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標題 [新聞] CNN:新數據顯示神秘暗能量正在演變
時間 Thu Apr  3 04:01:58 2025


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1.媒體來源:
CNN Science

2.記者署名:
Ashley Strickland, CNN


3.完整新聞標題:
‘Another mind-blowing change’: New data suggests mysterious dark energy is
evolving


4.完整新聞內文:
Updated 10:06 AM EDT, Wed April 2, 2025

New hints from one of the most extensive surveys of the cosmos to date suggest
 that mysterious dark energy may be evolving in ways that could shift how
astronomers understand the universe.

Dark energy is a term scientists use to describe an energy or force that
accelerates the expansion of the universe. But — although it represents 70%
of the energy in the cosmos — researchers still have no idea exactly what
dark energy is, said Mustapha Ishak-Boushaki, professor of physics and
astrophysics at the University of Texas at Dallas.

Ishak-Boushaki is a cochair of a working group for the Dark Energy
Spectroscopic Instrumentcollaboration, known as DESI. The instrument, now in
 its fourth year of surveying the sky, can observe light from 5,000 galaxies
at the same time. When the project concludes next year, it will have measured
the light of about 50 million galaxies.

The collaboration, which includes more than 900 researchers, shared the latest
 data release from DESI’s first three years of observations on March 19.
Among its findings are the measurements of nearly 15 million galaxies and
quasars, some of the brightest objects in the universe. Ishak-Boushak helped
lead the analysis of the latest DESI data release, which suggests that dark
energy — long called a “cosmological constant” given that astronomers
thought it was unchanging — is behaving in unexpected ways and may even be
weakening over time.

“The discovery of dark energy, nearly 30 years ago, was already the biggest
surprise of my scientific lifetime,” saidDavid Weinberg,a professor of
astronomy at The Ohio State Universitywho contributed to the DESI analysis,
in a statement. “These new measurements offer the strongest evidence so far
that dark energy evolves, which would be another mind-blowing change to our
understanding of how the universe works.”

The findings bring astronomers another step closer to unmasking the mysterious
 nature of dark energy, which may mean that the standard model of how the
universe works could also require an update, scientists say.

A deep look at the universe
The Dark Energy Spectroscopic Instrumentis atop the National Science
Foundation’s Nicholas U. Mayall 4-meter Telescope at Kitt Peak National
Observatory in Tucson, Arizona. The instrument’s 5,000 fiber-optic “eyes”
and extensive surveying capabilities are enabling scientists to build one of
the largest 3D maps of the universe and track how dark energy has influenced
and shaped the cosmos over the past 11 billion years.

It takes time for the light from celestial objects like galaxies to travel to
Earth, which means that DESI can effectively see what the cosmos was like at
different points in time, from billions of years ago to the present.

“DESI is unlike any other machine in terms of its ability to observe
independent objects simultaneously,” said John Moustakas, a professor of
physics at Siena College and colead of the data release.

The newest findings include data on more than double the cosmic objects that
were surveyed and presented less than a year ago. Those 2024 revelations first
 hinted at how dark energy may be evolving.

“We’re in the business of letting the universe tell us how it works, and
maybe the universe is telling us it’s more complicated than we thought it was
,” said Andrei Cuceu, a postdoctoral researcher at the US Department of
Energy’s Lawrence Berkeley National Laboratory, which manages DESI,and
cochair of DESI’s Lyman-alpha working group, in a statement. “It’s
interesting and gives us more confidence to see that many different lines of
evidence are pointing in the same direction.”

Mounting cosmic evidence
DESI can measure what scientists call the baryon acoustic oscillation, or BAO,
 scale — essentially how events that occurred early in the universe left
behind patterns in how matter is distributed across the cosmos. Astronomers
look to the BAO scale, with separations of matter by about 480 million light-
years, as a standard ruler.

