตํ•ด ๋ฏธ๋ž˜ ๊ณผํ•™ ๊ต์œก ๋ฐ ๋Œ€์ค‘ํ™” ๋ฐฉํ–ฅ์„ ์ œ์‹œํ•œ๋‹ค. 1. ๊ณผํ•™์˜ ์•„๋ฆ„๋‹ค์›€ ์ „๋‹ฌ ๋…ผ๋ฌธ์€ ๊ณผํ•™์˜ ์•„๋ฆ„๋‹ค์›€๊ณผ ๊ฒฝ์ด๋กœ์›€์„ ์ „๋‹ฌํ•˜๋Š” ๊ฒƒ์ด ํ•ต์‹ฌ ๋ชฉํ‘œ์ž„์„ ๊ฐ•์กฐํ•œ๋‹ค. ์ด๋ฅผ ์œ„ํ•ด, ๊ณผ๊ฑฐ์™€ ํ˜„์žฌ ์ƒํ™ฉ์— ๋Œ€ํ•œ ์ดํ•ด๋ฅผ ๋ฐ”ํƒ•์œผ๋กœ ๋ฏธ๋ž˜ 20๋…„ ๋™์•ˆ ๊ณผํ•™์˜ ์ค‘์š”์„ฑ์„ ๊ฐ•์กฐํ•˜๊ณ  ์žˆ๋‹ค. ํŠน

Physics HEP-PH
No Image

Properties of proper rational numbers

Catchy Title KO: ์œ ๋ฆฌ์ˆ˜์˜ ํ•ฉ์„ฑ๊ณผ ๊ณฑ์…ˆ: ์ง„๋ถ„์ˆ˜์™€ ์ •์ˆ˜์˜ ๊ด€๊ณ„ ํƒ๊ตฌ Abstract KO: ์ด ๋…ผ๋ฌธ์—์„œ๋Š” ์ •์ˆ˜์™€ ๋‹ค๋ฅธ ์œ ๋ฆฌ์ˆ˜, ํŠนํžˆ ์ง„๋ถ„์ˆ˜์˜ ํŠน์„ฑ์„ ๋ถ„์„ํ•˜๊ธฐ ์œ„ํ•ด ํ•ฉ์„ฑ๊ณผ ๊ณฑ์…ˆ ์—ฐ์‚ฐ์— ๋Œ€ํ•œ ์ด๋ถ„๋ฒ•์  ์ ‘๊ทผ์„ ์‚ฌ์šฉํ•œ๋‹ค. ์ฃผ์š” ๊ฐœ๋…์œผ๋กœ๋Š” ์œ ๋ฆฌ์ˆ˜ ์ง‘ํ•ฉ, ์ง„๋ถ„์ˆ˜์˜ ์ •์˜ ๋ฐ ํ‘œํ˜„ ๋ฐฉ๋ฒ• ๋“ฑ์ด ํฌํ•จ๋œ๋‹ค. ๋…ผ๋ฌธ์€ ์ง„๋ถ„์ˆ˜์™€ ์ •์ˆ˜์˜ ํ•ฉ๊ณผ ๊ณฑ์— ๋Œ€ํ•œ ๋ช‡ ๊ฐ€์ง€ ์ค‘์š”ํ•œ ์ •๋ฆฌ๋ฅผ ์ œ์‹œํ•˜๋ฉฐ, ํŠนํžˆ ๋‘ ์ง„๋ถ„์ˆ˜์˜ ํ•ฉ ๋˜๋Š” ๊ณฑ์ด ์ •์ˆ˜๊ฐ€ ๋˜๋Š” ์กฐ๊ฑด์„ ํƒ๊ตฌํ•œ๋‹ค. ๋งˆ์ง€๋ง‰์œผ๋กœ, ๋‘ ์œ ๋ฆฌ์ˆ˜์˜ ํ•ฉ๊ณผ ๊ณฑ ๋ชจ๋‘๊ฐ€ ์ •์ˆ˜์ธ ๊ฒฝ์šฐ ๊ทธ ๋‘ ์œ ๋ฆฌ์ˆ˜ ์—ญ์‹œ ์ •์ˆ˜๋ผ๋Š” ๊ฒฐ๋ก ์— ๋„๋‹ฌํ•œ๋‹ค.

Mathematics
A Statistical Significance Simulation Study for the General Scientist