“This separation scale is like a really gigantic ruler in space that we can
use to measure distances, and we use the combination of these distance and
redshifts (speed objects are moving away from us) to measure the expansion of
the universe,” said Paul Martini, a coordinator of the analysis and professor
 of astronomy at The Ohio State University.

Measuring dark energy’s influence across the history of the universe shows
how dominant a force it has been.

Researchers began to notice when they combined these observations with other
measurements of light across the universe such as exploding stars, the gravity
-warped light of distant galaxies, and the light leftover from the dawn of the
 universe, called the cosmic microwave background, the DESI data shows that
dark energy’s impact could be weakening over time.

“If this continues then eventually dark energy will not be the dominant force
 in the universe,” Ishak-Boushak said in an email. “Therefore the universe
expansion will stop accelerating and will go at a constant rate or even in
some models could also stop and collapse back. Of course, these futures are
very remote and will take billions and billions of years to happen. I’ve
worked on the question of cosmic acceleration for 25 years, and my perspective
 is, if the evidence continues to grow, and it is likely to, then this will be
 huge for cosmology and all of physics.”

Solving an enduring mystery
There isn’t enough evidence yet to declare a groundbreaking discovery that
definitively says dark energy is evolving and weakening, but that could change
 within just a couple of years, Ishak-Boushak said.

“My first big question is if we will continue to see evidence for evolving
dark energy as our measurements get better and better,” Martini said. “If we
 do get to the point where the evidence is overwhelming, then my next
questions will be: How does dark energy evolve? And what are the most likely
physical explanations?”

The new data release could also help astrophysicists better understand how
galaxies and black holes evolve and the nature of dark matter. Although dark
matter has never been detected, it is believed to make up 85% of the total
matter in the universe.

Scientists involved with the collaboration are eager to improve their
measurements using DESI.

“Whatever the nature of dark energy is, it will shape the future of our
universe,” said Michael Levi, DESI director and a scientist at the Lawrence
Berkeley National Laboratory. “It’s pretty remarkable that we can look up at
 the sky with our telescopes and try to answer one of the biggest questions
that humanity has ever asked.”

A new experiment called Spec-S5, or Stage 5 Spectroscopic Experiment, could
measure more than 10 times as many galaxies as DESI to study both dark energy
and dark matter, Martini said.

“Spec-S5 would use telescopes in both the northern and southern hemispheres
to map galaxies across the entire sky,” Martini said. “We are also excited
about how the (Vera) Rubin telescope will study supernovae, and provide a new,
 uniform dataset to study the (universe’s) expansion history.”

Other space observatories, like the Euclid space telescope and the Nancy Grace
 Roman Space Telescope, set to launch in 2027, will also contribute more key
measurements of dark matter and dark energy in the coming years that could
help fill in the gaps, said Jason Rhodes, an observational cosmologist at NASA
’s Jet Propulsion Laboratory in Pasadena, California. Rhodes, who is not
involved in DESI, is the US science lead for Euclid and principal investigator
 for NASA’s Euclid dark energy science team.

Rhodes, who calls the results intriguing, said the data shows a slight but
persistent tension between measurements from the early days of the universe
and those from the later universe.

“(This means) that our simplest model of dark energy doesn’t quite allow for
 the early universe we observe to evolve into the late universe we observe,”
Rhodes said. “DESI results (and some other recent results) seem to indicate
that a more complex model of dark energy is preferred.This is truly exciting
 because it may mean that new, unknown, physics governs the evolution of the
universe. DESI has given us tantalizing results that may indicate a new model
of cosmology is needed.”

中文翻譯:

「另一個令人震驚的變化」:新數據顯示神秘暗能量正在演變

這是迄今為止最廣泛的宇宙調查之一,它提供的新線索表明,神秘的暗能量可能正在以某
種方式演變,從而改變天文學家對宇宙的理解。

暗能量是科學家用來描述加速宇宙膨脹的能量或力量的術語。然而,德州大學達拉斯分校
物理學和天文物理學教授穆斯塔法· 伊沙克-布沙基說,儘管暗能量佔宇宙能量的 70%,
但研究人員仍然不知道暗能量到底是什麼。


Ishak-Boushaki 是暗能量光譜儀合作工作小組(DESI)的共同主席。該儀器目前已進入
天空勘測的第四年,可以同時觀測 5,000 個星系的光。當該計畫明年結束時,它將測量
大約 5000 萬個星系的光。


該合作計畫由 900 多名研究人員組成,於 3 月 19 日分享了DESI 前三年觀測的最新數
據。其發現包括對近 1500 萬個星系和類星體的測量,這些星系和類星體是宇宙中最亮的
物體之一。 Ishak-Boushak 幫助領導了最新 DESI 數據發布的分析,該分析表明,暗能
量——長期以來被稱為“宇宙常數”,因為天文學家認為它是不變的——正在以意想不到
的方式表現,甚至可能隨著時間的推移而減弱。


參與 DESI 分析的俄亥俄州立大學天文學教授戴維· 溫伯格在一份聲明中表示:“近 30
年前發現的暗能量已經是我科學生涯中最大的驚喜了。” “這些新測量結果提供了迄今
為止暗能量演化的最有力證據,這將再次極大地改變我們對宇宙運作方式的理解。”


科學家表示,這項發現使天文學家距離揭開暗能量的神秘本質又更近了一步,這可能意味
著宇宙運作的標準模型也需要更新。

深入觀察宇宙
暗能量光譜儀位於亞利桑那州圖森市基特峰國家天文台的國家科學基金會尼古拉斯· U·
梅耶爾 4 公尺望遠鏡的頂部。該儀器的 5,000 個光纖「眼睛」和廣泛的測量能力使科學
家能夠建立最大的宇宙 3D 地圖之一,並追蹤暗能量在過去 110 億年中如何影響和塑造
宇宙。


來自星係等天體的光需要時間才能到達地球,這意味著 DESI 可以有效地看到從數十億年
前到現在不同時間點的宇宙狀況。

「DESI 與其他機器不同,它能夠同時觀察獨立物體,」錫耶納學院物理學教授、數據發
布的共同負責人約翰· 穆斯塔卡斯 (John Moustakas) 說。

最新發現涵蓋的宇宙物體數據比不到一年前調查和呈現的數據多了一倍多。 2024 年的啟
示首次暗示了暗能量可能如何演變。

美國能源部勞倫斯伯克利國家實驗室(負責管理 DESI)的博士後研究員、DESI 萊曼-α
工作組聯合主席安德烈· 庫塞烏 (Andrei Cuceu) 在一份聲明中表示:“我們的工作是讓
宇宙告訴我們它是如何運轉的,也許宇宙告訴我們它比我們想像的要復雜得多。” “這
很有趣,讓我們看到許多方向的證據”。


越來越多的宇宙證據
DESI 可以測量科學家所稱的重子聲學振盪(BAO)尺度——本質上是宇宙早期發生的事件
如何留下物質在整個宇宙中分佈的模式。天文學家以 BAO 尺度為標準標尺,物質之間的
距離約為 4.8 億光年。


「這個分離尺度就像是太空中一把巨大的尺子,我們可以用它來測量距離,並利用這些距
離和紅移(物體遠離我們的速度)的組合來測量宇宙的膨脹,」分析協調員、俄亥俄州立
大學天文學教授保羅馬蒂尼說。


測量暗能量在宇宙歷史中的影響可以顯示它是多麼強大的力量。

研究人員開始注意到,當他們將這些觀測結果與宇宙中其他光的測量結果(如爆炸的恆星
、遙遠星系的引力扭曲光以及宇宙黎明時遺留下來的光(稱為宇宙微波背景))相結合時
,DESI 數據顯示暗能量的影響可能隨著時間的推移而減弱。