A Statistical Significance Simulation Study for the General Scientist

1. ์—ฐ๊ตฌ ๋ฐฐ๊ฒฝ ๋ฐ ๋ชฉ์  ํ†ต๊ณ„์  ์œ ์˜์„ฑ์€ ๊ณผํ•™์ž๋“ค์ด ์ž์‹ ์˜ ์‹คํ—˜ ๊ฒฐ๊ณผ๋ฅผ ๊ฒ€์ฆํ•˜๋Š” ๋ฐ ์ค‘์š”ํ•œ ์—ญํ• ์„ ํ•˜๋Š”๋ฐ, ์ด๋Š” ๊ด€์ฐฐ๋œ ์ฐจ์ด๊ฐ€ ์šฐ์—ฐํžˆ ๋ฐœ์ƒํ•œ ๊ฒƒ์ผ ๊ฐ€๋Šฅ์„ฑ์ด ๋งค์šฐ ๋‚ฎ๋‹ค๋Š” ๊ฒƒ์„ ์˜๋ฏธํ•œ๋‹ค. ์ผ๋ฐ˜์ ์œผ๋กœ p ๊ฐ’์ด 0.05 ๋ฏธ๋งŒ์ธ ๊ฒฝ์šฐ ํ†ต๊ณ„์  ์œ ์˜์„ฑ์„ ์ธ์ •ํ•œ๋‹ค. ๊ทธ๋Ÿฌ๋‚˜ ๋ณธ ๋…ผ๋ฌธ์€ ํ‘œ๋ณธ ์ˆ˜๊ฐ€ ์ฆ๊ฐ€ํ•จ์— ๋”ฐ๋ผ ๋‘ ๊ทธ๋ฃน ๊ฐ„์˜ ์ฐจ์ด๊ฐ€ ํ†ต๊ณ„์ ์œผ๋กœ ์œ ์˜๋ฏธํ•˜๊ฒŒ ์ž‘์•„์ง€๋Š” ํ˜„์ƒ์„ ๋ถ„์„ํ•˜๊ณ , ์ด๋กœ ์ธํ•ด p ๊ฐ’ ์ž„๊ณ„์น˜(p<0.05)๋ฅผ ์‚ฌ์šฉํ•˜๋Š” ๊ฒƒ์ด ๊ณผํ•™์ž๋“ค์—๊ฒŒ ๋งค์šฐ ๋‚ฎ์€ ๊ธฐ์ค€์„ ์„ค์ •ํ•œ๋‹ค๋Š” ๊ฒƒ์„ ์ง€์ ํ•œ๋‹ค. 2. ์—ฐ๊ตฌ ๋ฐฉ๋ฒ• ๋ณธ ๋…ผ๋ฌธ์—์„œ๋Š” ๋‘ ์ƒ˜ํ”Œ t ๊ฒ€์ •์„ ์‚ฌ์šฉํ•˜์—ฌ

Statistics Applications Physics
Astrophysical consequences of the OPERA superluminal neutrino

Astrophysical consequences of the OPERA superluminal neutrino

: OPERA ์‹คํ—˜์€ ์ค‘์„ฑ๋ฏธ์ž๊ฐ€ ๋น›๋ณด๋‹ค ๋” ๋น ๋ฅด๊ฒŒ ์ด๋™ํ•  ์ˆ˜ ์žˆ๋‹ค๋Š” ๊ฒฐ๊ณผ๋ฅผ ๋ฐœํ‘œํ•˜๋ฉด์„œ ๊ณผํ•™๊ณ„์— ํฐ ์ถฉ๊ฒฉ์„ ์ฃผ์—ˆ๋‹ค. ์ด๋Š” ๋กœ๋ Œ์ธ  ๋Œ€์นญ์„ฑ ์œ„๋ฐ˜(LSV)์˜ ๊ฐ€๋Šฅ์„ฑ์„ ์‹œ์‚ฌํ•˜๋ฉฐ, ๊ธฐ์กด ๋ฌผ๋ฆฌํ•™ ์›์น™๊ณผ ์ƒ์ถฉ๋˜๋Š” ๊ฒฐ๊ณผ๋กœ ์ธํ•ด ๋งŽ์€ ๋…ผ๋ž€์ด ์ผ์–ด๋‚ฌ๋‹ค. 1. ์ค‘์„ฑ๋ฏธ์ž์˜ ์ดˆ๊ด‘์† ์‹ ํ˜ธ์™€ ์ฒœ์ฒด๋ฌผ๋ฆฌํ•™์  ์ œ์•ฝ OPERA ์‹คํ—˜์—์„œ ๊ด€์ฐฐ๋œ ์ค‘์„ฑ๋ฏธ์ž ์‹ ํ˜ธ๋Š” ๋น›์˜ ์†๋„๋ณด๋‹ค ์•ฝ๊ฐ„ ๋” ๋น ๋ฅด๊ฒŒ ์ด๋™ํ•˜๋Š” ๊ฒƒ์œผ๋กœ ๋‚˜ํƒ€๋‚ฌ๋‹ค. ์ด๋Ÿฌํ•œ ๊ฒฐ๊ณผ๋Š” ์ง„๊ณต์—์„œ ์ค‘์„ฑ๋ฏธ์ž์˜ ๋น„ํŒ์†์ด ๋น›์˜ ์†๋ ฅ๋ณด๋‹ค ํฌ๋‹ค๋Š” ๊ฒƒ์„ ์˜๋ฏธํ•œ๋‹ค. ๊ทธ๋Ÿฌ๋‚˜, ์ด ๊ฒฐ๊ณผ๋Š” ์ฒœ์ฒด๋ฌผ๋ฆฌํ•™์  ๊ด€์ธก๊ณผ ์ƒ์ถฉ๋˜๋Š” ๋ฌธ์ œ๋ฅผ ์•ผ๊ธฐํ•œ๋‹ค. ํŠนํžˆ,

HEP-PH Astrophysics Physics

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