伊沙克-布希克在一封電子郵件中表示:「如果這種情況持續下去,那麼暗能量最終將不
再是宇宙的主導力量。」「因此,宇宙膨脹將停止加速,並以恆定的速度發展,甚至在某
些模型中也可能停止並坍縮。當然,這些未來非常遙遠,需要數十億年才能實現。我已經
研究宇宙加速問題 25 年了,我的觀點是整個物理學,如果整個物理學,如果這對宇宙學
的證據都很有證據。


解開一個持久的謎團
伊沙克-布希克表示,目前還沒有足夠的證據來宣布一項突破性的發現,明確表明暗能量
正在演變和減弱,但這種情況可能會在短短幾年內改變。

馬蒂尼說:“我的第一個大疑問是,隨著我們的測量技術越來越精確,我們是否會繼續看
到暗能量演變的證據。” “如果我們真的找到了壓倒性的證據,那麼我的下一個問題將
是:暗能量是如何演化的?最有可能的物理解釋是什麼?”


新發布的數據還可以幫助天文物理學家更好地理解星系和黑洞如何演化以及暗物質 的性
質。儘管暗物質從未被偵測到,但人們認為它佔宇宙中總物質的85%。

參與合作的科學家們渴望利用 DESI 來改進他們的測量方法。

「無論暗能量的性質是什麼,它都會塑造我們宇宙的未來,」DESI 主任、勞倫斯伯克利
國家實驗室的科學家邁克爾· 萊維說。 “我們能夠用望遠鏡仰望天空,並試圖解答人類
有史以來最大的問題之一,這真是太了不起了。”


馬蒂尼表示,一項名為 Spec-S5(第五階段光譜實驗)的新實驗可以測量比 DESI 多 10
倍的星系,以研究暗能量和暗物質。

馬蒂尼說:“Spec-S5 將使用北半球和南半球的望遠鏡繪製整個天空的星系圖。” “我
們也對(維拉)魯賓望遠鏡如何研究超新星感到興奮,並為研究(宇宙的)擴張歷史提供
新的、統一的數據集。”


美國太空總署加州帕薩迪納噴射推進實驗室的觀測宇宙學家傑森· 羅德斯說,其他太空觀
測站,如歐幾里德太空望遠鏡和南希· 格雷斯· 羅曼太空望遠鏡,也將在未來幾年對暗物
質和暗能量進行更多關鍵測量,這可能有助於填補空白。歐幾里德太空望遠鏡和南希· 格
雷斯· 羅曼太空望遠鏡將於 2027 年發射。羅茲沒有參與 DESI,但他是歐幾里德的美國
科學負責人,也是美國太空總署歐幾里德暗能量科學團隊的首席研究員。


羅德斯稱這些結果非常有趣,他表示數據顯示,對宇宙早期和晚期的測量結果之間存在輕
微但持續的矛盾。

「(這意味著)我們最簡單的暗能量模型並不能完全解釋我們觀察到的早期宇宙演化成我
們觀察到的晚期宇宙,」羅德斯說。 「DESI 的結果(以及其他一些近期結果)似乎表明
,更複雜的暗能量模型更受歡迎。這確實令人興奮,因為它可能意味著新的、未知的物理
學控制著宇宙的演化。DESI 為我們提供了誘人的結果,可能表明需要一種新的宇宙學模
型。”


5.完整新聞連結 (或短網址)不可用YAHOO、LINE、MSN等轉載媒體:
https://edition.cnn.com/2025/04/02/science/desi-dark-energy-results/index.html
Unexpected dark energy finding may change our understanding of the universe | CNN
[圖]
New observations of the cosmos show that the dark energy, a mysterious force that accelerates the expansion of the universe, is evolving. ...

 


6.備註:
美國科學家使用暗能量光譜儀(DESI)繪製宇宙最大3D地圖,未來將更精確測量宇宙歷史


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